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SURFACE INTERMEDIATES, MECHANISM AND REACTIVITY OF SOOT OXIDATION By Shazam Williams A thesis submitted in conformity with the requirements for the degree of Doctor of Philosophy Department of Chemical Engineering and Applied Chemistry University of Toronto © Copyright by Shazam Williams 2008

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Page 1: Fundamentals of Soot Oxidation Master Test 2 · PDF fileof soot oxidation Shazam Williams ... Where dC = moles of carbon ... Ro,SIMS is the rate of ion x of the ToFSIMS data using

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SURFACE INTERMEDIATES, MECHANISM AND REACTIVITY OF SOOT OXIDATION

By

Shazam Williams

A thesis submitted in conformity with the requirements for the degree of Doctor of Philosophy

Department of Chemical Engineering and Applied Chemistry University of Toronto

© Copyright by Shazam Williams 2008

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Surface intermediates, mechanism, and reactivity

of soot oxidation Shazam Williams

Doctor of Philosophy

Department of Chemical Engineering and Applied Chemistry,

University of Toronto

2008

Abstract

Factors that may govern diesel particulate matter (DPM) oxidation at low temperatures

(~200°C) were studied using reactivity and TP-ToFSIMS analysis. Best-case scenarios that

give maximum gasification rates were determined for DPM impregnated with KOH and non-

catalyzed DPM using temperature programmed oxidation and isothermal experiments.

Conditions of intimate catalyst-carbon contact (K/C molar ratio=1/50) and high NO2

concentrations (1%) to improve the reactivity of the carbon reactive sites were unable to meet

the steady state gasification rate needed for particulate filter regeneration for a modern diesel

engine at 200°C. Oxygen-free thermal annealing (>500°C) caused reactivity losses of a

maximum of 40% that correspond to changes to surface morphology and/or concentration of

oxygen-containing functional groups.

TP-ToFSIMS identified surface functional group changes with temperature on non-dosed and

NOX pre-dosed (1.5%NO, 1%NO2, 4.5%O2, balance helium) diesel soot and sucrose char.

Detailed analysis of the NOX dosed sucrose char spectra using both inspection and principal

component analysis techniques revealed that the 1200 ion fragments created could be reduced

to five sets of ions that are chemically and kinetically distinct. These sets presumably

represent surface functional groups on the carbon. For example, Set IV may represent

carboxylic acid, lactone, or carboxylic anhydride functional groups. Based on these results a

mechanism for the surface reaction of NO2 with carbon under vacuum conditions was

postulated. At temperatures less than 200°C the ion fragments contain primarily carbon-NO2

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type ions. As temperature increases between 200 and 400°C the ion fragments are primarily

carbon-NO and carbon-N type fragments. At higher temperatures (>500°C) the surface is

enriched with nitrogen containing functional groups. A surface reaction mechanism is

proposed where NO2 is bonded to an armchair site and with increasing temperatures and

molecular rearrangements the N is incorporated into the carbon ring. The initial surface

composition of NOx containing functional groups changes within the area of relevance of low

temperature soot regeneration (i.e. between 25° and 200°C). Further studies are needed to

understand the effect of N-incorporation on carbon reactivity. No rate processes either in

reactor studies or based on surface functional groups met the rate criteria for low temperature

DPM oxidation.

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Acknowledgements There are many people who have played important roles in my journey to complete this thesis.

The most influential is Prof. Charles Mims, who has always been a great mentor, instructor and

a friend over the many years that I have known him. And yes Chuck, now I do believe that I

have made a significant contribution.

It is true that a good thesis is not possible without an outstanding committee. My sincere

thanks to my committee members – Prof. Greg Evans, Prof. Jim Wallace, Prof. Charles Jia,

Prof. Jane Phillips, and Prof. Brian Haynes – for their excellent feedbacks, comments on the

thesis and their valuable time. Special thanks go to Prof. Phillips for her mentoring and

instruction since my bachelor degree years.

This journey would not have begun without the encouragement and support of Mr. George

Swiatek, his wife Eva, John Muter and my many colleagues at DCL International Inc. Thank

you, George, for having the confidence in me.

Thanks to Peter Broderson, Chris Bertole, Vik Pandit, Tom Wood, Cassie Liu and Naim

Ghany, for the support and the discussions during this time.

Thank you to my family, Mom, Dad, grandparents, Kevin, Carissa, Sheri, Jay, Kris, Josh,

Brianna and many friends for their support. Finally, my fiancée Josephine, her constant smile

and encouragement have made the journey enjoyable.

Financial support of this research was provided by DCL International Inc. and NSERC.

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Nomenclature

A is the frequency factor

Ao is the frequency factor at a fractional conversion of 10%

CAT – Soot collected from a Caterpillar 3306 engine

CO – Carbon monoxide

CO2 – Carbon dioxide

CS - Total quantity of carbon in the filter or reactor

DPF – Diesel Particulate Filter

DPM – Diesel Particulate Matter

DRIFTS- Diffuse Reflectance Infrared Fourier Transform Spectroscopy

fc – Fractional conversion of carbon

fs = carbonsites (site density)

FID – Flame Ionization Detector

FTIR – Fourier Transform InfraRed spectroscopy

GC – Gas Chromatography

HRTEM – High Resolution Transmission Electron Microscopy

IR – InfraRed spectroscopy

k - represents the TOF of single ion from ToFSIMS data using the differential analysis method.

k0.1 represents the gasification rate of a single ion based on TOF values or k values calculated

from ToFSIMS data using the differential analysis method.

K- Potassium based catalyst

K/C – Potassium to carbon ratio

ntj = total of all atoms in the ion j

nxj represents the number of atoms of element x in ion j

N(x)T – Normalized intensity ratio of component x used in ToFSIMS experiments

Na – Sodium based catalyst

NIST – National Institute of Science and Technology

NIST-ANN – Soot sample from NIST annealed in an inert atmosphere

NIST-0 – Soot sample from NIST as-is

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NO – Nitrogen monoxide

NO2 – Nitrogen dioxide

NOx – Nitrogen oxides, a mixture of nitrogen monoxide and nitrogen dioxide

ri, sims – represents the microscopic gasification rate or TOF of single ion based on the integral

analysis of the ToFSIMS data.

ri, sims (average) - is the microscopic gasification rate of an ion group (Set) based on the integral

analysis of the ToFSIMS data

rg, sims - is the gasification rate of a given ion group based on the integral analysis of the

ToFSIMS data

Rfco is the rate of carbon gasification at a fractional conversion of 10%

RG – Macroscopic gasification rate

RGo – Macroscopic gasification rate under steady state conditions where mass of carbon in

filter or reactor system is not varying.

Ro,SIMS is the rate of ion x of the ToFSIMS data using the integral analysis method

S – reactive sites on carbon

SC_NOX- Sucrose char exposed to nitrogen oxides

SC-AIR – Sucrose char exposed to air

SIMS – Secondary Ion Mass Spectroscopy

SOF – Soluble Organic Fraction

ta – time of acquisition of ToFSIMS spectra

tr- time to temperature ramp heated stage from one temperature to another during ToFSIMS

experiments

ts – time to stabilze the vacuum pressure in the ToFSIMS equipment

th- time of operator interruptions during ToFSIMS experiments

tann - Time that carbon was annealed in an inert atmosphere

TEM – Transmission Electron Microscopy

Tfc – Temperature to reach a given fractional conversion of carbon during TPO

TGA – Thermal Gravimetric Analysis

TPR – Temperature Programmed Reaction

TPD – Temperature Programmed Desorption

TOFG –Turn over frequency or microscopic gasification rate of a reactive site

ToFSIMS – Time of Flight Secondary Ion Mass Spectroscopy

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TP-ToFSIMS – Temperature Programmed Time of Flight Secondary Ion Mass Spectroscopy

XPS – X-ray Photoelectron Spectroscopy

yxj = atomic ratio of element x in ion j defined as yxj = nxj/ntj, where ntj = total of all atoms in

the ion j, nxj represents the number of atoms of element x in ion j

Reactivity terminology

RG - macroscopic gasification rate is defined as:

SG Cdt

dCR 1•−= (1/time = 1/h)

Where dC = moles of carbon reacted, CS = total quantity of carbon in the filter or reactor and, t

= time.

Microscopic reactivity rate – single site

RG = TOFG * S/C Where S/C is the number of reactive sites per total carbon in the system. Microscopic reactivity rate – multiple sites

RG = ∑(TOFG, i * Si/C) Where, subscript, i, represents a single reactivity type TOFG - Turnover frequency or microscopic reactivity rate

SdtdCTOFG

1•−= (mol/time *1/site) (h-1)

Here, dC = moles of carbon reacted, S is the number of carbon reactive sites, and dt is time of reaction yxj = atomic ratio of element x in ion j defined as yxj = nxj/ntj, where ntj = total of all atoms in the ion j, nxj represents the number of atoms of element x in ion j yx sample @ T is the mole fraction of a given element (x) in the complete spectrum at a single temperature

yx sample @ T = [Σ (Ij @ T * yxj)]/ I total @ T

Itotal @ T = Σ Ij @ T

where Ij @ T is the ion intensity of ion j at the specified temperature, T, and I total is the sum of all ion intensities at temperature T

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N(x)T – Normalized intensity ratio of component x used in ToFSIMS experiments is defined as

)()(

2)( −=

CIxIxN T

where, I(x) = intensity of component x at T, I(C2-) = intensity of C2

- ion at T, N = normalized intensity of ion x at temperature T Ro,SIMS is the rate of ion x of the ToFSIMS data using the integral analysis method

Ro,SIMS25

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N(x) *t N(x) - N(x)

=Δ=

T

TT

where , ∆t is the difference between the time of the start of the acquisition and the end of the acquisition. k - represents the TOF of single ion from ToFSIMS data using the differential analysis method.

k (1/h) = Δ N(x)/Δ t *1/N(x)o = slope/y-intercept Where N(x)o is the normalized intensity at time = 0.

k0.1 represents the gasification rate of a single ion based on TOF values calculated from ToFSIMS data using the differential analysis method.

k0.1(1/h) = k * sites/C where sites/C = 0.1 ri, sims represents the microscopic gasification rate or TOF of single ion based on the integral analysis of the ToFSIMS data.

ri, sims = a

i

NdtdN 1

ri, sims (average) is the microscopic gasification rate of an ion group (Set) based on the integral analysis of the ToFSIMS data.

ri, sims (average) = set

ions

ionsimsi

n

r∑ ,

rg, sims is the gasification rate of a given ion group based on the integral analysis of the ToFSIMS data

rg, sims = - simsir , (average) * fs

where fs = carbonsites (site density)

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Table of Contents Abstract..................................................................................................................................... ii

Acknowledgements...................................................................................................................iv

Nomenclature.............................................................................................................................v

Reactivity terminology ........................................................................................................... vii

Table of Contents......................................................................................................................ix

List of Figures...........................................................................................................................xi

List of Tables ...........................................................................................................................xv

1 Motivation/Overview.........................................................................................................1

1.1 Motivation..............................................................................................................1 1.2 Overview................................................................................................................4

1.2.1 Research Objectives.......................................................................................4 1.2.2 Thesis Structure .............................................................................................4

2 Background........................................................................................................................5

2.1 Fundamental understanding of carbon oxidation ..................................................5 2.1.1 Carbon structure.............................................................................................5 2.1.2 Identification of surface functional groups....................................................9 2.1.3 Carbon reaction mechanism ........................................................................11 2.1.4 Active Sites..................................................................................................12 2.1.5 Oxidant effects.............................................................................................13 2.1.6 Structural effects on soot oxidation .............................................................19 2.1.7 Catalyst effects.............................................................................................21

2.2 DPM filter technology and state of the art...........................................................24 2.2.1 Current legislation and technology..............................................................24 2.2.2 Relating fundamental kinetics to engineering targets..................................30

3 Experimental procedure for reactivity studies.................................................................35

3.1 Soot characterization and catalyst impregnation .................................................35 3.1.1 Materials ......................................................................................................35 3.1.2 Impregnation of carbon samples with catalyst precursors...........................36 3.1.3 Elemental characterization...........................................................................36 3.1.4 Spectroscopic characterization of soot ........................................................38

3.2 Reactivity studies.................................................................................................39 3.2.1 Reactor system.............................................................................................39 3.2.2 Reactor loading............................................................................................42 3.2.3 Data analysis ................................................................................................43

4 Reactivity Studies ............................................................................................................44

4.1 Introduction..........................................................................................................44 4.2 Overview: ............................................................................................................46 4.3 Published carbon reactivity studies .....................................................................46

4.3.1 Survey of literature carbon oxidation rates with NOX.................................47

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4.3.2 Temperature Programmed Oxidation Experiments in O2 atmosphere (with and without catalyst)....................................................................................................51 4.3.3 Reaction testing of soot and catalyzed soot in NO2 atmosphere .................54 4.3.4 Thermal annealing (Isothermal experiments) O2 atmosphere ....................56 4.3.5 Temperature Programmed Oxidation - Thermal Annealing Experiments ..66

4.4 Conclusion/Summary ..........................................................................................72 4.5 Future Work/Suggestions ....................................................................................73

5 ToFSIMS study of surface functional group reactivity ...................................................74

5.1 Introduction..........................................................................................................74 5.2 Experimental Procedure.......................................................................................78

5.2.1 Sample preparation and pre-treatment.........................................................78 5.2.2 TP ToFSIMS experiment description..........................................................79 5.2.3 ToFSIMS spectra, data calibration and peak assignment............................82 5.2.4 Data Analysis...............................................................................................84 5.2.5 Reference ions and relative intensities ........................................................86 5.2.6 Plan of data analysis ....................................................................................86

5.3 Results..................................................................................................................87 5.3.1 SIMS atomic composition change with temperature...................................87 5.3.2 SIMS elemental compositions of diesel soots .............................................90 5.3.3 General SIMS atomic change observations.................................................96 5.3.4 SIMS molecular fragment changes..............................................................97 5.3.5 Rate analyses of ion fragment data ............................................................106 5.3.6 Effect of temperature on individual ion sets, SC_NOX ............................130 5.3.7 Reactivities of surface ion precursors........................................................133 5.3.8 Surface mechanistic considerations...........................................................138

5.4 Conclusions........................................................................................................149 5.5 Recommendations for future work ....................................................................150

6 Conclusions and Recommendations ..............................................................................151

7 References......................................................................................................................154

8 Appendix Information ...................................................................................................180

8.1 Appendix A: Soot impregnation technique and procedure................................181 8.2 Appendix B: SEM photos..................................................................................190 8.3 Appendix C: Raman experimental procedure and results .................................193 8.4 Appendix D: PCA plots .....................................................................................201 8.5 Appendix E: Certification and specification sheets...........................................211

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List of Figures Figure 2.1.1: Oxygen containing functional groups on carbon .............................................6 Figure 2.1.2: Representation of hexane soot showing defects and distortions from Smith et

al. 18................................................................................................................................8 Figure 2.1.3: Marsh-Griffiths model of graphitisation from Marsh 22 ..................................8 Figure 2.1.4: Illustration of acidic and basic groups on carbon. 25 ......................................10 Figure 2.1.5: Carbon structure identifying zigzag and armchair sites .................................13 Figure 2.2.1: General comparison of on-road heavy-duty diesel (HDD) standards in the

US, Japan, and Europe. Estimated engine-out emissions for 2007 and 2010 (range) are shown. Steady-state cycle. 243 Reprinted with permission from SAE Paper# 2006-01-0030 © 2006 SAE International. ............................................................................25

Figure 2.2.2: Example of exhaust flow through wall flow filter .........................................26 Figure 2.2.3: Example of exhaust flow thorough (non-blocking) filter (DCL) 251 Reprinted

with permission from SAE Paper# 2007-01-4025 © 2007 SAE International............27 Figure 2.2.4: Base case gasification rate criteria .................................................................31 Figure 2.2.5: Example of gasification rate chart indicating desired reaction region...........32 Figure 3.2.1: Reactor system setup......................................................................................40 Figure 3.2.2: Example of FID calibration............................................................................40 Figure 3.2.3: Calculated FID flame chemistry limiting O2 cases ........................................41 Figure 3.2.4: Example of flow controller calibration ..........................................................43 Figure 4.3.1: Literature survey of gasification rate data for catalyzed carbon reaction with

NOX. Data normalized to total NOX values of 1000 ppm ..........................................50 Figure 4.3.2: Example of temperature programmed oxidation experiment. Sample NIST,

10% O2.........................................................................................................................51 Figure 4.3.3: Gasification rate plot with TPO O2 data: NIST soot and K-NIST (K/C mol

ratio = 1/50) compared to Yezerets et al. 2003 70, 2005 69 data; reaction conditions: 10% O2, 7000 h-1, ramp rate 5.8°C/min, Symbols with thin lines are literature values. Heavy lines represent thesis experimental data. ..........................................................53

Figure 4.3.4: Gasification rate plot with non-catalyzed and catalyzed NIST samples in O2 and NO2 atmospheres: Reaction conditions: Ramp rate: 5.8°C/min, 7000 h-1, O2 runs: 10% O2, NO2 runs: 4.5% O2, 1 % NO2, 4 % NO, K-NIST sample: K/C : 1/50 mol ratio, Na-NIST sample: Na/C : 1:50 mol ratio Symbols with thin line represent literature data. Heavy lines represent thesis experimental data. .................................56

Figure 4.3.5: Effect of isothermal thermal annealing: Reaction Temperature = 550°C, B1, B2: Base case- burnoff curves with 10% O2/He. T2: Step change in Oxygen concentration from 10% to 0%, Thermal annealed for 1 hour at 550°C with He only......................................................................................................................................61

Figure 4.3.6: Effect of in-situ high temperature annealing: Reaction Temperature = 550°C, B1, B2: Base case- burnoff curves with 10% O2/He. T2: Step change in Oxygen concentration from 10% to 0%, 1st Thermal anneal at 550°C for 1 hour and 2nd Thermal anneal at 700°C with He only. ......................................................................64

Figure 4.3.7: Effect of 200°C pre anneal and reaction with oxygen (T3): Temp2 = 550°C, B1, B2: Base case- burnoff curves with 10% O2/He. T2: Step change in Oxygen concentration from 10% to 0%, Thermal annealed for 1 hour at 700°C with He only. T3: Pre anneal at 200°C in He and then oxidation in O2. ............................................65

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Figure 4.3.8: Effect of Annealing time on Temperature for a specified fractional conversion, 5% NO2, 10% O2, Annealing Temperature: 700°C, Ramp rate: 5.8°C/min.....................................................................................................................................68

Figure 4.3.9: K impregnated NIST soot (Thermal Annealing) TPO Annealing T= 680°C, K/C mol ratio = 1:50....................................................................................................70

Figure 4.3.10: K impregnated Carbon (Thermal Annealing) TPO Annealing T= 680°C. Fractional Conversion versus RGo Plot ........................................................................71

Figure 4.3.11: Comparison of slopes of rate curves. Same conditions as Figure 4.3.9.......72 Figure 5.1.1: Functional groups on soot surface listed according to their thermal stability.

Acidity represents only the general trend. (Muckenhuber et al.35 )............................75 Figure 5.2.1: Timing events during typical TP ToFSIMS experiments, ta= acquisition time,

tr= ramp time, th = operator interruptions, ts= vacuum stabilization time....................81 Figure 5.2.2: Example of TP-ToFSIMS spectra for Negative Ions – Sample NIST-0,

Temperatures of spectra displayed: room temperature (~25 °C), 100 °C, 200 °C, 400 °C, and 550 °C. Y-axis: Intensity (log scale), X-axis: mass units (m/z, linear scale) 83

Figure 5.2.3: Effect of temperature on the intensity of each individual ion for sample SC_NOX negative ions. Panel A = high intensity, low molecular weight ions: Panel B = lower intensity, higher molecular weight ion intensities (unlabeled) to show variety of temperature dependent behaviour. ..........................................................................85

Figure 5.3.1: Elemental (C, H, O, N) SIMS spectral composition as a function of temperature for SC_NOX negative Ions......................................................................88

Figure 5.3.2: Elemental (C, H, O, N) SIMS spectral composition as a function of temperature for SC_AIR Negative Ions. .....................................................................88

Figure 5.3.3: Effect of NOX treatment on sucrose char. Difference in elemental mole fractions between NOX treated sucrose char (SC_NOX) and non-treated sucrose char (SC_AIR). Positive values indicate higher mole fractions in SC_NOX. Negative values indicate higher mole fractions in SC_AIR. ......................................................90

Figure 5.3.4: Elemental Composition Change (C, H, O, N) with Temperature of NIST-0 Negative Ions. ..............................................................................................................91

Figure 5.3.5: Elemental Composition Change (C, H, O, N) with Temperature of CAT-0 Negative Ions. ..............................................................................................................92

Figure 5.3.6: Elemental Composition Change (C, H, O, N) with Temperature of NIST-ANN Negative Ions. ....................................................................................................93

Figure 5.3.7: Effect of thermal annealing at 700 °C in He on NIST diesel soot. Difference in elemental mole fractions between non-treated NIST diesel soot (NIST-0) and thermally annealed NIST soot (NIST-ANN). Positive values indicate higher mole fractions in NIST-0. .....................................................................................................93

Figure 5.3.8: Difference in elemental mole fractions between NOX -treated sucrose char (SC_NOX) and non-treated NIST diesel soot (NIST-0). Positive values indicate higher mole fractions in SC_NOX. Negative values indicate higher mole fractions in NIST-0. ........................................................................................................................94

Figure 5.3.9: Difference in elemental mole fractions between non-treated NIST diesel soot (NIST-0) and CAT 3306 diesel soot (CAT-0). Positive values indicate higher mole fractions in NIST-0. Negative values indicate higher mole fractions in CAT-0. .......95

Figure 5.3.10: Example of identified peaks from TP- ToFSIMS data ................................99

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Figure 5.3.11: Effect of temperature on Individual Ion intensity ratio for each sample. (Intensity scale x100) where 0= NIST-0, 1= CAT-0, 2= NIST-ANN, 3= SC_NOX, 4= SC_AIR......................................................................................................................101

Figure 5.3.12: Effect of NOX exposure on sucrose char. Comparison of the CN- ion between SC_NOX and SC_AIR. ...............................................................................102

Figure 5.3.13: Effect of NOX exposure on sucrose char. Comparison of the CHNO- and C3NO- ion between SC_NOX and SC_AIR ..............................................................103

Figure 5.3.14: Change in nitrogen containing ions during temperature ramping, Nitrogen, oxygen, hydrogen and carbon containing ions only shown, where N=I(x)/I(C2

-), Sample: SC_NOX. The order of the ions in the figure is identical to the list in the right hand margin.......................................................................................................104

Figure 5.3.15: O depletion of C, H, O only containing ions during temperature ramping. Sample:(SC_NOX) The order of the ions in the figure is identical to the list in the right hand margin.......................................................................................................105

Figure 5.3.16 (a-d): Examples of positive and negative correlations for ion pairs of Integral rate versus Temperature. Units: h-1 panels (a,b): positive, panels (c,d): negative....108

Figure 5.3.17: Identified curve shapes for rate versus T plots grouped into Sets for sample SC_NOX. y-axis is rate, x-axis is temperature.........................................................110

Figure 5.3.18: Contribution of each integral rate set with Temperature, Top left: All Sets, Top right: Magnification of top fraction showing Sets II, III, and IV. No contribution from Set V. Bottom centre: Magnification of bottom fraction showing Sets I and II. Sample: SC_NOX......................................................................................................112

Figure 5.3.19: Time-dependent isothermal intensity changes in normalized intensity (CH- /C2

-) for CH- at 25°C for sample SC_NOX negative ions. Top (a): All data during data collection, Bottom (b): The same date averaged over 10 primary ion pulses...114

Figure 5.3.20: Effect of temperature on differential rates for CH-, NO-, CHN-, and CN- ions (Sample SC_NOX) ....................................................................................................117

Figure 5.3.21: Examples of positive (top panel) and negative (bottom panel) correlations for Sample (SC_NOX) negative ions. .......................................................................119

Figure 5.3.22: PCA Loading Plots for Sample SC_NOX negative ions: Loading plot (a) and Biplot (b) of PC1 versus PC2 (▼- scores, ♦ - loadings), Cumulative variance captured by each PC (c). Loading plots indicate identified sets within the ToFSIMS data.............................................................................................................................126

Figure 5.3.23: PCA Loading Plots for Sample SC_NOX positive ions: Loading plot (a) and Biplot (b) of PC1 versus PC2 (▼- scores, ♦ - loadings), Cumulative variance captured by each PC (c). Loading plots indicate identified groupings within the ToFSIMS data............................................................................................................128

Figure 5.3.24: PCA Loading Plots for Sample SC-AIR negative ions: Loading plot (a) and Biplot (b) of PC1 versus PC2 (▼- scores, ♦ - loadings), Cumulative variance captured by each PC (c). Loading plots indicate identified groupings within the ToFSIMS data.............................................................................................................................129

Figure 5.3.25: Top (a): Effect of temperature on the non-normalized intensity of each individual Set, Centre (b): Effect of temperature on the normalized Set intensity, Bottom (c): Surface conversion of each Set with temperature ..................................131

Figure 5.3.26: Effect of Temperature on the gasification rate for each ion Set leaving the carbon surface. Sample SC_NOX: NOX dosed sucrose char negative ions ..............135

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Figure 5.3.27: Specific gasification reaction rate of individual ions for sample SC_NOX. The lines are included to make it easier for the reader to locate the data points and are not intended to show trends. ......................................................................................137

Figure 5.3.28: Reaction Scheme 1 .....................................................................................139 Figure 5.3.29: Examples of NO2 bonding to carbon .........................................................146 Figure 5.3.30: Reaction Scheme 2 - Generalized surface reaction mechanism with NO2

bonding via nitrogen atom to the carbon surface.......................................................147 Figure 5.3.31: Reaction Scheme 3 - Generalized surface reaction mechanism of NO2

bonding via the oxygen atom to the carbon surface ..................................................148 Figure 8.1.1: Sample location for Image Experiment 1.....................................................183 Figure 8.1.2: Photo Images of Experiment 2 .....................................................................186 Figure 8.1.3: Photo Images of Experiment 1 .....................................................................187 Figure 8.2.1: Sucrose char .................................................................................................190 Figure 8.2.2: CAT diesel soot............................................................................................191 Figure 8.2.3: NIST diesel soot...........................................................................................192 Figure 8.3.1: Raman spectra of SCV3a x-axis: wavenumber, y axis: intensity, dots= data,

solid line fitted peaks .................................................................................................197 Figure 8.3.2: Raman Spectra of SCVM_4 x-axis: wavenumber, y axis: intensity, dots=

data, solid line fitted peaks ........................................................................................198 Figure 8.3.3: D/G peak ratios of Raman spectra ...............................................................200 Figure 8.4.1: PCA Loading Plots for Sample CAT-0 negative ions: Loading plot (a) and

Biplot (b) of PC1 versus PC2 (▼- scores, ♦ - loadings), Cumulative variance captured by each PC (c). Loading plots indicate identified groupings within the TOFSIMS data.............................................................................................................................201

Figure 8.4.2: PCA Loading Plots for Sample NIST-ANN negative ions: Loading plot (a) and Biplot (b) of PC1 versus PC2 (▼- scores, ♦ - loadings), Cumulative variance captured by each PC (c). Loading plots indicate identified groupings within the TOFSIMS data...........................................................................................................202

Figure 8.4.3: PCA Loading Plots for Sample SC_NOX negative ions: Loading plot (a) and Biplot (b) of PC1 versus PC2 (▼- scores, ♦ - loadings), Cumulative variance captured by each PC (c). Loading plots indicate identified groupings within the TOFSIMS data.............................................................................................................................203

Figure 8.4.4: PCA Loading Plots for Sample SC_AIR negative ions: Loading plot (a) and Biplot (b) of PC1 versus PC2 (▼- scores, ♦ - loadings), Cumulative variance captured by each PC (c). Loading plots indicates identified groupings within the TOFSIMS data.............................................................................................................................204

Figure 8.4.5: PCA Loading Plots for Sample NIST-0 negative ions: Loading plot (a) and Biplot (b) of PC1 versus PC2 (▼- scores, ♦ - loadings), Cumulative variance captured by each PC (c). Loading plots indicates identified groupings within the TOFSIMS data.............................................................................................................................205

Figure 8.4.6: PCA Loading Plots for Sample NIST-0 positive ions: Loading plot (a) and Biplot (b) of PC1 versus PC2 (▼- scores, ♦ - loadings), Cumulative variance captured by each PC (c). Loading plots indicate identified groupings within the TOFSIMS data.............................................................................................................................206

Figure 8.4.7: PCA Loading Plots for Sample CAT-0 positive ions: Loading plot (a) and Biplot (b) of PC1 versus PC2 (▼- scores, ♦ - loadings), Cumulative variance captured

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xv

by each PC (c). Loading plots indicate identified groupings within the TOFSIMS data.............................................................................................................................207

Figure 8.4.8: PCA Loading Plots for Sample NIST_ANN positive ions: Loading plot (a) and Biplot (b) of PC1 versus PC2 (▼- scores, ♦ - loadings), Cumulative variance captured by each PC (c). Loading plots indicate identified groupings within the TOFSIMS data...........................................................................................................208

Figure 8.4.9: PCA Loading Plots for Sample SC_NOX positive ions: Loading plot (a) and Biplot (b) of PC1 versus PC2 (▼- scores, ♦ - loadings), Cumulative variance captured by each PC (c). Loading plots indicate identified groupings within the TOFSIMS data.............................................................................................................................209

Figure 8.4.10: PCA Loading Plots for Sample SC_AIR positive ions: Loading plot (a) and Biplot (b) of PC1 versus PC2 (▼- scores, ♦ - loadings), Cumulative variance captured by each PC (c). Loading plots indicate identified groupings within the TOFSIMS data.............................................................................................................................210

List of Tables Table 3-1: Sample designation ............................................................................................36 Table 3-2: Prepared catalyst impregnated carbons..............................................................36 Table 3-3: Comparison of carbon content in NIST soot......................................................37 Table 3-4: ICP and PIXE analysis of catalyzed and non-catalyzed soots ...........................37 Table 4-1: Information on literature data sources used in Figure 4.3.1 below....................49 Table 4-2: Information on literature data sources in Figure 4.3.3 .......................................53 Table 5-1: List of Samples used in TPD-ToFSIMS analysis ..............................................79 Table 5-2: Integral rate sets, SC_NOX, Ions in bold are suspect. .....................................111 Table 5-3: Differential rate sets, SC_NOX. Ions in italics are suspect. ...........................118 Table 5-4: Max negative and positive rate categories, SC_NOX......................................121 Table 8-1: Catalyst impregnated carbon samples prepared for image analysis experiments

...................................................................................................................................182 Table 8-2: Estimate of oxidation for Experiment 1 Image Analysis (Peak Temperature 425

ºC) ..............................................................................................................................184 Table 8-3: Estimate of oxidation for Experiment 2 Image Analysis (Peak Temperature 350

ºC) ..............................................................................................................................185 Table 8-4: Sample designation of Raman Samples. # indicates file of Raman spectra and

that the measurement was repeated on a different part of the sample. ......................196

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1 Motivation/Overview

1.1 Motivation Diesel engines are the workhorses for industrial, commercial and personal transportation and

also play a vital role in power generation. The combustion process in the diesel engine is

extremely efficient which provides excellent fuel economy and torque. Unfortunately there is

a major negative effect, the emission of diesel particulate matter (DPM); it is composed

primarily of carbon or soot with minor components of organic compounds from unburned fuel,

lubricating oil and inorganic compounds such as ash (inorganic minerals) and sulphur

compounds. Reduction of diesel particulate matter (DPM) emissions is of prime importance

for both environmental 1 and health concerns 2. These concerns have lead to many

governmental agencies legislating stricter emissions regulations (US EPA 3, the European

Union and others globally). In order to meet these regulations and prevent DPM emissions

into the atmosphere, the current accepted method of removing diesel particulate matter is to

trap the DPM using a filter in the exhaust. As the filter accumulates DPM, it builds up

backpressure that has many negative effects such as decreased fuel economy and possible

engine and/or filter failure. To prevent these negative effects, the trapped DPM needs to be

periodically removed by gasification/oxidation to carbon monoxide (CO) and carbon dioxide

(CO2). The ease of removal is governed by the intrinsic kinetics of carbon and is discussed in

greater detail in Chapter 2. The understanding of the fundamentals that govern carbon

reactivity is important to improve technology for carbon filtration and oxidation.

The filtration device systems have limitations that strongly depend on the duty cycle of a given

engine or vehicle. Duty cycles where the exhaust temperature is low for the majority of its

operation do not allow the regeneration of the filter as a consequence of normal operation.

Engines that spend a lot of their time at low speeds and loads (e.g. buses, garbage trucks, and

forklifts) make it difficult to oxidize the DPM trapped on the filter due to the low average

exhaust temperature and occasionally low levels of active oxidant such as oxygen or nitrogen

dioxide. Many investigators have studied the application of these filtration devices onto

engines and the regeneration of them 4-8. It is known that the regeneration of the filtration

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device is dependent on its temperature, type of oxidants, engine make and model, and most

importantly the nature of the carbon particle 5. How the current technology for DPM filtration

performs is well described in the literature and is discussed in detail in Chapter 2.

The underlying limiting chemical process for regeneration of these filtration systems is the

oxidation kinetics of the carbon. The reaction kinetics is complex because the carbon’s

reactivity is dependent on its history (formation during combustion, residence time in the

filter), the morphology of the carbon particle and the functional groups located on the carbon

surface. Carbon oxidation kinetics and its mechanism have been heavily studied. As fully

discussed in Chapter 2, the reaction kinetics and mechanism are dependent on a variety of

factors such as the carbon structure, gas composition, and aging effects on the carbon structure,

attached carbon functional groups, catalytic impurities present with the carbon and others.

Functional group chemistry is central to the reactivity. Although there is a vast amount of

knowledge in this area, particularly for the carbon-oxygen reaction some important questions

still are not answered. For example, it is unclear what are the reaction mechanism and the

reaction intermediates formed on the carbon surface during its oxidation. The reaction of NO2-

carbon is faster than O2-carbon and plays a critical role in current DPM filter technology 9.

The NO2-carbon reaction has received less attention and its mechanism is less well understood.

Aging of carbon particles can reduce the reaction rate. Aging can refer to changes in structure

caused by thermal and also to poisoning effects on the carbon or in some cases specifically the

filter device by additional species in the exhaust. Information on thermal aging effects on

carbon present on filters is very limited 10,11. As discussed in Chapter 2, thermal aging effects

on carbon itself have been shown. However, information on the effects of thermal annealing

on soot and its implications on filter operation at low temperatures is lacking. Other species in

the exhaust have been shown to play a role. A recent study by Caterpillar 11 indicates that the

lube oil poisoning causes a loss in the activity of the carbon, mostly likely due to the lube oil

blocking the reactive sites of the carbon.

A considerable amount of information is available on DPM oxidation at temperatures from

250°C and above under real and simulated exhaust environment conditions. However, little

information is available on fundamental limitations of the technology with regards to carbon

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oxidation rates at the low temperatures relevant to advancement of technology under low load,

idle engine conditions.

For example,

• Are all the reactive sites on the carbon being used to maximize the rate of oxidation?

• Is there a limit to this rate?

• Is this limiting rate sufficient to prevent accumulation of DPM inside the filter system?

This thesis will examine these fundamental issues to study carbon oxidation with a practical

goal of extending the low temperature limit of filter operation.

This thesis will:

i) Provide evidence towards the lower limits for carbon kinetics and practical limits

towards low temperature operation for real world systems.

ii) Investigate thermal annealing of carbon and its effect on carbon reactivity and its

relevance towards filter operation.

iii) Study the identity and reactivity of surface functional groups on the carbon

structure that could be involved in the carbon gasification/oxidation mechanism by

a new technique, ToFSIMS (Time of Flight Secondary Ion Mass Spectroscopy).

The three goals above are chosen to assess fundamental information towards the limitations of

DPM filter operation at low temperatures of 200°C and provide input towards achieving this

goal under real-life exhaust conditions.

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1.2 Overview

1.2.1 Research Objectives

The two questions that are being addressed in this thesis are 1) can gasification rates at 200°C

be achieved that can maintain or reduce accumulated carbon loads in or on a filter media, 2)

can information be provided to better understand the fundamental parameters that affect DPM

gasification with and without a catalyst by studying the affects of change on active sites and

surface functional groups on the carbons.

1.2.2 Thesis Structure

The thesis is organized in the following manner:

• Chapter 2 contains introductory and background material. It is broken down into two parts:

o Section 2.1: A review of the fundamental information on carbons and what is

known about the carbon reaction mechanism and definitions of the fundamental

terms used throughout the document.

o Section 2.2: A review of the technology available and approaches used to oxidize

carbon on vehicles.

• Chapter 3 describes the material and the experimental procedures used in this study to

investigate reaction rates.

• Chapter 4 describes the results of the reaction kinetic studies under selected “standard”

conditions.

• Chapter 5 describes the surface group study by ToFSIMS.

• Chapter 6 reviews the conclusions of this study and how it helps advance the understanding

of carbon oxidation and its application to DPM filter technology. It also provides

recommendations on additional studies to advance the understanding of carbon oxidation

and its practical application to exhaust filtration devices.

• Several appendices contain additional information and exploratory studies that do not add

to main body of the thesis.

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2 Background The process of carbon oxidation/gasification is critical for many applications. These

applications range from environmental issues (diesel exhaust after-treatment) to power

generation (coal gasification) and others. In the case of exhaust after-treatment and coal

gasification, the reaction of carbon + oxidant is used to produce carbon oxides, water and

energy. This apparently simple reaction of carbon + O2 to produce carbon dioxide or carbon

monoxide has been extensively studied for over 50 years and is still not fully understood. This

is mainly due to carbon’s complex structure and chemistry. The reaction of NO2-carbon is

faster than O2-carbon and is less well studied. The structural and compositional chemistry of

the carbon, various oxidants and catalysts has been found to affect the carbon conversion

process. Carbon oxidation with respect to fundamental understanding is reviewed below in

Section 2.1. Section 2.2 reviews the application of technology for exhaust filtration and the

current state of the art and provides a bridge to the required carbon oxidation kinetics.

2.1 Fundamental understanding of carbon oxidation

2.1.1 Carbon structure The structure of carbon is complex. The basic structure of carbon, graphite, consists of

trigonally bonded carbon atoms (Figure 2.1.1) forming a single plane or basal plane 12-15.

These are stacked in layers and have an interspatial spacing of about 3.5 angstroms 12. Carbon

types differ due to morphology changes caused by stacking of the aromatic layers and

imperfection within the layers. The layers of carbon sheets in soot can be visualized as being

similar to layers of an onion. As the carbon layers or particles grow, defects, distortions and

inclusion of atoms into the structure cause the carbon to become disordered (Figure 2.1.2) 12.

Peripheral carbons (“edges”) of the graphitic sheet are the reactive centres for the reactions

with carbon - trigonally bonded “interior” carbons are not. During the course of reaction the

edges can be populated with an array of functional groups. The reactive edges of each of these

layers can terminate with functional groups such as hydroxyls, lactones, carboxylic acid,

anhydrides, bridged peroxides, pyrones and many others 12,13,16,17 (Figure 2.1.2). These

oxygen-containing functional groups are reported to comprise up to 50% of the functional

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groups on the surface of the carbon 18. These functional groups can be directly involved in the

reaction mechanism as intermediates resulting in liberation of CO or CO2. Conversely, these

functional groups can be “spectators” to the reaction and thus can modify the reactivity of the

active centres. The degree of disorder and type of surface functional groups can affect the

reactivity of the carbon by providing more surface area and a greater number of active sites.

Active sites are locations on the carbon where reaction with the oxidant is more likely to occur.

The concept of active sites is discussed in more detail later.

Figure 2.1.1: Oxygen containing functional groups on carbon

Carbon morphology is affected by temperature during formation. Diesel soot is formed by

short exposure times to high combustion temperatures (~1500°C and higher) (see Stanmore et

al.13 for greater details). These conditions produce a carbon particle whose morphology is

highly disordered. In this case, ordering refers to the stacking and the uniformity of the carbon

layers. Graphite is a highly ordered structure while diesel soot is more disordered. The

conditions that form diesel soot produce a carbon structure that has greater surface area than

graphite. This higher surface area may make diesel soot more reactive. Also, the fraction of

edge sites providing “reactive surface area” is strongly dependent on the thermal and reactive

history. The ordering of graphite and diesel soot can be visualized using the Marsh-Griffiths

model 12 (Figure 2.1.3). The model illustrates the graphitization process of carbons with

increasing temperature. The model shows that with exposure to higher temperatures the

carbon structure becomes ordered and thus the available surface area is reduced. For example,

diesel soot would have a structure similar to that on the far left of Figure 2.1.3, while graphite

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would have a structure more like that on the far right. Vander Wal et al. 19 captured images of

the highly disordered nature of combustion soots using high resolution TEM. They produced

photos of various combustion soots for different fuels (e.g. propane, diesel, acetylene and

others). Images of all these combustion soots, especially diesel soot, showed high disorder in

the stacking of the aromatic layers in the structure. Particulate matter has differences in

graphitic nature as demonstrated by investigations using NEXAFS (Near edge x-ray adsorption

fine structure); it was shown that NIST SRM (National Institute of Science and Technology

Standard Reference Material) 1648 urban particulate matter (PM) is more graphitic than NIST

SRM 2975 forklift PM 20. Unfortunately, the effects of disorder and the details of individual

layer stacking on the reactivity of carbon are not very well understood. Quoting Mims21

discussing carbon structure and reactivity the possible important details are ‘1) the actual

chemical configurations of the domains and their deviation from ideal portions of a graphite

layer and 2) the inter domain bonding. Even for graphitised carbons, the number and types of

defects are not completely known.’ Disorder in the carbon structure is important in the

reactivity of the carbon due to availability of sites for oxidation; this will be discussed in more

detail later.

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Figure 2.1.2: Representation of hexane soot showing defects and distortions from Smith et al. 18

Figure 2.1.3: Marsh-Griffiths model of graphitisation from Marsh 22

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2.1.2 Identification of surface functional groups Identification of surface groups on the carbon surface and how they affect reactivity continues

to be studied. The nature and the quantity of surface groups formed depend on the history of

formation of the carbon surface, its surface area and the treatment temperature 23. Surface

functional groups on carbon and model compounds are identified with the use of a variety of

analytical techniques. These include chemisorption, chemical titration 16,24,25, infrared (IR) 26-

35, TPD-MS (temperature programmed desorption mass spectrometry) 35, x-ray photoelectron

spectroscopy (XPS) 17,36,37, SIMS (secondary ion mass spectrometry) and INS (inelastic

neutron scattering) 37. Chemical methods were found to not account for all of the chemisorbed

oxygen based on surface functional group estimation 38. Other attempts to use simple organic

compounds to predict surface groups and their reactivity are difficult due to possible

interaction between groups on the carbon surface 38. In the next paragraph is a brief summary

of the work performed in the area of surface group identification on carbons; additional

reviews can be found in Stanmore et al, Marsh, and Boehm. 12,13,16.

Chemical titrations have been used by a number of researchers to identify surface groups. It

has been proposed that three types of surface groups exist, acidic, neutral, and basic (Figure 4).

Early studies by Boehm24 used bases in increasing strength to classify the acidic surface groups

on carbon black and oxidized charcoal. These acidic surface oxides are formed when carbon is

treated with oxygen at temperatures up to 400°C. The acidic functional groups present on the

carbon are carboxylic, lactonic and phenolic, or a frozen layer of CO2 is proposed to render the

carbon surface polar in character (Bansal and Donnet and references therein 39). Rivin 40,41

combined acidimetry and vacuum pyrolysis technique to determine the distribution of

functional groups on several carbons and their attributed surface acidity to carboxylic,

phenolic, neutral lactone and to quinone groups. Decomposition of these surface groups is

reported to occur between the temperature range of 300– 800 °C under vacuum and inert

atmosphere by evolving CO2 39. Neutral surface oxides are formed by the irreversible

adsorption of oxygen at the unsaturated sites (ethylenic type) present on the carbon surface 39.

The oxygen atoms form a –C-C-O-O-C bond that decomposes into CO2 on heat treatment in

vacuum. The neutral surface oxide is more stable than the acidic surface oxide, and begins to

decompose in the temperature range 500-600°C 39. Basic surface oxides are also reported on

the carbon surface 16,25. Garten and Weiss proposed a pyrone structure (a heterocyclic oxygen-

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containing ring with an activated =CH2 or =CHR group (R is an alkyl group) 42. Boehm and

Voll suggest a pyrone–like structure with the oxygen atoms located in two different rings of a

graphite layer 39. According to Montes-Moran 25, the thermodynamic stability and redox

potential of pyrone type structures makes them the primary source of basicity in basic carbons.

Figure 2.1.4: Illustration of acidic and basic groups on carbon. 25

Infrared spectroscopy is used by many investigators to study the surface functional groups on

carbon 18,26,30,43-45. A variety of IR assignments for various functional groups has been

determined, see Fanning and Vannice 30. These assignments are controversial (as discussed by

Boehm16), the band near 1600 cm-1 has been described as explaining stretching frequencies of

aromatic C=C bonds or could be describing a hydrogen-bonded, highly conjugated carbonyl

groups. Smith and Chungtai used IR to investigate reactions of NO2 and ozone with carbon

black in atmospheric type conditions (i.e. room temperature and atmospheric pressures) 18.

Detailed molecular characterization of surface chemistry of carbon has been pursued by many

techniques. These studies address static properties such as adsorption in addition to

gasification mechanism and kinetics. Quantitative information on the oxides present on carbon

surfaces has been collected using x-ray photoelectron spectroscopy (XPS) 17,33,46-48. The

various surface oxides present on carbon can be identified and estimated using the chemical

shift of the C1s peak. Vander wal et al. has shown the applicability of XPS to diesel soots 36.

Unfortunately getting information on concentration distributions of oxides on carbon using

XPS is difficult because of the small differences in binding energies for the different oxides

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and the limited resolution of common XPS equipment 16. In addition, Boehm 16 suggests that

the results can be misleading when the exterior surfaces are more strongly oxidized by aging

on porous samples. Langley et al. 17 recently performed chemical derivatization reactions with

XPS to determine functional groups on a carbon surface. They were able to make functional

groups more readily observable by reacting fluorine containing groups onto the carbon.

SIMS (Secondary Ion Mass Spectroscopy) is a technique used to investigate surfaces. SIMS is

very surface sensitive and can measure the first one to two monolayers of the surface.

Furthermore, molecular ions can give rich molecular information. The SIMS technique

involves the bombardment of the surface with a primary ion. This ion collides with the surface

causing surface fragments (secondary ions) to be ejected from the surface that are sent to the

detector. State of the art SIMS is represented by Time of Flight Secondary Ion Mass

Spectrometry (ToFSIMS). As discussed in Chapter 5, ToFSIMS provides maximum

sensitivity and mass resolution giving the richest molecular information of the surface.

ToFSIMS also has a greater sensitivity than XPS. XPS sensitivity is in the 0.1% range while

SIMS can measure surface concentration at ppm levels 49,50. Albers et al. used SIMS in

conjunction with INS and XPS to study the hydrogen content and graphiticity of carbons from

diesel soot and various carbon blacks 37. The diesel soot was tested before and after an

oxidation catalyst in the exhaust stream and after extraction of the soluble organic fraction.

The C2-/C2H- and C2

-/CH- fragmentation ratio, collected on a Leybold IQ 12/38, was used as a

crude measure to distinguish between graphitic and poorly crystalline surfaces. Albers et al.37

suggests that the oxidation catalyst reduced the hydrogen content on the surface of the carbon.

This paper indicates that the use of a sensitive SIMS instrument could provide valuable

information on carbon surfaces. For a more detail review and description of the SIMS

technique see Briggs 49.

2.1.3 Carbon reaction mechanism

Carbon oxidation is dependent on the type of oxidant, its morphology, thermal effects and the

presence of catalytic materials to increase the reaction rate 12,13,21,51. How these variables affect

the carbon reaction mechanism is still not fully understood although much research has already

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been performed and is discussed below. However, the reactivity of the different edge carbons,

the form of the reactive intermediate, and whether the attached functional groups on the carbon

edges affect the rate of oxidation remain unresolved. These factors may affect the active site

for reactivity of the carbon.

2.1.4 Active Sites

2.1.4.1 Reactive site concept (active site, reactive active site) As discussed earlier the edge carbons are the centre of carbon reactivity. Walker et al. first

introduced the concept of active sites to describe carbon reactivity in the 1960’s 52. This

concept was used by Boudart to describe catalytic reactions 53. An active site is an atomic or

molecular structure that is in an electronically favourable configuration for a reaction to most

likely occur on the catalyst. In the case of carbon these sites are located on the edges of the

aromatic layers 54 (See section 1 for details on carbon structure). These layers terminate to

form zigzag and armchair-type sites 55 and dangling carbon atoms 56. Computational methods

(Haynes and Sendt 57 and references therein) suggest that zig-zag sites are more reactive than

armchair sites (Figure 2.1.5).

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Figure 2.1.5: Carbon structure identifying zigzag and armchair sites

Application of the active site concept to carbon is difficult. The number of active sites is

dynamic because they are involved in the reaction: the active sites are removed as CO or CO2

upon gasification/oxidation. Unlike an active site for a catalyst that is replenished, the carbon

active site is removed and it is unknown if a new active site is created immediately to replace

it. Thus, during the process of carbon oxidation, the number and type of active sites change as

the carbon is consumed. Calo and Hall 58 have stated that ‘…over time a consensus has

developed among workers in the field which focuses upon an understanding of the nature and

behaviour of “active sites” on carbon surfaces as the key to resolving this problem. It is

reasoned that if these sites and the surface complexes that occupy them can be identified,

characterized, and understood quantitatively, then the key to carbon reactivity would emerge.

Although it is difficult to argue with this hypothesis, the complexity of carbons and chars most

probably precludes the realization of ever completely knowing, to the degree necessary, the

detailed physico-chemical nature of the carbon surface and the surface complexes.’

2.1.5 Oxidant effects A variety of oxidants has been investigated for the carbon oxidation reaction. These include

molecular oxygen 52,59-73 on various carbons (eg. DPM, pyrolytic carbons, carbon black),

nitrogen oxides 35,74-79, ozone 80-83, gas phase ions produced by plasma, water 76, CO2 84 and

Zig-zag sites Armchair

sites

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many others. In this section, the focus will be on the most common and readily available

oxidants in engine exhaust, oxygen and nitrogen oxides.

The kinetics and mechanism of oxygen reaction with carbon have been widely studied. A

variety of techniques has been used to elucidate the reaction mechanism and kinetic parameters

such as: IR (infrared spectroscopy), TPD (temperature programmed desorption), TGA (thermal

gravimetric analysis), and reactor studies. Reaction studies with oxygen are reported for a

wide range of carbon types from various coals to model compounds such as sucrose chars. The

kinetic parameters vary greatly depending on the type of carbon. Orders of reaction vary from

0.5 to 1.0 with activation energies spanning 102 kJ/mol to 210kJ/mol 13. Much of these

variations are due not only to the type of carbon but also the amount of contaminants present in

the carbon. In most cases, inorganic minerals play a role in catalyzing the gasification.

2.1.5.1 Oxygen reactions with carbon

A gap is present between the molecular structural information and mechanisms proposed in

relation to kinetics. Molecular information on the surface structure of carbon is incomplete.

This makes relating the structure to kinetics difficult to impossible. Typically for surface

reaction mechanisms or catalytic reaction mechanisms, the molecular conformation is not

specified and instead generic terms are used in kinetic models.

Many reaction mechanisms have been proposed for the reaction of oxygen on the surface of

carbon. In all cases, an oxygen intermediate is the proposed pathway to formation of carbon

monoxide or carbon dioxide. Haynes and references therein 85 describe two stoichiometrically

distinct surface reaction pathways: Type A reactions occur with the adsorption of oxygen

without gasification of the carbon substrate: C(_) + O2 C(O2) (two Type A O atoms

adsorbed). Type B chemisorption is favoured at higher temperatures and longer oxygen

exposures: C(_) + O2 C(O) + CO. Here, C(_) represents a free carbon site, C(O) represents

an oxidized carbon site with atomic oxygen and C(O2) represents an oxidized carbon site with

molecular oxygen. Biniak 86 proposed that superoxide ions O2- are formed on the carbon

surfaces by adsorbing molecular oxygen and use evidence provided by XPS 87 and IR 88 to

support their theory.

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The following mechanism (Mechanism 1) was used by Haynes to develop a turnover model

that describes carbon site heterogeneity 85. Here, C represents a free carbon site and C(O)

represents an oxidized carbon site. The free carbon site (C(_)) reacts with gas phase molecular

oxygen to form an oxidized site (C(O)) and gas phase carbon monoxide (equation 2-1a). The

oxidized site can produce a free carbon site and gas phase carbon monoxide or carbon dioxide

(equation 2-1b). Also the oxidized site can react with molecular oxygen to form an additional

oxidized carbon sites and release carbon monoxide and carbon dioxide. The model was used

to describe how power law kinetics takes into account the intrinsic heterogeneity of the carbon

(Hurt and Haynes89 and references therein). It predicted data collected on Spherocarb 85,

polymer char 90,91, coal char 92 and graphite 93.

Mechanism 1

C(_) + O2 ….C(O) + CO {2-1a} C(O)…. C(_) + CO,CO2 {2-1b} C(O) + O2 C(O) + CO/CO2 {2-1c}

Other proposed mechanisms include additional intermediate reaction steps. The reaction

scheme (Mechanism 2) proposed by Marsh et al 12 involves a free carbon site Cf, chemisorbed

localized oxygen C(O2), chemisorbed mobile molecular oxygen C(O2)m, chemisorbed

localized atoms of oxygen C(O) and chemisorbed mobile atoms of oxygen C(O)m. Here, a

free carbon site reacts with molecular oxygen to form a C(O2) site or C(O2)m sites (Equation 2-

2a). The C(O2)m sites form C(O)m and/or C(O) sites (Equation 2-2b). Gas phase CO can be

released from C(O) and C(O)m (Equation 2-2c and 2-2d respectively). Also, gas phase CO2

and a free carbon site can be created from gas phase CO, C(O)m and C(O) (Equations 2-2e to

2-2h). Last, gas phase molecular oxygen can react with C(O) sites to form gas phase carbon

dioxide (Equation 2-2i).

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Mechanism 2

Cf + O2 C(O2) or C(O2)m {2-2a} C(O2)m C(O) + C(O)m or/and C(O)m + C(O)m or/and C(O) + C(O) {2-2b}

C(O) CO {2-2c} C(O)m CO {2-2d} C(O)m + C(O)m Cf + CO2 {2-2e} C(O)m + C(O) Cf + CO2 {2-2f} CO + C(O) Cf + CO2 {2-2g} CO + C(O)m Cf + CO2 {2-2h} O2 +2 C(O) 2CO2 {2-2i}

Ahmed et al.71 suggest the formation of a stable carbon complex (Mechanism 3) where Cf

refers to an edge carbon atom (a free site), C(O2) refers to an adsorbed molecule before the

formation (of a stable surface complex) takes place, and (CO)c refers to the stable surface

complex. A free carbon site can react with molecular oxygen to form C(O2) (Equation 2-3a).

This C(O2) site can react with another Cf site to form the stable carbon complex (CO)c

(Equation 2-3b). These stable complexes can form gas phase carbon monoxide and a free site

(equation 2-3c). Or, react with a free site and gas phase molecular oxygen to form carbon

dioxide, another surface complex and a different free carbon site (equation 2-3d). The stable

carbon complex with C(O2) can form CO2, a stable carbon complex and a free carbon site

(Equation 2-3e). Or, can react with another stable carbon complex to form carbon dioxide and

a free carbon site. As well, Walker et al. 61 proposed that a fleeting carbon complex is formed

on the surface during the oxidation process. In all of these cases, the structure of the stable or

fleeting complexes that affect the reaction mechanism is not described. Again, the chemical

structure represented by these carbon oxygen complexes is unclear.

Mechanism 3

Cf +O2 C(O2) {2-3a} Cf + C(O2) 2(CO)c {2-3b} (CO)c CO(g) +Cf {2-3c} Cf + (CO)c + O2 CO2 + (CO)c + Cf {2-3d} (CO)c + C(O2) CO2 + (CO)c +Cf {2-3e} (CO)c + (CO)c CO2 + Cf {2-3f}

Even these “simplified” mechanisms speak to the complexity of the reaction and the lack of

detailed molecular knowledge.

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2.1.5.2 NOX reactions with carbon Nitrogen oxides have been known for some time to increase the reactivity of carbon at lower

temperatures 9,13,74,75,94,95. This section discusses the information available on the reaction

kinetics of NO 9,13,94,96 and NO2 9,13,74,75 with carbon in the absence of a catalyst. In this

section, focus will be primarily on surface groups present on the surface of the carbon during

this reaction.

Nitrogen oxides are good reactants with carbon. Early work by Smith et al. 94 proposed that

oxygen surface complexes are formed during the reaction of NO with sucrose char. The

reaction of NO + O2 with carbon and in the absence of a catalyst is known to be slower than

NO2 but faster than O2 9,97-99. This observed higher reactivity of NO2 with carbon is the basis

of carbon oxidation for some commercialized exhaust filtration technology discussed later in

section 2.2. Kinetic studies indicate that C reacts with NO2 to form NO and CO as the main

product pathway 9,75,100. Reported activation energies for the temperature range from 180 °C to

350 °C are 50 to 86 kJ/mol 100-102. More recently, Bueno-Lopez 103 proposed the following

model (Mechanism 4) for the NOX –carbon reaction with oxygen for complete reduction of

NOX to N2 using model information from Yamashita (see reference Bueno-Lopez 103). Here a

free carbon site (Cf) reacts with molecular oxygen to form carbon-oxygen complexes ((CO)#)

that can decompose into carbon dioxide (equation 2-4a). All other carbons ( C ) can react with

these carbon-oxygen complexes ((CO)#) to form CO2 and additional free carbon sites (Cf)

(equation 2-4b). Nitrogen oxides react with free carbon sites (Cf) to give nitrogen gas and

carbon –oxygen complexes ((CO)#) (Equation 2-4c). Last, NOX with other carbons ( C ) and

carbon oxygen complexes ((CO)#) form carbon dioxide, nitrogen gas and free carbon sites (Cf)

(equation 2-4d).

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Mechanism 4

Cf +O2 (CO)# {2-4a} n1C + (CO)# CO2 + n1Cf {2-4b} NOX + Cf ½ N2 + (CO)# {2-4c} NOX + n2C + (CO)# CO2 + ½ N2 + n2Cf {2-4d}

Where Cf are free sites or highly reactive unsaturated atoms of carbon, (CO)# are all surface

oxygen complexes that decompose as CO2 with the C to O ratio not necessarily being 1:1, C

represents all remaining C atoms not described by Cf and (CO)#. 103

Studies under atmospheric conditions show NO2 can interact with carbon (even at room

temperature) causing the formation of HONO intermediates 28,104-110. Early work performed by

Chughtai et al. 27, using FTIR at atmospheric conditions, showed that nitrogen-bonded

complexes are formed. From this information they proposed a dual path mechanism 27 that is

not discussed here. The nitrogen containing surface groups identified were C-NO2 and C-

ONO, as well as some other species

Muckenhuber et al 35 give evidence that an acidic functional group is formed that decomposes

into CO2 and NO at 140°C. Reaction of the NO2 with the carbon is proposed by them to react

directly with the surface and is not influenced by pre-existing surface groups.35 They propose

a reaction mechanism where two oxygen atoms from two different nitrogen dioxide molecules

produce CO2 and NO. Also, an acidic functional group is formed as an intermediate (acyl-

nitrite type) (O=C-O-NO). (Equation 2-5a,b)

Mechanism 5

C + NO2 C-O-NO {2-5a} C-O-NO ⎯⎯⎯ →⎯Tincrease C=O + NO {2-5b} C=O + C-ONO [O=C-O-NO]* CO2 + NO {2-5c}

Tomita et al 111 studied the high temperature (850°C) reaction between NO, pure carbon and

oxygen using isotope labelled reactants. They suggest that reaction between C(N) groups and

NO is the major route for N2 formation. In addition they propose that the O2 helps increase the

C(N) turnover by producing gaseous products.

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Zawadski et al 106 studied the interaction of nitrogen oxides with the surface of the carbon

using in-situ FTIR between reaction temperatures of 295 to 573K. They observed that surface

species for both reactions of NO2 and NO-O2 were C-NO2, C-ONO, C-NCO and anhydride

structures. The authors state that the reduction of NO2 to N2 can be achieved with microporous

carbons without additional reductant; significant NO2 to N2 was observed at 623K. They

exposed carbon to NO/O2 (680ppm NO, 270 ppm NO2, and 5% O2) mixture at 473K and found

three distinct IR adsorption bands at 1851, 1782 and 1743 cm-1. They suggest that the bands at

1851 and 1782 cm-1 are due to the formation of lactone and anhydride groups. At 573K, the

mixture leads to the formation of surface oxygen compounds. Between 523 to 573K, the above

mixture leads to the formation of iso-cyanate species. The formed NCO species may come

from the reaction of NO and CO. Thermal stability of the surface functional groups was

checked after exposure to the mixture. The sample was heated to higher temperatures and the

sample analyzed using IR. Out-gassing to 723K indicated small amounts of surface

compounds are destroyed (1851 cm-1 and 1782 cm-1). At 773K, oxygen surface compounds

show minor destruction with no major changes in the NCO bands at 773K. At 873K, CN

surface species are decomposed.

As discussed above, the intermediates formed during the reaction of NOX with carbon are not

clear. Definitely, further study is needed to identify the influence of surface groups on the

reaction mechanism of NOX with carbon.

2.1.6 Structural effects on soot oxidation In the last few years, there has been a great deal of study on soot morphology and how it

affects the reaction rate of the carbon 10,19,36,112-121. Ishiguro et al 112 studied diesel soot

oxidized in air at various stages of burnoff. They found surface area increased with the

removal of SOF (soluble organic fraction) during early stages of burnoff. TEM images showed

the soot structure is turbostratic (i.e. has a wavy structure). The wavy structure is caused by

formation of 5 and 6 member rings and defects located within the layers during the soot

formation. Ishiguro et al 112 provides evidence of crystallites at the edges of the particles

flaking off instead of the particle becoming smaller. FTIR data of the different burnoff levels

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show a decrease of the 1700 cm-1 (corresponds to the C=O group) with respect to the C=C

vibration at 1600 cm-1.

Vander Wal et al. 10,19,113 using HRTEM investigated oxygenated diesel fuel soots and found

that highly disordered carbon structures can be produced that are potentially higher in

reactivity. The highly disordered carbon structure exposes a greater number of edge carbon

atoms. As discussed earlier, these edge carbons are well established as the most reactive 52,54,122. HRTEM work has shown that thermal annealing (700°C) causes the outer layers of the

soot particle to become more graphitic 113. The images indicate the oxidation of the particle

proceeds from the inside to the outside. Su et al 119 and Muller et al 120 found that diesel soot

from a Euro IV heavy-duty diesel engine consisted of more fullerene type (onion-like)

structure and the soot started combusting at 573K. Further studies by Muller et al 120 compared

the reactivity of soots from four different sources in order of increasing graphitic nature: spark

discharged soot, Euro IV soot, soot from a smoking diesel engine and furnace soot. The soots

with lower graphitic content and thus more disorder in the carbon structure were more reactive.

Raman spectroscopy is used to show differences in the amorphous and graphitic behaviour of

carbons 123. The pioneering work of Tuinstra and Koenig 124 showed that variations in Raman

spectra were observed in different carbon materials. In this initial work, they observed a shift

of the intensities between the 1350cm-1 (D) peak and 1600cm-1 (G) wavenumber peaks. Of

these two main features, the 1350cm-1 is thought to relate to ”edge” carbons and the disorder of

the carbon structure, while the second feature at 1600 cm-1 is thought to relate to crystalline

graphite. The change of the D (1350cm-1) and G (1600cm-1) peaks gives an indication of the

graphitic nature of the carbon, while the D/G intensity ratio gives an indication of the degree of

disorder. Compagnini et al. and references therein 125 has provided evidence that the D peak

correlates with disordered carbons on graphite and is possibly related to edge carbons. The

application of Raman spectroscopy to graphite and amorphous carbon is available in review

articles by Ferrari 126 and Pimenta et al. 127. Also, the technique has been applied by a variety

of authors 118,128,129 to diesel soots. Further information on Raman can be found in Section 8.3,

Appendix C- Raman.

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On a macroscopic scale, Higgins et al 130 developed an experimental method to extract surface

kinetic rates based on size-selected nanoparticles. A modified Arrhenius method gave

activation energy of 164 kJ/mol with different pre-exponential factors for each initial particle

size over the temperature range of 800 – 1200°C. They reported that the results agreed with

other published work.

2.1.6.1 Thermal aging Exposure of carbons to high temperatures is shown to negatively affect the carbons reactivity

on phenol formaldehyde resins 90,91 and coal 131-133 using high temperature anneals (> 900°C)

in an inert atmosphere. Suuberg et al. 90,91 show that the surface area of the carbon measured

using oxygen chemisorption decreases with increasing annealing temperature and with

exposure time. Possibly annealing of the carbon (DPM) in an exhaust environment may cause

loss of surface area and rearrangement of surface functional groups that could result in the loss

of active sites.

2.1.7 Catalyst effects Catalysts are effective in improving carbon reactivity. They work by creating new reaction

pathways that have rate limiting steps with lower activation energies and/or by the creation of

active sites. The review paper by Mims 21 documents that nearly all the elements on the

periodic table are effective at catalyzing the carbon oxidation reaction. Stanmore et al. 13

documents more recent catalysts used in DPF applications. Many catalysts 21,84,99,122,134-221 are

reported with a variety of structures and elemental compositions that have been used to

catalyze the carbon oxidation reaction.

Two factors that affect catalyzed carbon oxidation are the carbon catalyst contact and the type

of catalyst. Catalyst–carbon contact is a key element. Some catalytic elements are mobile

enough under reaction condition to ‘wet’ the carbon surface and effectively disperse their

activity and move to non-reacted carbons. Other catalysts remain as discrete particles but are

mobile enough to maintain contact with the carbon. More static catalytic elements require the

carbon to contact them. Moulijn et al. has described two modes of carbon catalyst contact,

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loose and tight 201. Loose contact mode was found to best simulate contact of carbon and

catalyst in a DPF environment. Tight contact provides higher reaction rates and may

correspond closer to certain types of DPM oxidation catalyst, such as fuel borne catalysts 201.

Type of catalyst is important. The most active of these catalytic species are the oxides of the

alkali and alkaline earth group metals (Na, K, Ca) 84,167,168,183,184,187 and some transition group

metals such as V, Ce, Fe, etc. 163,188,204,208,211,213,214. The key to the reactivity of these elements

is their mobility (“wetting”) on the carbon structure allowing for excellent carbon-catalyst

interaction at the active site and providing intimate availability of oxygen (present in the

catalyst) at the carbon active site. Other catalysts (such as Pt) can catalyze the NO + O2

reaction to NO2. As discussed earlier the NO2 + C reaction is faster than the O2 + C reaction.

However, it is unclear if the presence of a catalyst improves the NO2 + C reaction or only

catalyzes the formation of additional NO2 through the NO + O2 reaction, thus indirectly

affecting the carbon reactivity.

Alkali metals have high mobility allowing for excellent ‘wetting’ of the carbon. They are

known to be effective coal gasification catalysts at high temperatures (>600°C) 84,167,168,170-

172,183,184,186,187,206,207. At temperatures greater than 300°C, the alkali metals become mobile and

are able to migrate across the surface and decorate the edge carbons. Once at the active site

they can directly supply oxygen to the active sites and initiate the formation of carbon

monoxide or dioxide. An intermediate in the reaction mechanism for K catalyzed carbons is a

phenoxide intermediate using a bridged K ion 21,206,207. Electron microscopy work by Yang et

al. 122, Baker et al. 208 and McKee et al. 170, show the migration of catalytic particles across

graphite crystals (‘wetting’) and the recession of the carbon edges. Bueno-Lopez et al. 103

report that NOX reduction increases from 3% on a non-catalyzed carbon sample to 63% with

4.2wt% K loaded bituminous coal using a gas stream of 0.5% NO + 5% O2 at 350°C. Van

Setten et al. 201 investigated alkali metals on diesel soot reactivity and its application to diesel

particulate filters. They report alkali metals, Cs and K based, have carbon ignition

temperatures of around 350°C. Unfortunately for DPM filters, alkali elements are very mobile

and tend to migrate into the cordierite filter structure and thus the catalytic material becomes

ineffective 220.

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Noble metal catalysts are very active for the carbon oxidation reaction 209,214 and especially so

for nitrogen oxide containing streams. Pt based catalysts are known to catalyze the reaction of

NO + O2 to NO2 68,74,75,185. Tests with oxygen and a Pt catalyst report ignition temperatures of

400 – 425°C for the C + O2 reaction. As discussed earlier (Section 2.2.2), NO2 is able to

oxidize the carbon at a faster rate than oxygen and is used in current diesel particulate matter

filter technology for regeneration.

Inorganic metals are present in diesel soot. These may play a role in catalyzing the oxidation

of the carbon. However the presence of sulphur and phosphorus in the exhaust stream may

diminish their effectiveness by creating less catalytically active metal sulphates and/or

phosphates.

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2.2 DPM filter technology and state of the art In this section, an update of the technological requirements is provided and links these needs to

kinetic requirements. Reduction of emissions of DPM (diesel particulate matter) is of prime

importance and has lead to many governmental agencies legislating stricter emissions

regulations. In order to meet these regulations, systems have been devised to trap the DPM

and limit its emission into the atmosphere 5,222,223. Techniques that are used to oxidize the

trapped solid DPM, primarily carbon into gaseous components, such as CO or CO2, include the

use of catalysts 5,224-228, creating oxidant (ozone 229, plasma 230,231, NO2 74,75,226,227) and the

addition of energy (fuel injection 232-234, electrical heating 235,236, microwave heating 237). All

of these systems have limitations and strongly depend on the duty cycle of the engine or

vehicle. Engines that spend a lot of their time at low speeds and loads have difficulty oxidizing

the DPM trapped on the filter. The underlying root of these systems is the oxidation kinetics of

the carbon and was reviewed in Section 2.1. In Section 2.2, a review is given of the

technology being implemented in real world applications.

2.2.1 Current legislation and technology

Diesel engines are important for industrial, commercial, and personal transportation because of

their excellent fuel economy and torque. Diesel particulate matter is a product of incomplete

combustion in diesel fuelled vehicles. It is also known that the DPM can cause environmental

and health effect problems 238-240. In 1996, the California Air Resources Board designated

DPM as a possible carcinogenic substance 241,242. The passing of tougher regulations and

lowering of fuel sulphur levels have provided favourable conditions for wider usage of diesel

particulate filters for the capture of the DPM for many years to come (Figure 2.2.1) 4,243-246.

Figure 2.2.1 shows current, past and future regulations for NOX and DPM emissions for on-

road engines for the European Union, Japan, and the US (Large squares). Anticipated engine

out emissions are shown using the dashed lines.

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NOX and DPM emissions are inversely related. Engine manufacturers are able to influence the

exhaust emissions through ignition timing to cause either higher NOX outputs or DPM outputs

because engines can be tuned to meet the DPM requirement but would require SCR (selective

catalytic reduction) as per Euro IV regulations. Engines in the US have higher DPM emissions

and lower NOX emission and require DPFs to meet US 2007 regulations. Future regulations

will require some combination of both DPM filters and NOX reduction technology. Off road

regulations are similar to on-road regulations but have implementation dates two to three years

behind on-road regulations. Filters are complex to implement into vehicles. The filters must

be able to fit the limited space on the vehicle, have minimal fuel penalty, not create excess

backpressure on the engine and periodically must be cleaned or regenerated to remove the

DPM.

Figure 2.2.1: General comparison of on-road heavy-duty diesel (HDD) standards in the US, Japan, and Europe. Estimated engine-out emissions for 2007 and 2010 (range) are shown. Steady-state cycle. 243

Reprinted with permission from SAE Paper# 2006-01-0030 © 2006 SAE International.

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There are two main types of filters available commercially, blocking and non-blocking filters.

Most commonly used are blocking filters that consist of wall flow or deep bed filters. These

types of filters force 100% of the exhaust flow through the filter media. Wall flow filters

(Figure 2.2.2) are highly effective and can filter 99% of the particulate matter 247. They are

made of cordierite (NGK 248, Corning 247) or silicon carbide (Ibiden 249, NoTox, Liqtech) or

metal fleece (Purem). They consist of parallel channels with alternating ends plugged, causing

the exhaust to flow through the porous wall and trapping the DPM. If the particulate matter is

not oxidized to remove the carbon (also known as filter regeneration), the accumulated DPM

on the wall flow filter can cause backpressure build-up on the engine causing engine stoppage,

failure of the engine or failure of the filter. Additionally increased backpressure can also be

caused by the accumulation of ash deposited on the filter from the lube oil. Non- blocking

filters (Figure 2.2.3) (Emitec 250, DCL 251) have an open structure and use exhaust flow

diversion and hydrodynamic pressure differentials across the filter media to force a portion of

the exhaust flow through the filter media. The open structure protects the engine by preventing

backpressure increases by bypassing the exhaust flow around the filter media if it becomes full.

The disadvantage is that the filtration efficiency is lower and can vary from 0 to 60%. For both

non-blocking and blocking filters the need to regenerate the DPM by oxidizing the carbon is

vital to maintain the operation of the device.

Figure 2.2.2: Example of exhaust flow through wall flow filter

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Figure 2.2.3: Example of exhaust flow thorough (non-blocking) filter (DCL) 251 Reprinted with permission from SAE Paper# 2007-01-4025 © 2007 SAE International.

Diesel particulate matter is composed of three major components. The soluble organic fraction

consists of unburned diesel fuel and lube oil. Solid elemental carbon is the most significant

component by mass, and is contaminated with inorganics from lube oil blow-by and trace

amounts present in diesel fuel. Dihydrogen sulphate, made from sulphur in the fuel and lube

oil, makes up the rest of the particle. The proportions of these components have changed

greatly with engine improvements, changes in fuel sulphur and the use of ‘environmental

friendly’ fuels (biodiesel, Fischer Tropsch). The inorganics in the DPM may play a role in

catalyzing the oxidation of the carbon, however the presence of sulphur and phosphorus in the

exhaust stream may diminish catalytic effectiveness of these inorganic elements. A recent

review by Maricq 252 discusses chemical characterization and methods of analysis of diesel

particulate matter. Newer engines (>2007) are anticipated to produce a particulate with a

majority composition of elemental carbon in the form of soot due to the more efficient

combustion of the fuel. In addition, research has shown that morphology and microstructure of

the carbon changes with engine operating conditions 10,19,36,113,114,116,130 and the type of fuel

used such as biodiesel or Fischer Tropsch 115,118. Biodiesel was found to have greater surface

oxygen groups and was more reactive than Fischer Tropsch fuels 118. This makes the removal

and oxidation of soot at low temperatures one of the most difficult of the various emissions

regulations to meet.

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Duty cycles and exhaust temperatures of diesel engines vary with application and engine

manufacturer 253. Normal operating temperatures of diesel engines typically range between

150°C (idle) to 600°C at full load depending on the engine and duty cycle of the equipment.

For example, a forklift might be operating 90% of its time at idle and 10% of its time at full

load where the temperature may not exceed 380°C. Similarly, a school bus picking up kids in

a neighbourhood may spend its entire time at idle or low load condition and never reach

sufficient temperatures for DPM burn off. Conversely, a mining hauler may operate 70% of its

time at idle and the remainder of the time the exhaust temperature may exceed 600°C because

it is transporting up a grade thus, giving an opportunity to regenerate the filter. If the DPM is

not removed from the filter, excess backpressure will develop and cause the engine to stall or

cause damage to the engine. In some cases, applying too much backpressure to the engine will

void the engine manufacturer’s warranty.

DPM can be collected using either a catalyzed or non-catalyzed diesel particulate filter (DPF).

Although DPF’s are able to solve many applications, the criteria of operating temperature and

duty cycle are applied to both catalyzed and non-catalyzed DPFs 253. DPM begins to burn in

diesel exhaust without a catalyst at around 600°C. Current, base metal catalyzed DPF’s have

been tested and found to give balance point temperatures of 380-420°C. Pt based DPF’s are in

the 350 to 400°C. Balance point temperature is a commonly used method of evaluation of

DPF regeneration. At this temperature the engine soot production rate is equal to the removal

rate of DPM or oxidation rate of the carbon. An example of a commercial DPF is the Johnson

Matthey (JM) patented catalyzed regeneration filter (CRT) 74,75,222. It uses an oxidation

catalyst (e.g. Pt/Al2O3) upstream of the DPF. The oxidation catalyst converts NO in the

exhaust to NO2. The NO2 enters the DPF and oxidizes the DPM. This has been reported to

remove DPM at a balance point temperature of 320°C, but is strongly dependent on the NO

content in the exhaust stream, the NO/NO2 thermal equilibrium, exhaust temperature and

sulphur content in the fuel. BASF’s (formerly Engelhard) DPX commercial filter is reported to

operate at temperatures of 225 °C under certain conditions 254. An added drawback for Pt

catalyzed technologies is the emission of high levels of NO2 at the tailpipe. Recent regulations

by California Air Resources Board (CARB) prevent increases of NO2 greater than 20% over

engine out emissions 255. Precious metal based filters are under scrutiny by the underground

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mine community because of the higher NO2 emissions that reduce air quality. Both of these

devices (JM and BASF) have undergone extensive field trials. Although both systems can

operate well at times they have problems with low temperature/low engine load applications.

Under these conditions, the carbon overloads the filter and eventually ignites causing high

temperatures that melt the filter and cause failure. For the 2007 on-highway regulation, the

technology uses sophisticated methods to track the amount of soot in the filter and a burner or

engine modifications to cause regeneration of the filter that can lead to higher fuel

consumptions costs. Improved catalytic systems at these lower temperatures could potentially

solve this problem.

Solutions to low temperature applications involve complicated systems and controls, some

operator intervention, added energy and high maintenance (e.g. fuel burner, electrical heating,

air throttling, etc.) 256-261. The ultimate solution is a catalyzed DPF that needs minimal

maintenance, requires no additional power input, uses molecular oxygen, minimizes NO2

production, and is a “bolt and go” solution. Can catalyzed DPF’s be used for low

temperature/low load engine applications with the right catalyst? Extensive research has been

performed on different catalyst, but there have been no reports of a lower temperature limit on

catalyzed DPM oxidation. An important question to ask is whether or not the lower

temperature limit on catalyzed DPM oxidation has yet been reached.

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2.2.2 Relating fundamental kinetics to engineering targets

2.2.2.1 Macroscopic reactivity requirements

Here the engineering target for a continuously operating filter is established. At this

macroscopic level, a gasification reactivity is required to continuously operate the filter.

Additionally, this reactivity is required at a target temperature. On this level, the macroscopic

gasification rate is defined as:

SG Cdt

dCR 1•−= (1/time = 1/h) {2-7}

Where dC = moles of carbon reacted, Cs = total quantity of carbon in the filter or reactor, t =

time, and dC/dt is the extensive gasification rate in moles per time. It must be noted that the

term (RG) has the units of a first order rate constant, but for solid reactants this specific

reactivity on a solid (not volumetric) basis is standard.

The value for the required macroscopic specific rate (RG) is based on soot emission outputs

from a modern diesel engine. The lowest raw emission rate from the 2007 engine output line

on Figure 2.2.1 was used as this value. This value is 0.02g DPM/bhp-hr (0.027g DPM/kWh).

An emission rate at this level would be considered an extremely clean engine based on the

2002 EPA standards (0.1g/bhp-hr for an on-road 2002 bus engine, off road about 10 times

higher). However, the standard was changed in 2007 to the current on-road emission

requirement of 0.01g/bhp-hr and thus would require at least a 50% reduction of particulates

and is achieved with the use of a filter device.

Figure 2.2.4 shows a 480 hp engine with this emission rate and thus gives 10g/h of carbon.

The emissions from this engine pass into a particulate filter where the carbon is trapped.

Another flow stream is shown leaving the filter. This stream contains gas phase carbon

oxidation products such as carbon monoxide and carbon dioxide and would be 10g/h on a

carbon basis under steady state conditions. The filter was sized to give a maximum

backpressure of 40” water on a 480 hp engine when filled with DPM (maximum of 60g). It is

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assumed the DPM contains carbon only. However to allow for disturbances in emission rates

and duty cycle changes, the engineering target is based on 1/3 of this maximum filter hold up

of 60g, giving a value of 20g of carbon in the filter. Thus the gasification rate is 10g/h of

carbon (∆C/∆t) divided by filter hold up of 20g (1/Cs) to give a macroscopic gasification rate

of 0.5 h-1 under steady state conditions (RGo) and is the reactivity necessary for a low-

temperature passive system. It is approximately 50% of the instantaneous soot inventory

oxidized per hour (0.5 h-1)(Figure 2.2.4). This macroscopic gasification rate (0.5 h-1) assures

that the steady-state inventory of soot on the filter is at or below that required for continuous

operation.

Figure 2.2.4: Base case gasification rate criteria

A target temperature of 200°C is established as the temperature criteria for continuous steady

state regeneration of the filter. This temperature is higher than idle engine temperatures that

can be as low as 150°C. Under low load conditions it is assumed that the exhaust engine

temperature will meet this target temperature and is chosen to reflect low load, low temperature

applications discussed in Section 2.2.

Evaluation of experimental and literature information in light of the criterion above is done by

using a plot in Figure 2.2.5. The plot contains the gasification rate plotted on the y-axis and

inverse temperature on the x-axis. The horizontal and vertical lines represent the engineering

targets of the macroscopic gasification rate and target temperature. The shaded region in the

plot (Figure 2.2.5) indicates the target region for the carbon oxidation reaction to operate

within for typical diesel applications. Below 200°C (1.74e-3/K) is the desired operating target

Engine

DPF ~20g

Max: 60g

10.5” dia. x 12” DPF 480 hp engine 40” H2O ~3g soot/ litre filter

10g/h at steady state 10g/h at steady state

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for low temperature diesel applications with a minimum steady state gasification rate (RGo) of

0.5 grams carbon oxidized/(grams of carbon initially in reactor or filter * hours) or (g/(g-h) or

(1/h). Later in Chapter 4, this plot is used to evaluate the reactivity of the carbon-oxidation

reaction with oxygen and nitrogen oxides with and without catalyst for both literature and

results acquired in this work. This plot is useful for both the overall gasification rate and also

to place the reactivity of surface functional groups in context of DPM technology.

Figure 2.2.5: Example of gasification rate chart indicating desired reaction region

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2.2.2.2 Microscopic reactivity requirements

2.2.2.2.1 Definition of turnover frequency (TOF)

On a microscopic basis, the measure of site reactivity is the turnover frequency (TOF).

Turnover frequency is the rate of product molecules produced per reactive site and is defined

as:

SdtdCTOFG

1•−= (mol/time *1/site) (h-1) {2-8}

Here, S is the number of carbon reactive sites, and dC/dt is the extensive gasification rate.

If it is assumed that all the reactive sites on the carbon have the same reactivity the

macroscopic gasification rate is:

RG = TOFG * (S/C)

However, as discussed earlier in section 2.1 the edge carbons can be populated with a variety

of functional groups and other contaminants. Each of these can change the reactivity of the

carbon reactive sites and neighbouring carbon reactive sites and thus the carbon can contain a

number of reactive sites with differing reactivities. This makes the macroscopic gasification

rate a function of these multiple reactivities and is defined as:

RG = ∑(TOFG, i * Si/C)

Where, subscript, i, represents a single reactivity type

In the case of carbon these reactive sites are edge carbons located on the periphery of the

carbon sheets. Electron microscopy studies by Yang et al. 122, Baker et al. 208 and McKee et al. 170 use turnover frequency to report recession rates on carbon surfaces (i.e. carbon removal). It

was found that the recession rates of the basal plane atoms were significantly lower than the

edge carbons. The measurement of turnover frequency for disordered carbons is difficult and

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are never reported in any application literature and rarely reported in laboratory bench scale

studies.

Additionally in section 2.1, it was discussed that the reaction of carbon can contain a large

number of individual steps that have various micro-kinetic parameters. This is not addressed

here, however ToFSIMS can provide information on individual surface reaction rate steps and

is discussed further in Chapter 5. Reactivity parameters are expressed as rate terms (ri, sims and

rg, sims) with units of h-1 and are based on methods discussed in Chapter 5.

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3 Experimental procedure for reactivity studies

3.1 Soot characterization and catalyst impregnation

The chapter covers materials used and the method of preparation for the samples used to

address active site reactivity and surface functional group reactivity experiments. ToFSIMS

methods will be covered in Chapter 5 where these results are discussed.

3.1.1 Materials

Carbon samples used to study the reaction fundamentals of DPM gasification/oxidation are

shown in Table 3-1. They include a pure carbon made from sucrose char and two diesel soots.

Sample NIST, a National Institute of Science and Technology Standard reference material

(NIST SRM 2975), is diesel particulate matter collected from a diesel-fuelled forklift. Its

certification and specifications can be found in Appendix E. Sample CAT was collected at

DCL International Inc. on a Caterpillar 3306 diesel engine at an engine load of 200Nm, 1400

rpm and an exhaust temperature of 200°C

Sucrose char was prepared by slowly heating sucrose (Sigma S-9378 - Lot#: 22K0066). The

sucrose was heated at 1°C/min to 400°C and held for 2 hours under air in a muffle furnace.

Upon completion, the sucrose char produced was black and brittle. The char was ground using

a mortar and pestle to produce small particles of 300um.

Surface areas measured by BET N2 adsorption were 77m2/g and 12 m2/g for the NIST and

sucrose char respectively. SEM photos of the gross morphology can be found in Appendix B -

SEM. Sucrose char is macro-structurally smooth while possessing internal surface area. The

diesel soot image shows a lacy morphology from agglomeration of 20nm primary particles.

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Table 3-1: Sample designation

Sample designation

Type of Sample

NIST NIST traceable diesel particulate matter SRM 2975 Sucrose Char (SC)

Sucrose char made by ramping temperature at 1°C/min to 400°C heating in air

CAT Engine soot collected on a CAT 3306 diesel engine at an exhaust temperature of 200°C, Engine Load 200 Nm, 1400 rpm

3.1.2 Impregnation of carbon samples with catalyst precursors Three standard catalytic elements were chosen from review of the relevant literature (see

Chapter 2). Intimate contact was the objective of the impregnation to achieve the maximum

possible reaction rate. The three catalysts are listed in Table 3-2. Through intimate contact

and high catalysts/carbon ratios a greater number of the carbon edge sites will be catalyzed.

Catalysts were prepared by impregnation of the carbons with soluble metal precursor solutions

and the preparation method is described in Appendix A.

Table 3-2: Prepared catalyst impregnated carbons

Sample Designation

Carbon Sample

Catalyst/Carbon mol ratio

Ion impregnated

Ion precursor

K-NIST NIST 1:50 K KOH V-NIST NIST 1:100 V Ammonium meta

vanadate Na-NIST NIST 1:50 Na NaNO3

3.1.3 Elemental characterization Elemental analysis was performed using PIXE, and carbon combustion at EAI – Elemental

Analysis Inc., Lexington, Kentucky. ICP analysis was performed by Chemisar Laboratories,

Guelph, Ontario. Carbon combustion results indicates carbon contents on the two samples

were similar between the NIST and the vanadium impregnated NIST with carbon content of

85-86% (Table 3-3). The inorganic component accounts for the remainder of the mass of the

soot. Carbon content of the CAT and K-NIST samples was not measured.

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Table 3-3: Comparison of carbon content in NIST soot

Sample ID Carbon (wt%) NIST 85.3%

V-NIST 86.4%

The composition of the inorganic ash was measured using two methods: ICP (Inductively

Coupled Plasma Spectroscopy) and PIXE (Proton Induced X-ray Excitation). Samples for the

ICP were first combusted to remove the organic carbon and the ash was dissolved in aqua regia

for analysis. PIXE samples were examined as-is.

Table 3-4: ICP and PIXE analysis of catalyzed and non-catalyzed soots

CAT NIST K-NIST V-NIST NIST Element ICP, % ICP, % ICP, % PIXE, % PIXE, %

Na 2.20 14.40 2.34 0.00 0.00 Mg 0.78 6.00 0.48 0.00 0.00 Al 2.05 2.53 0.37 0.00 0.00 P 0.98 12.03 0.84 0.00 0.00 S N/A N/A N/A 62.60 30.63 K 0.27 1.56 93.17 0.00 0.00 Ca 8.26 10.90 0.92 3.42 14.31 V 0.00 0.00 0.00 4.93 0.00 Cr 2.29 0.00 0.20 1.55 4.74 Mn 0.80 0.00 0.00 0.00 0.00 Fe 75.82 11.10 0.84 20.03 23.85 Co 0.26 0.00 0.00 0.00 0.00 Ni 2.79 0.00 0.00 0.00 0.68 Cu 0.00 0.00 0.00 0.26 0.63 Zn 2.95 39.60 0.53 7.22 25.18 Ba 0.07 0.00 0.00 0.00 0.00 Ce 0.07 0.00 0.00 0.00 0.00 Pb 0.08 0.00 0.00 0.00 0.00 Tl 0.20 0.00 0.00 0.00 0.00 B 0.14 1.88 0.31 0.00 0.00

ICP results of the inorganic materials without S content are shown in Table 3-4 for the NIST

soot, CAT soot and NIST soot impregnated with K (K-NIST). The K-NIST sample contains

primarily K in the inorganic fraction. The major inorganic components found in the NIST and

CAT soot were Zn, Na, P and Ca. Ca, Zn and P are from lubricating oil 262,263. The CAT

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diesel contains a high concentration of Fe (~ 50000 ppm). The presence of Fe in the CAT

diesel is due to the following: lube oil ash, wear in the engine cylinder or corrosion of the

exhaust pipe. The latter two choices are more likely due to the high concentration of Ni and Cr

present. Also, Ce was observed in trace amounts on the soot, the trace amounts could be from

the lube oil ash or a result of experiments performed with fuel additives on this test engine

about 10 years prior to the collection of the soot sample. All of these materials have elements

that have proven to have some catalytic activity towards carbon oxidation (see Chapter 2.4).

The above samples were investigated in the catalytic screening runs using the reactor.

3.1.4 Spectroscopic characterization of soot

Sample characterization was performed using various methods. Analysis was performed to

determine edge sites and functional groups found on the carbon surface. Raman spectroscopy

was used to determine qualitatively the presence of edge sites and the disorder of the carbon.

Time of flight secondary ion mass spectroscopy (ToFSIMS) was used to determine the

functional groups present on the carbon surface. The ToFSIMS experimental procedure is

described in detail in Chapter 5.

Raman spectroscopy was performed with mixed results using the micro-Raman instrument at

the University of Toronto’s Institute of Optical Science, laser spectroscopy department. The

technique, experimental procedure and results are discussed in Appendix C. Interestingly due

to the type of Raman instrument used in this experiment it was observed that the D/G peak

ratio (see Chapter 2.2.6) changed with laser exposure. This changing ratio is likely due to local

heating of the surface and possibly oxidation of the carbon creating edge sites. A search for a

spinning sample stage that would reduce the local heating effects on the carbon was

unsuccessful resulting in further experimentation being abandoned. In further chapters of this

document, results will be presented regarding thermal annealing of the carbons. An interesting

experiment would be to perform Raman under a He atmosphere and observe if the D/G peak

ratio changes with laser exposure. This could give interesting information toward surface

morphology changes on the carbon and possibly creation/destruction of edge sites.

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3.2 Reactivity studies Brief screening studies were attempted to evaluate a larger suite of catalysts in parallel. These

are discussed in Appendix A, but are supplemental to the information in this thesis. Literature

indicates that the alkali metals and vanadium maintain higher catalyst-carbon contact by

“wetting” the carbon surface and being sufficiently mobile to maintain such contact during

reaction. Materials with “standard” catalytic elements were tested using the gas reactor shown

in Table 3-2. The methods used to prepare the samples and reactivity screening method using

image analyses are described in Appendix A.

3.2.1 Reactor system

The reactor, as shown in Figure 3.2.1, is composed of an up-flow reactor. Reaction products

from the reactor are monitored with a continuous FID (flame ionization detector) that is

discussed in detail later. Inlet gas reactants are introduced into the reactor system using two

mass flow controllers (Omega 5400) that feed 10% oxygen/He and He only respectively. The

mass flow controllers were calibrated using a Buck calibrator giving linear calibrations (Figure

3.2.4). A four-way valve is installed with inlets from the oxygen and He streams. One outlet

stream from the four-way valve goes to the reactor and the other to the CO oxidizer. The four

way valve allows for easy switching between the He and oxygen feed to the reactor. This has

two benefits. The first is having oxygen at the CO oxidizer. The second is having a constant

oxygen supply to the FID; this helps maintain constant flame chemistry and a constant

response during the switching experiments and minimizes flow disturbances. The CO oxidizer

contains a 5wt% Pt on Al2O3 catalyst that is held constant at 300°C. The catalyst is highly

active for CO oxidation with a light-off temperature of 160°C (light-off temperature is the

temperature where 50% conversion of the reactant occurs). This ensures complete conversion

of the CO to CO2. This is needed to ensure a constant response from the FID (Figure 3.2.2).

CO has a higher sensitivity factor on the FID detector than CO2. A mass flow controller is

installed to control the flow stream from the reactor to the GC sample inlet and a backpressure

valve is used to maintain a constant pressure in the reactor system.

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Reactorwith Carbon andQuartz beads

Mass Flow ControllerTo FID

To Vent

CO Oxidizer/Pt catalyst10% O2/He

He

He

H2

Four-way valve

Relief valve

MethanizerPt Catalyst

NO/NO2

Figure 3.2.1: Reactor system setup

y = 44.378x + 8.68R2 = 0.9802

0

100

200

300

400

500

600

0 2 4 6 8 10 12 14

mV

ppm

C

Figure 3.2.2: Example of FID calibration

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The SRI-GC (gas chromatograph) has been modified to act as an on-line continuous

measurement device. The GC column is removed and the reactor effluent is piped directly to

the FID after dilution with hydrogen and helium before the FID. Flows of gases to the FID are

matched closely to the original specifications for normal operation of the GC with columns

present. Two additional catalyst beds are present inside the GC oven; an oxidation catalyst (5-

wt% Pt/ Al2O3) is added and a methanizer (Ni/Al2O3) catalyst is part of the GC FID assembly.

An excess amount of hydrogen is fed to the GC stream as a source of reductant for the removal

of the oxygen over the 5-wt% Pt/ Al2O3 catalyst. Residual oxygen removal is needed to

maintain the methanizer catalyst (Ni/Al2O3) in the reduced state. The methanizer is used to

convert the CO2 to methane, which can be detected by the FID. In addition He is added to

dilute the stream and maintain flows to the FID similar to that when a column is installed in the

GC. The FID flame is maintained by using additional hydrogen and air feeds in the GC.

Flows to the FID and ratios of gases were set as close as possible to original flows with the GC

column installed in order to maintain equipment sensitivity. The gas ratios at the flame were

checked through calculation of various limiting conditions on the entire reactor system. The

graph indicates little variation in the gas ratios with the different gas concentrations and flows

used for all experiments (Figure 3.2.3).

Figure 3.2.3: Calculated FID flame chemistry limiting O2 cases

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3.2.2 Reactor loading

Carbon samples diluted with Aldrich–325 mesh SiO2 were loaded into quartz reactors. Sample

carbon /diluents ratios were 0.04 to 0.08. Carbon samples of about 3 mg were measured on a

microbalance (Mettler Toledo Model #AJ100) with 0.0001 g resolution. The reactors were

washed with nitric acid and then rinsed with deionised water to remove any alkalis from the

surface before loading the carbon samples. Quartz wool is used on both ends of the sample to

prevent entrainment of the sample in the gas stream. A type K, 0.2mm O.D., thermocouple

was placed inside a quartz 1/8” O.D x 0.25mm I.D. sheath. The thermocouple was positioned

0.5 cm above the reactor bed. The reactor furnace was controlled using an OMEGA CNi3244-

C24 controller with temperature feedback from the thermocouple. Temperature data were

collected every 5 seconds using an Omega OM-CP-Quadtemp temperature data logger.

The reactions were run via one of the following experiments described below. All experiments

began by warming up the gas flow meters for a minimum of ten minutes and setting desired

flows. Typically, total gas flow through the reactor was held constant at 15 cc/min giving a

space velocity through the reactor bed of 7000h-1 (STP). Deviations from this flow are

described in the individual experiments. At the beginning of the experiment, helium flushed

residual air through the reactor system giving a peak on the detector attributed to atmospheric

CO2 levels of about 370ppm undiluted.

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Figure 3.2.4: Example of flow controller calibration

3.2.3 Data analysis

Collected FID traces are calibrated by correcting the calibration factor to give a total carbon

conversion of 99%. All runs are to complete burn off of carbon. This is verified by increasing

the reactor temperature and monitoring when the FID signal returns to baseline at the end of

the experiment. Visual inspection of the reactor tube also confirms complete reaction of the

carbon samples. Calibration of the FID detector by diluting a 1%CO/1%CO2/balance He

mixture gives a linear curve for the analysis ranges of the experiments described here. At

maximum CO2 production the oxygen conversion is 10%; this maintains a differential type

reactor. At high carbon conversion (~90%) the calculated rate data (RG) are not very reliable

due to possible mass transfer effects and the small carbon quantities 264.

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4 Reactivity Studies

In this section soot and carbon oxidation rates are measured and discussed to address two

questions:

1) Can low temperature oxidation occur at sufficient rates to satisfy the criteria for steady

state operation of DPM established in Chapter 2? In addition to published data,

experimental data are presented at selected conditions and compared with these

requirements. The experimental data cover steady state rates at isothermal conditions

as well as temperature programmed oxidation procedures. A brief catalyst-screening

program is described in Appendix A.

2) Are there time-dependent changes in the reactivity of soot? Here, information is

presented to address the effects of temperature and gas composition changes on the

reactivity of carbon, eventhough the reactivity of carbon is a function of many

parameters. In other words, does annealing affect the reactivity of carbon?

4.1 Introduction

In this study, two approaches were used to evaluate catalysis of the carbon oxidation reaction

to meet steady state gasification rates at 200°C. The first is a survey of published catalyst

reactivity and a comparison to the gasification criteria discussed in Chapter 2.7. The second

involves evaluating two catalysts for their maximum reactivity. The two catalysts (Na-NIST

and K-NIST) were chosen because of their high reactivity as displayed in screening

experiments and literature surveys. Early reports by various authors show that alkali metals are

more reactive than other base metals for the oxidation of carbon with oxygen feed streams 21,167,170,207. The most promising catalytic candidates for meeting the required reaction rates for

the criteria in this thesis are the alkali metals. Alkali metals have high mobility and tend to

decorate the edge carbons where the carbon is the most reactive 207. However, alkali metals are

not attractive for DPF type systems due to their mobility and tendency to migrate into the

cordierite material 201,220. Nevertheless, due to their high initial reactivity we have tested these

materials and others (see Chapter 3 and Section 8.1:Appendix A for preparation and rapid

screening experiments, respectively) for their ability to catalyze the O2- carbon and NO2 –

carbon reactions and to meet the required criteria levels using screening experiments. The

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results of rapid screening evaluation experiments indicate that these two catalysts (Na-NIST

and K-NIST) show the best low temperature performance and are further discussed later in this

chapter.

Base case experiments were performed in oxygen and nitrogen oxide atmospheres with non-

catalyzed NIST and catalyzed NIST soot (K-NIST, Na-NIST) using temperature programmed

oxidation experiments. These types of experiments involve reacting the carbon sample with an

oxidant and ramping the temperature at a known controlled rate. The data collected in these

experiments were plotted on the previously described gasification plot (Figure 2.2.5) to

determine if they meet the criteria levels of normalized rate (RGo) of 0.5 at 200°C. As

discussed in Chapter 3, the catalysts are applied to the carbon by wet impregnation and

correspond to a tight contact 201. This gives maximum rates and allows the testing of the

criteria limit established in Chapter 2 of RGo = 0.5 at 200°C.

Furthermore selected experiments were performed to evaluate annealing effects on the carbon

samples. The thermal history of the carbon can influence the reactivity of carbon as shown in

Senneca et al. 131-133. Exposure of the carbon to high temperatures can cause loss of surface

area and loss of functional groups on the carbon surfaces and edges. In the oxidizing

atmosphere of a particulate filter the soot can be reacted with oxygen or possibly annealed to

remove sites for oxidation. Both of these processes could occur simultaneously and would

affect the reaction rate of the carbon. Information on low temperature thermal annealing of

carbon is difficult to find in the literature, however high temperature annealing (>900°C) has

been investigated on coal chars and formaldehyde resin chars 90,131-133. Thus, a preliminary

investigation to evaluate the influence on the reactivity of the carbon used in this study is

discussed here. These experiments include gas composition changes performed under

isothermal conditions as well as temperature excursions under non-reactive gas conditions.

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4.2 Overview: This chapter is organized in the following sections:

4.1) A survey of published carbon reactivity measurements and a comparison of these

rates to the reactivity targets discussed in Chapter 2.

4.2) Temperature programmed oxidation studies of the reactivity of the thesis samples to

compare with published data in 4.2.

4.3) Temperature programmed oxidation studies of the thesis carbon materials under

various NO2 and O2 atmospheres. These conditions are chosen to achieve the

maximum rate expected in typical diesel exhaust.

4.4) Temperature programmed oxidation experiments with selected catalysts known to

maintain intimate contact with carbon. These catalytic rates are compared to the

criteria discussed in Chapter 2.

4.5) Thermal annealing experiments to test the effect of annealing period in inert gas on

the isothermal reactivity of the carbon materials.

4.6) Temperature programmed oxidation experiments to test the effect of annealing on

the reactivity of selected catalyzed carbon samples in a NOX gas atmosphere.

4.3 Published carbon reactivity studies

While the kinetics and mechanism of carbon oxidation have received a great deal of research

attention over the years, there are little relevant data for carbon reactivity under the conditions

of interest here - namely catalyzed oxidation at low temperatures near 200°C, particularly with

species other than molecular oxygen. The existing reports are diverse and include (1) ignition

temperature measurements where steady state rates are difficult to extract 265-267, (2)

temperature programmed reaction measurements which allow better inter-comparison of

oxidation catalysts and atmospheres, but absolute rates are not readily available from these

studies. Recently, a few papers have been published to address the kinetics of diesel soot: O2-

DPM 68-70, NO2, O2 + DPM 268,269 and NO2, O2 + DPM with catalyst 76,77,270. In addition, many

of the studies that use engine exhaust provide clear measurements of the efficacy of a given

system, but they are difficult to relate to other measurements because of incomplete

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characterization of the carbon mass, the gas atmosphere, or other key reaction condition

parameters.

4.3.1 Survey of literature carbon oxidation rates with NOX

Table 4-1 collects the published studies used here. This literature can be classified in two

categories: 1) Measurements of gasification rates, RG, as described in Chapter 2.2) The

measure of site-specific rates or turnover frequencies (TOF). The latter include microscopic

studies of the edge recession rate on graphite. Here, gasification rates are calculated from

literature values and plotted on the gasification plot. Although the catalytic literature is

diverse, the study takes literature data that lend itself to this type of analysis 99,271-274 (Figure

4.3.1). Only data using NO + O2 and NO2 have been included in the analysis because NO2 has

been shown to be more active than molecular oxygen 74,75. The literature covers catalysts with

reported good contact 99, various base metals, precious metal catalysts, combinations of the

above, as well as two non-catalyzed NO2-carbon studies 271,272 (see Table 4.1). The table also

indicates the carbon sources that include carbon black, graphite and various sources of diesel

soot. Typical minimum data used to complete this analysis are rate data with partial pressures,

the catalyst type, oxidant types, flow rates and reaction temperatures, and carbon mass.

Analyses include interpolating rate data, extracting rate data from TPR (Temperature

Programmed Reaction) data through leading edge analysis, and determining rate data from

TGA (Thermal Gravimetric Analysis) data. Very rarely are actual rate expressions reported in

the literature 74,75,199,275 . Many papers report only peak temperatures or some do not indicate

the catalyst type 136,140,144,146,276. These incomplete studies are not included in this analysis. In

other papers, rates are calculated from the slopes of mass carbon removed per time at known

temperature or taken directly from rate versus temperature curves. These derived rates are

normalized to the starting carbon mass or area under the rate versus time curve. In order to

compare the literature values on the same basis, the derived rates are extrapolated to 200°C by

assuming Arrhenius temperature dependence and corrected for different NOX gas compositions

by normalizing the rate to 1000ppm total NOX (NO + NO2) assuming first order kinetics.

Whenever possible calculation of the steady state gasification rate (RGo) was performed at low

conversions of carbon or using initial rate data. In cases where data are expressed in arbitrary

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units, for example Matyshuk et al. 277, for temperature programmed oxidation (TPO), rates are

calculated at certain temperatures and then normalized using the calculated area under the

curve. These data are plotted in Figure 4.3.1.

The shaded region in Figure 4.3.1 indicates the target reactivity region established in Chapter

2. Below 200°C (1.74 e-3 /K) is the desired operating target for low temperature diesel

applications with a steady state gasification rate of 0.5 (RGo). The criterion used here was

presented in Chapter 2. This plot indicates that few of the catalysts used in this analysis meet

this low temperature requirement though some are close. Interpretation of this figure is

complicated by the differing reactant feed streams that contain varying concentrations of NO,

O2 and NO2. It is unclear whether the presence of the catalyst is catalyzing the NO + O2

reaction to NO2 and then the NO2 is reacting with the carbon or if the catalyst is helping the

NOX - carbon reaction.

What is certain is that the reactivities reported here are insufficient for continuous low

temperature operation. The reason is not clear - is the catalyst poorly distributed onto the

active carbon sites, or is the inherent reactivity of the catalyzed sites insufficient? Two

exceptions are the data labelled C and F in Figure 4.3.1. Both of these use Pt based catalysts

that are likely catalyzing the reaction of the NO + O2 reaction to NO2 and thus make the

concentration of NO2 present in the reactor uncertain. Chu and Schmidt (labelled A in Figure

4.1)271 have measured the reaction rate in nitrogen oxides of active edge carbons in graphite,

using microscopic examination of the edge recession rates or turnover frequencies. These

values were not converted into gasification rates, RG, but can be roughly estimated using

site/carbon ratio of 10% 61. Thus, the gasification rates for Schmidt’s work would be about 10

times less than the turnover frequencies presented on Figure 4.3.1. This microscopic work

follows earlier work of Thomas et al. 208, Yang et al. 122,204,213 and others 163,209,214-216,278,279 at

higher temperature conditions and with other oxidants. These rates are difficult to extrapolate

to soot carbons, but are instructive and can be used to evaluate various catalysts 216.

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Table 4-1: Information on literature data sources used in Figure 4.3.1 below

Label Catalyst Oxidant Carbon Source Analysis Reference

A None NO2 Highly oriented crystalline

graphite

STM and isothermal

heating Ind. Eng. Chem. Res. 32 271

B None NO2 Printex U TGA and Gas analysis

J. Chem. Tech. Biotec. 75 213 272

C Ce/1wt%Pt/Si-Al 250ppm NO + 10%O2 Lister Petter LPW2 NA diesel

with fuel additives Flow reactor Cat. Tod. 53 623 99

D Fe/1wt%Pt/Si-Al 250ppm NO + 10% O2Lister Petter LPW2 NA diesel

with fuel additives Flow reactor Cat. Tod. 53 623 99

E Pt/SiO2 1000ppm NO2 + 10%

O2 + 7% H2O Carbon Black TPR App. Cat. B 30 259 273

F MoO3/SiO2 1000ppm NO2 + 10%

O2 + 7% H2O Carbon Black TPR App. Cat. B 30 259 273

G V2O5/SiO2 1000ppm NO2 + 10%

O2 + 7% H2O Carbon Black TPR App. Cat. B 30 259 273

H La1.9K0.1Cu0.95V0.05O4 0.5% NO, 5% O2, He Diesel soot TPR Cat. Tod. 27 107 274

I Cu/V/K/Cl/Ti 1000ppm NO Soot from burner TPO Cat Tod. 60 43 280

J Cu/ beta 600ppm NO, 1500ppm C3H6 + 5% O2

Charcoal TPR Cat Tod. 119 262 177

K Pt/ beta 600ppm NO, 1500ppm C3H6 + 5% O2

Charcoal TPR Cat Tod. 119 262 177

L KCu/ beta 600ppm NO, 1500ppm C3H6 + 5% O2

Charcoal TPR Cat Tod. 119 262 177

N CePrOx 600ppm NO + 10% O2 Printex U TGA and flow reactor Top. Cat. (42-43) 221 281

O Pt/Al2O3 600ppm NO + 10% O2 Printex U TGA and flow reactor App. Cat. B 72 299 282

P Ru/NaY 600ppm NO + 10% O2 Printex U TGA and flow reactor App. Cat. B 72 299 282

Q KNO3 (11)/ZrO2 1500ppm NO + 8% O2 Soot (Type not indicated) TPO Cat. Comm. 4 124 193

R La0.8Bi0.2MnOx 0.5% NO2 + 10.5%O2 Diesel soot TPO Kin. Cat. 47 400 277

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50

B

C

D

E

F

G

H

I

M

O

P

Q

A

J K

N

L

0.0000001

0.000001

0.00001

0.0001

0.001

0.01

0.1

1

10

100

1000

10000

1.00 1.20 1.40 1.60 1.80 2.00 2.20 2.40 2.60 2.80 3.00

Inverse Temperature (1/K)

RGo

(mol

C/(h

*Co)

)

Target ReactionRegion

Figure 4.3.1: Literature survey of gasification rate data for catalyzed carbon reaction with NOX. Data normalized to total NOX values of 1000 ppm

50

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4.3.2 Temperature Programmed Oxidation Experiments in O2 atmosphere (with and without catalyst)

Experiments using temperature-programmed oxidation (TPO) were performed to obtain initial

gasification (oxidation) rates of the thesis carbons and provide a baseline for comparison with

subsequent data. The samples were temperature ramped at a rate of 5.8°C/min from room

temperature to the final reaction temperature of 650°C in a 10% oxygen gas stream. The high

oxygen content (10%) is near the upper limit of oxygen concentration in diesel exhaust and

provides an upper limit for the carbon oxidation rate. TPO was used primarily as a screening

tool. The parameters of sample size and ramp rate were kept constant. The quantative rate

data used later were taken from the initial low conversion part of the curve that has minimal

mass transfer effects. For information on parameters that affect TPO see Querini and Fung283

and Redhead284. Figure 4.3.2 shows a typical temperature programmed oxidation experimental

run, rate evolution and temperature with time. From this data the gasification rate (RG) at each

time is determined. Data are plotted on an Arrhenius type plot (gasification plot) (Figure 4.3.3)

to compare to the target criteria.

-2.00E-06

0.00E+00

2.00E-06

4.00E-06

6.00E-06

8.00E-06

1.00E-05

1.20E-05

1.40E-05

1.60E-05

1.80E-05

0 20 40 60 80 100 120 140 160

Time (min)

dC/d

t (m

oles

car

bon

evol

ved

per m

inut

e)

-100

0

100

200

300

400

500

600

700

Tem

pera

ture

(°C)

Figure 4.3.2: Example of temperature programmed oxidation experiment. Sample NIST, 10% O2

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The non-catalyzed NIST diesel soot–oxygen reaction rate data are compared to selected

literature data 68-70 in Figure 4.3.3. The curves (heavy lines) shown on the gasification plot are

from the present study while the literature values (symbols with thin lines) do not fall within

the target region for low temperature operation. The individual runs for NIST diesel soot

reacted with 10% O2 are very similar with an average temperature of 505°C at RG = 0.5. In

addition, the data collected in this study show good agreement with the reaction data collected

by Yezerets et al 69,70 in the temperature ranges that they studied. Yezerets et al. studied three

different engine soots with temperatures varying from 410°C to 530°C for RG = 0.5 and

varying oxygen conversions (3 to 25 vol%). Their data show a wide variation in soot reactivity

in their materials. A second feature of the curve for the NIST, O2 data is the slight plateau in

slope at 1.8 x 10-3 1/K. This curve is observed in the carbon oxidation literature and in this

case may be attributed to the soluble organic fraction of the soot 285, which contributes to a

faster rate at lower T but which is no longer present at the higher temperatures

The addition of a potassium catalyst to the soot (K-NIST) causes the C + O2 reaction to occur

at lower temperatures (~200°C lower than non-catalyzed soot (~600°C)) (see Figure 4.3.3).

An improvement in rate of a maximum of 120 times over the non-catalyzed soot sample is

observed. The slopes of the catalyzed curve and the non-catalyzed samples are similar

indicating little change in the apparent activation energy. Despite this increase in activity, the

rates with K catalyst are still too slow. These rates from the tight contact K catalyst in this

thesis compare well with other tight contact K supported materials with a carbon/catalyst

weight ratio of 1/10 (labelled S, T, U, Table 4-2), their rates are also too slow. Comparison of

this thesis’ tight contact K-catalyst to literature tight contact K2O (carbon/catalyst weight ratio

of 1/10, labelled W, Table 4-2) shows that better contact improves activity.

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Figure 4.3.3: Gasification rate plot with TPO O2 data: NIST soot and K-NIST (K/C mol ratio = 1/50) compared to Yezerets et al. 2003 70, 2005 69 data; reaction conditions: 10% O2, 7000 h-1, ramp rate 5.8°C/min, Symbols with thin lines are literature values. Heavy lines represent thesis experimental data.

Table 4-2: Information on literature data sources in Figure 4.3.3

Label Catalyst Oxidant Carbon Source Analysis Reference

R KNO3/MgO 21% O2 Carbon Black (Monarch 430) TGA and Gas analysis App. Cat. A (2006) 314 81 155

S K/CeO2 10%O2 Printex U TPO Cat Comm 8 1274 219

T K/Ce0.5Zr0.5O2 10%O2 Printex U TPO Cat Comm 8 1274 219

U K/ZrO2 10%O2 Printex U TPO Cat Comm 8 1274 219

V CeO2 10%O2 Printex U TPO Cat Comm 8 1274 219

W K2O 10%O2 Printex U TPO Cat Comm 8 1274 219

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4.3.3 Reaction testing of soot and catalyzed soot in NO2 atmosphere

Similar experiments were performed with NOX present in the gas stream. As a limiting case, a

high concentration of NO2 is used to test the criteria needed for steady state conversion at

200°C. A gas stream containing 5% NO is mixed with 10%O2/He to give a gas mixture of

2.5% NO, and 5% O2. The NO2 concentration is given by the reaction of NO + O2 NO2.

NO2 compositions are calculated using the equations of Glasson and Tuesday 286 and

information from the review by Tsukahara et al. 287. The concentration at the entrance of the

reactor bed is estimated based on the residence time from the mixing point of the reactant gas

streams to the soot bed (~ 10 seconds) but is uncertain. It is estimated that the concentration of

NO2 was a minimum of 10000 ppm. Due to the large concentrations and the uncertainty of

time the concentration of NO2 is estimated at 8000 to 12000ppm. This NO2 concentration is

obviously not a realistic NO2 value in engine exhaust (typically 1000 ppm) but is used here as a

limiting case to help establish if soot oxidation can meet the criteria.

Figure 4.3.4 compares the reaction rate in NOX to the O2 results. Addition of NO2 causes an

increase in the rate of carbon oxidation and shifts the burn-off rate curve to much lower

temperatures. Based on the criteria for steady state operation the gasification rate (RGo) of 0.5

is at 315°C. This implies that using a high concentration of NO2 cannot meet the criteria level,

although this gasification rate temperature is very high compared to others. Other workers

have reported filter balance point tests on engines as low as 250°C with NO2 223 . This could

be a result of lower engine-out carbon emissions.engine or a higher carbon oxidation rate, but

since these tests do not report engine-out carbon emissions it is impossible to compare to our

results. One possible reason for a different oxidation rate is the presence of water in the

exhaust gas. Others 74,76,288 have shown that the presence of water can improve reaction rates

of the C- NO2 reaction. Or these differences in reactivity could be due to the carbon samples.

The addition of the K or Na catalyst to the NIST sample (catalyst/carbon = 1:50 mol ratio) and

using the same NO2 gas composition gives an improvement in the rate of carbon oxidation. At

similar temperature, the rates are increased by 2 to 3 times with Na and K catalysts,

respectively, over the non-catalyzed soot. This boost in reactivity is smaller than that seen for

O2 reactions. However, these data do not clarify whether this effect is due to the catalysis of

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the NO2 carbon reaction or from the catalysis of oxidation of NO to NO2 reaction. Although

there was considerable improvement in the carbon oxidation rate, the addition of the catalyst

did not meet the targeted criteria. The best catalyst with NO2 was able to only achieve at RG of

0.5 a temperature of 250°C.

An interesting observation is that the curves from these TPO experiments are concave for all

cases studied for non-catalyzed and catalyzed soot with oxygen and NO2. This indicates that

the activation energy, frequency factor or both are changing with extent of reaction. A similar

observation is made by Yezerets et al. on O2 only experiments 70,289. In all cases, it appears

that carbon reaction kinetics is changing. The double plateau observed in the non-catalyzed O2

experiments does not exist with the NO2 and catalyzed soot experiments. This may be due to

the NO2 and catalyst improving the reaction of the adsorbed hydrocarbons on the soot.

The most favourable rate in this study, achieved at 200°C, is RGo = 0.1. This would allow

continuous operation at an engine emission rate of 0.004g/bhp-h. The data show that under the

most favourable conditions of high catalyst to carbon ratio, intimate (tight) catalyst/carbon

contact, and highly favourable gas compositions that the carbon reaction rate does not achieve

the steady state carbon oxidation rates needed for 200°C operation at the soot emission rate of

0.02 g/bhp-h. The lower emission rate of 0.004 may be achievable under some low

temperature engine operating modes such as idle or low load, low speed conditions.

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Figure 4.3.4: Gasification rate plot with non-catalyzed and catalyzed NIST samples in O2 and NO2 atmospheres: Reaction conditions: Ramp rate: 5.8°C/min, 7000 h-1, O2 runs: 10% O2, NO2 runs: 4.5% O2, 1 % NO2, 4 % NO, K-NIST sample: K/C : 1/50 mol ratio, Na-NIST sample: Na/C : 1:50 mol ratio Symbols with thin line represent literature data. Heavy lines represent thesis experimental data.

4.3.4 Thermal annealing (Isothermal experiments) O2 atmosphere

Aging of soot filter applications is mentioned often in the literature and can describe many

situations. In some cases, aging can be referring to the catalyst 3, the cordierite filter 11 and in

some cases the soot 68,70,290. As discussed previously, carbon oxidation can be affected by a

variety of factors such as contaminants, oxidant used and its thermal and chemical history, all

of which affect the active sites on the carbon. This set of experiments investigates two of the

factors that affect soot aging, thermal and gas composition effects using limiting conditions.

TPO annealing experiments were attempted but are difficult to interpret because of the

simultaneous change of temperature and carbon conversion during the experiment. Addition of

K catalyst further complicates the analysis due to decomposition of catalyst precursors and the

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mobility of the catalyst. TPO experiments are briefly discussed here but are difficult to

interpret due to the above-mentioned reasons.

4.3.4.1 Experimental procedure for annealing experiments

1) He at room temperature (~25°C) was used to purge the reactor for a minimum of 10

minutes.

2) The sample is ramped to the reaction temperature of 550°C in 15 minutes under He

and allowed to stabilize for 5 minutes.

3) Reaction

a. Base case: (B1, B2):

i. When the reactor temperature is stabilized, 10% O2/He

(15 cc/min) is switched to the reactor.

ii. The two base cases were run at a temperature of 550°C until

completion (B1 and B2). Sample B1 and B2 were both pre annealed

in He at 550°C for 30 minutes. Sample B1 is ramped at ~ 39°C/min

to 700°C and then cooled immediately to 550°C. Sample B2 is

ramped at ~ 30°C/min to 550°C similar to Sample T2 below. The

observed rise in temperature at the end of the run was intended to

burnoff any residual carbon in the reactor and complete the mass

balance.

b. Treatment 2: T2 - In-situ constant Temperature anneal (Composition

change):

i. When the reactor temperature is stabilized, 10% O2/He

(15 cc/min) is switched to the reactor.

ii. After 5 minutes, the helium is switched back to the reactor.

iii. The sample is heated for 1 hour under helium. 10% O2/He

(15 cc/min) is introduced for 5 minutes and Helium switched to the

reactor for 30 minutes.

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iv. At the end of this period, 10% O2/He is introduced to the sample and

allowed to completely react the remaining soot.

c. Treatment 3: T3 - Pre-anneal low temperature anneal with oxygen

i. Anneal carbon at 700°C.

ii. Low temperature anneal at 200°C in 10% O2 for 1 hour

iii. Isothermal burnoff at 550°C

d. Treatment 4: T4 - In-situ High Temperature Anneal

i. Same as Treatment 2: T2 with the exception at the second Helium

switch (iii) the temperature is raised to 700°C in 15 minutes and held

for 1 hour. At the end of the thermal treatment, the sample is cooled

back to the reaction temperature before switching the oxygen stream

to the reactor.

4.3.4.2 Analysis The rate is calculated at each sampling point during the burn-off curve (moles carbon

consumed with time) and normalized with respect to the initial mass of carbon loaded into the

reactor. Variability due to the sample mass loaded, sample composition variability and its

history give rate curves that vary greatly in initial reactivity. This variability in sample

reactivity makes it difficult to directly compare sample-to-sample runs. One solution is to

normalize the rate curves to the same initial conditions and plot this rate versus the fractional

conversion (fc) of the carbon. This is done in the following manner.

The ratio (A/Ao) is used here to describe the availability of the active sites by manipulation of

equation {4-1a}. A few assumptions are needed to get this ratio. First, it is assumed that the

oxygen concentration is in excess throughout the experiment. Second, it is assumed that the

carbon reaction order is pseudo first order. These assumptions reduce equation {4.1a} to

equation {4.1b} and rearrangement gives equation {4.1c}. Third, the rate constant, k, is

assumed to follow Arrhenius type kinetics {4.1d} that can be used in equation {4.1c} to give

{4.1e}. The value R/[C] represents the rate at a given fraction conversion of carbon and is

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defined as Rfc. The (R/[C]) @fc=10% is defined as a basis point for comparison and is defined

as Rfco. Cancelling the exponential terms creates the ratio of A/Ao, equation {4.2}. This is

possible because of the constant reaction temperature (isothermal conditions) and the

assumption that the activation energy is constant with carbon conversion. By using this

method of analysis, the carbon is used as an internal standard and allows for comparison

against other sample runs by reducing the effects of sample weights, sample homogeneity,

reactor effects, and differences in thermal history.

R= k [C][O2] {4-1a}

Assuming pseudo first order kinetics, and excess oxygen, Equation {4-1a} can be reduced.

R= k [C], {4-1b}

R/[C]= k, {4-1c}

k= A exp (-Ea/RT) {4-1d}

R/[C] = Rfc= A exp (-Ea/RT) {4-1e}

(R/[C])fc=10% = Rfco= Ao exp (-Ea/RT) {4-1e}

Rfc / Rfco = A/Ao {4-2}

Where fc = fractional conversion,

Rfco is the rate of carbon gasification at a fractional conversion of 10%

Ao is the frequency factor at a fractional conversion of 10%

In the results below, the initial soot amount [Co] replaces [C] above to simplify the

calculations and does not affect the comparisons made or conclusions. Plots of A/Ao versus

fractional conversion of carbon for each of the experiments are shown below.

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4.3.4.3 Results

Figure 4.3.5A gives an example of the oxidation rate of the carbon with changing time,

temperature history and oxygen pulses during the experiments. Arrows on the figure indicate

the corresponding y-axis. The square wave line indicates whether the oxygen pulse is on or

off. The gasification rate (RGo) curve indicates the evolution of carbon oxides from the carbon

surface. At the start of the experiment, the sample is temperature ramped in helium to the

reaction temperature (~550°C) and held to remove any volatiles of reactive oxygen on the

carbon surface. The reaction temperature of 550°C on this reactor set-up was chosen so that a

measurable rate of oxidation could be measured and that the reaction would be completed in a

reasonable time of 1 to 2 hours. During this temperature ramp it was observed that a peak is

present that may be attributed to the desorption of the volatile organic fraction of the soot or

reaction of oxygen containing surface functional groups and this is observed in the increase

above zero of the RGo curve at ~ 40 minutes. This indicates that oxygen-containing functional

groups on the carbon surface are reacting to release carbon oxides. After this peak is complete,

an oxygen pulse was sent to the reactor for five minutes followed by a temperature anneal in

He. Although the figure shows the oxygen is shutoff, there are still some carbon oxides

evolving. This is due to available oxygen for oxidation present in the reactor due to residence

time effects and possibly consumption of adsorbed oxygen on the carbon surface. The oxygen

pulse is repeated a second time followed by a second thermal anneal and finally a complete

carbon burn-off in oxygen. The analysis proceeds by determining the Rfc for a fraction

conversion of 10% (Rfco) and then normalizing as described above to calculate A/Ao values.

Figure 4.3.5B is created from this information and is described in detail below.

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Figure 4.3.5A

Figure 4.3.5B

Figure 4.3.5: Effect of isothermal thermal annealing: Reaction Temperature = 550°C, B1, B2: Base case- burnoff curves with 10% O2/He. T2: Step change in Oxygen concentration from 10% to 0%, Thermal annealed for 1 hour at 550°C with He only.

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4.3.4.3.1 Base case (B1, B2)

The two base cases follow the same general trend of a gradual decrease in the frequency factor

(A/Ao) with fractional conversion (fc) (Figure 4.3.5B). For these two curves, the initial 10% to

15% of conversion have similar normalized frequency factors (A/Ao). The two curves diverge

and have a maximum difference in A/Ao of 0.1. At a fractional conversion of 0.5 the base

cases have dropped on average by 25% relative to A/Ao=1 at 10% fc. This difference is

unclear and may be experimental error or possibly attributed to the pre-annealing affecting the

internal morphology and/or functional groups. In addition the 700°C treatment on sample B1

may reactivate sites on the carbon giving it better activity than sample B2.

4.3.4.3.2 Treatment T2: In-situ constant temperature anneal (Composition change)

Experiment T2 shows the same initial A/Ao for the first 10% to 15% of conversion as the base

case (Figure 4.3.5B). After the first thermal treatment, the A/Ao drops by about 40% relative

to base cases (B1 and B2). At a fractional conversion of 0.5 and higher, A/Ao is 60% less than

the initial A/Ao of 1 at 10% fc. This observation indicates that under an oxygen deficient

environment that the number of active sites on the carbon is reduced and would affect the rate

of soot oxidation with respect to the initial carbon inventory.

The above experiment would simulate a worst-case situation of an engine operating under high

loads and medium speeds where soot emissions are high and the oxygen concentration is

extremely low. Extended low oxygen environments over long periods are rare and would

never extend for 1 hour on most engines. Examples of such a low oxygen situation are a bus

going up a steep hill or a forklift lifting a heavy load. This data indicate that repeated exposure

to oxygen deficient environments could lower the reactivity by a value of 40% and would

represent an upper limit to active site loss.

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4.3.4.3.3 Treatment T4: In-situ high T anneal

This experiment is a repeat of the gas composition change experiment above with the second

anneal in He at a temperature of 700°C (Figure 4.3.6A). The ramp to higher temperature was

intended to cause further sintering and removal of adsorbed oxygen on the soot. A peak

indicating desorption of carbon oxides is observed at ~75 minutes. It was expected that a

higher temperature would cause more rapid loss of active sites and show a larger activity loss.

This was not the case. Instead the normalized A/Ao exhibits a similar change after the 700°C

anneal as seen with a 550°C anneal under He (Figure 4.3.6B). It is suspected that the higher

temperatures may have desorbed contaminants on the surface exposing active sites.

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Figure 4.3.6A

Figure 4.3.6B

Figure 4.3.6: Effect of in-situ high temperature annealing: Reaction Temperature = 550°C, B1, B2: Base case- burnoff curves with 10% O2/He. T2: Step change in Oxygen concentration from 10% to 0%, 1st Thermal anneal at 550°C for 1 hour and 2nd Thermal anneal at 700°C with He only.

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4.3.4.3.4 Treatment T3: Pre anneal at 200°C with O2: complete burnoff

In this treatment, the sample was ramped to 200°C in He and then reacted with 10% oxygen for

1hr (Figure 4.3.7). The results show no significant difference from the baseline rate curves.

This experiment was performed to simulate an engine idling for 1 hour at 200°C which then

experiences a temperature increase. What is observed is that the 200°C pre-anneal does not

appear to change the rate at higher temperatures and closely resembles the burn-off curves of

the base case burn-off curves. The short exposure to He during the purging and ramp up in

temperature to 550°C does not affect the shape and trend of the curve. The amount of burn-off

during this step change from 200°C to 550°C is about 1% of the soot mass. This low mass

burn-off is too low to cause a noticeable difference in A/Ao from the 200°C pre-anneal on the

oxidation rate of the carbon.

Figure 4.3.7: Effect of 200°C pre anneal and reaction with oxygen (T3): Temp2 = 550°C, B1, B2: Base case- burnoff curves with 10% O2/He. T2: Step change in Oxygen concentration from 10% to 0%, Thermal annealed for 1 hour at 700°C with He only. T3: Pre anneal at 200°C in He and then oxidation in O2.

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All of the above experiments show that there is an effect on carbon reactivity with changing

temperature and gas atmospheres under extreme cases. What this implies is that possible

engine load condition changes may affect the carbon reactivity during steady state operation.

Soot resident in the filter would constantly be reacting at a slower rate, as it is burned off.

During transients in engine operation the carbon reactivity could be reduced quicker by low

oxygen concentrations and high temperature excursions. In effect, the filter would eventually

accumulate low reactivity soot if a regeneration event did not occur. Although, in an actual

engine application the effects of these changes may not be clearly obvious from filter testing

due to few reports on the subject, making it likely a minor contributor to filter device

deactivation, or due to the difficulty in measuring the effect.

4.3.5 Temperature Programmed Oxidation - Thermal Annealing Experiments

4.3.5.1 NO2 atmosphere- non-catalyzed conditions (Annealing Treatments) The experiment was performed by initially annealing the carbon sample under He at the

specified annealing temperature, cooling in He and then performing a TPO experiment in a

NOX gas stream as described previously in Section 4.3.2. The annealing time (tann) was

varied to determine the effect on the reactivity. Annealing times of tann= 0, 2.5, 4, and 8 hours

were tested. The analysis of the data was performed by extracting from each individual TPO

experiment the temperatures for each fractional conversion of carbon (0, 0.1, 0.2,…1) at

similar gas composition and temperature ramp rate. A plot of the temperature at the specified

fractional conversion (Tfc) versus annealing time is shown in Figure 4.3.8A. These Tfc values

were normalized to Tfc at annealing time of 0 hours to give the ratio Tfc/(Tfc @tann=0)

(Figure 4.3.8B). The ratio gives the effect of annealing time by comparing the change in

temperature needed to give a certain fractional conversion at the same temperature ramping

rate. At a fractional conversion of 0.1, the temperature increases by greater than 1.15 times

after four hours of annealing. Further increases in annealing time give minimal changes in the

ratio. A similar flat profile is observed for fc= 0.2, 0.25, and 0.4 after 6 hours of annealing. At

high fc’s greater than 0.5 the temperature ratio is observed to trend upward while fc=0.9 trends

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linearly with temperature and does not appear to have hit a plateau. One possible explanation

is that the longer annealing exposure times at high temperature are needed to cause changes in

the active sites of the carbon. These changes could manifest as reordering of the graphene

sheets within the carbon particle reducing the surface area and thus the number of active sites.

The first 10% of fractional conversion of the carbon is likely represented by the outer layer of

the carbon particles and would be subject to initial reordering of the graphite sheets and edge

functional group reorganization. Exterior carbon lamellae of collected DPF soot particles have

greater graphitisation as observed by microstructural examination of soot particles using

HRTEM 19,113,118. Vander Wal and others also report for carbon exposed to oxygen and

temperatures present in DPF’s (200-500°C) that the interior of the particles is hollow

indicating faster oxidation of the disordered interior carbon nanostructure 19,118. These may

explain the observations seen here, that at high fractional conversions the interior of the

particle may be reordering with increasing exposure time under annealing conditions. Oxygen

concentrations at the interior of a carbon particle are uncertain and may play a role in loss of

reactivity. The oxygen-free annealing experiments performed here are limiting cases that may

reflect what is occurring during long anneal times within a carbon particle in a particulate

filter. The reordering of the interior of the particle to less reactive material or loss of reactive

sites may explain the increase in the Tfc/Tfc@tann=0 ratio at long anneal times and high

fractional conversions.

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Figure 4.3.8A

Figure 4.3.8B

Figure 4.3.8: Effect of Annealing time on Temperature for a specified fractional conversion, 5% NO2, 10% O2, Annealing Temperature: 700°C, Ramp rate: 5.8°C/min

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4.3.5.2 Annealing treatments (K catalyzed soot) A TPO annealing experiment was performed to determine the effect of annealing on the K

impregnated samples (K-NIST (K/C = 1/50)). In Figure 4.3.9, a plot of the native soot, NIST

is shown with catalyzed samples with and without thermal annealing. It is shown that all of the

catalyzed samples are reactive at much lower temperatures than the non-catalyzed soot.

Longer thermal treatments at 680°C cause a shift in the reactivity curves to higher

temperatures. A curious feature is also seen in these thermal treatments. It appears that the K-

NIST samples with thermal treatment have two reaction regimes. Although, the cause of these

two regions was not determined the following questions can be asked. Is the potassium being

encapsulated during the annealing process? Is potassium carbonate or other less reactive

species being formed at the high temperatures? Is potassium migrating to the silica diluents or

is it evaporating and being re-deposited in the cool zone of the reactor? The likely explanation

for the shift in reactivity may be gas phase mobility but further tests are required. Jelles et al.

showed at >1000K that K compounds are mobile in the gas phase, but does not indicate the

rate of gas phase mobility 291. The temperature used for annealing in this experiment is below

this temperature but some migration could have occurred either to the diluents, reactor wall, or

quartz wool. Furthermore graphitisation on the exterior of the particle could encapsulate the

mobile catalyst rendering it inactive or possibly accelerating internal particle oxidation. This

would make the reactivity measured in this experiment a function of two factors: active

catalyst concentration change and thermal annealing. Further investigations are needed to

decouple these two effects.

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Figure 4.3.9: K impregnated NIST soot (Thermal Annealing) TPO Annealing T= 680°C, K/C mol ratio = 1:50

A reactor that was used for a K catalyzed reaction was reloaded and tested for effects of any

residual K on the reactor walls. For this test the reactor contents were removed and the used

reactor (contains residual K on walls) was loaded with the non-catalyzed soot (NIST). It is

seen that at low temperature the reactivity of the soot in the used reactor is initially higher than

the NIST soot in a clean reactor but at higher temperatures it matches the clean reactor NIST

soot reactivity. The low quantity of K may have “wet” some of the carbon and this could

explain the higher low temperature reactivity. As the carbon is converted, the K was likely

unable to wet the remaining carbon and reactivity drops to that of the native soot.

The RGo versus conversion plot (Figure 4.3.10) shows that the rate is increasing with

conversion indicating that possibly more sites are catalyzed or sites being created. The valleys

are also observed in this plot. The 8h anneal under He shows a drop in reactivity at low

fractional conversions (0.4) and the 2h anneal in He having a drop in reactivity at higher

fractional conversions (0.7). This may indicate during the long annealing time that the catalyst

has migrated from the carbon and thus reduces the amount of catalyzed active sites.

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Figure 4.3.10: K impregnated Carbon (Thermal Annealing) TPO Annealing T= 680°C. Fractional Conversion versus RGo Plot

Additionally, assuming Arrhenius type behaviour, the slopes of the rate curves for the different

anneal samples containing K catalysts vary in the same manner indicating that the activation

energies are similar (Figure 4.3.11). The observed shift of the curves to higher temperatures is

due to the change in the frequency factor that indicates possible change in the number of active

sites.

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Figure 4.3.11: Comparison of slopes of rate curves. Same conditions as Figure 4.3.9

4.4 Conclusion/Summary

The data collected in both the isothermal and temperature programmed experiments support

that there is an observable change in the reactivity of carbon after exposure to high

temperatures in the absence of oxygen. Isothermal experiments indicate that the rate drops by

a maximum of 40% while TPO shows a shift in the reaction temperature to reach a specified

carbon fractional conversion. Under these conditions, it is proposed that the carbon active sites

are decreasing by either morphological changes of the carbon particle through graphite sheet

reordering and/or loss of oxygen functional groups at the carbon edges. The observed changes

in the carbon oxidation rate were low under these drastic conditions. It is practically

impossible for the collected diesel soot to not be exposed to oxygen unlike here where

extended periods of oxygen-less exposure are seen. The rate changes reported here could be

regarded as upper limits for carbon rate changes. These results show that the contribution of

thermal annealing to changes in carbon reactivity may be a minor contributor in the observed

rate of carbon trapped on real life diesel particulate filters. However under NOX gas

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conditions, a method is needed to measure in-situ NO2 creation to answer if the catalyst is

accelerating the formation of NO2 or catalyzing the C + NO2 reaction.

4.5 Future Work/Suggestions

Work here is inconclusive for determining if morphology changes and/or functional group

availability is the primary cause of rate limitations on carbon reactivity. One potential

experiment to help clarify this question is to perform longer pre-anneals and/or in situ anneals

at high temperature (700°C or higher). This would cause the surface to be cleaned of all

oxygen functional groups that would be desorbed during carbon burn-off. Extended exposure

at high temperature anneals would allow the carbon structure more time to change and stabilize

in a final structure. Each of the samples with varying degrees of anneal on the carbons would

be cooled in helium and then reoxidized in a known concentration of O2 for constant length of

time followed by a burn-off. The above experiment would indicate that the carbons reactivity

could be changed and possibly renewed. It would help confirm or deny that reactivity changes

are primarily due to the presence of surface functional groups and/or morphology changes of

the carbon.

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5 ToFSIMS study of surface functional group reactivity

5.1 Introduction

This chapter covers the study of the reactivity of the functional groups on the carbon surface

using secondary ion mass spectroscopy. As discussed in Chapter 2, the reaction mechanism of

carbon oxidation consists of a series of smaller elementary steps. These small steps in the

mechanism consist of the adsorption of the oxidant, the interaction of the oxidant with the

carbon to form surface intermediates, the formation of the product molecule and the desorption

of the product molecule 13. As described in Chapter 2, the mechanism of carbon oxidation

involves functional groups on the edge carbons of the graphite carbon sheets. These functional

groups serve as reaction intermediates and in the generic mechanism step

O2 + C (site) C(O) COx + C

C(O) represents one or more surface intermediates, i.e. functional groups on the carbon

surface. Details of these crucial steps, the formation and reaction of surface intermediates, are

not clearly understood. Additional understanding of these surface intermediates and their

reactivities may hold the key to better understanding of the carbon oxidation reaction

mechanism and possibly provide insight into how to improve the reaction. For this study, the

reactivities of the surface functional groups are measured directly and not on the basis of total

carbon.

Early reports have established that edge carbons on the polyaromatic sheets of the carbon

structure are the most reactive 61,122,213. These edge carbons react to form a variety of

functional groups that may serve as “active sites”, some playing a role as intermediates in the

gasification mechanism of the carbon. They are also responsible for the adsorption properties

of activated carbon materials. Early reports identified that active sites (discussed in detail in

Chapter 2) on the carbon surface are important to the carbon reaction mechanism 52,59,61,62.

Studies on various carbon materials (activated carbon 26,86,292, graphite 293, carbon black 18,23,30,293, soot 31,35,78, chars 30,31) have proposed that the carbon surface is populated with

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functional groups such as lactones, carboxylic acids, carboxylic anhydrides, lactols, pyrone,

and pyridine groups 16,24,293. Figure 5.1.1 shows these possible functional groups formed by

reaction with oxygen and/or water vapour and their respective decomposition temperature

ranges. These functional groups may control reactivity of the carbon sheets and are likely the

active sites. Many surface reaction schemes have been postulated and have been described in

greater detail in Chapter 2.

Figure 5.1.1: Functional groups on soot surface listed according to their thermal stability. Acidity represents only the general trend. (Muckenhuber et al.35 )

As discussed in Chapter 2, Section 2.1.3, reaction mechanisms involving such surface

intermediates have been postulated for the C + O2 and C + NO2 reactions. Nevertheless, the

reaction mechanism for carbon oxidation is uncertain. Furthermore, the species involved in the

more rapid NO2 – carbon reaction, utilized in the soot filter technology, have received much

less attention and are relatively unknown. Published reactor studies provide information on

primary and secondary product 13,61. These studies report that the reaction of carbon and

oxygen forms primarily carbon oxides above 500°C 13,61 and the reaction of C with NO2 forms

CO and NO at temperatures as low as 250°C 74,75. Isotopic labelling studies were able to

identify that carbon dioxide and carbon monoxide are both produced directly by desorption as

gaseous products from carbon-oxygen complexes on the surface 64. In all cases the oxidant

molecule is proposed to interact with a carbon site to form surface intermediates that react and

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rearrange on the surface and eventually desorb as CO or CO2. These reactor analysis

techniques, although informative, shed only limited light on the surface reaction mechanism.

The introduction of sophisticated analysis techniques that investigate the surface reactions

allowed greater insight into the reaction steps by the identification of surface groups. Early

attempts were made using surface titration experiments to identify functional groups on the

carbon surface such as lactones, carboxylic acids, anhydrides, etc 16,24. More recently, in-situ

infrared (IR) techniques give additional insight into adsorbed species on the carbon surface 26,28

and give real time information of reaction products on surfaces. DRIFTS has been used by

Fanning 30 to examine the reaction of oxygen with carbon black. More recently, Muckenhuber

et al. 35,78,79 used DRIFTS and TPD –MS to study the interaction of NO2 and commercial soots

(Printek U and Monarch 120) for the identification and reaction of surface groups. XPS was

used to give chemical oxidation states of the carbon surface and possible surface group

identification by derivatization reactions 17. Raman spectroscopy gives information on the

morphology of the carbon 123,125, but is insensitive to functional groups because of selection

rules.

A surface technique that has not been extensively studied with respect to carbon oxidation is

SIMS (Secondary Ion Mass Spectroscopy). It is a surface sensitive technique that uses ion

bombardment to release mass fragments from the sample surface and is thus capable of giving

molecular information. Despite the fact that a small fraction of the desorbed fragments are

ionized and detected, it has a high sensitivity, down to ppm levels 49,50, much greater than other

surface techniques such as XPS, which is limited to the 0.1% range. SIMS is also very surface

specific, Briggs has shown that SIMS data examine ~ 2 monolayers (10 angstroms) or less of

the surface 294. Both negative and positive ions can be measured by changing the polarity of

the detector. New TOF technology has increased the sensitivity of this technique, by detecting

all of the ions desorbed by brief pulses of primary ions. Modern ToFSIMS machines providing

high mass resolution (m/Δm of ~ 10,000) allowing for the separation of similar mass

fragments, such as S (m/z=31.9716) and O2 (m/z = 31.9898). Liquid metal ion guns allow

spatial resolution to 50 nm and new cluster ion beams provide higher yield of high molecular

weight fragments. Detailed information on the ToFSIMS technique and instrumentation can be

found in the recent book by Briggs 295 and references therein. Despite the advantages, the

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technique is difficult to quantify, due to the highly variable yields of the various secondary

ions. Furthermore, due to absence of reliable fragmentation patterns from known surface

species, the assignment of a fragment or group of fragments to a given precursor is not always

easy or possible. Nevertheless, SIMS is capable of providing molecular information with a

much higher degree of sensitivity. When combined with TPD (Temperature Programmed

Desorption) it allows relative changes of the surface composition to be followed in great detail.

The combination of SIMS and TPD was first used to study the dehydrogenation reaction of

ethylene on Pt (111) and the isotopic exchange between hydrogen and deuterium in adsorbed

ethylidyne on Pt (111) surface 296. This technique thus offers an opportunity to evaluate the

types and reactivity of the surface intermediates on the carbon that may control the oxidation

rate at different temperatures, like other ‘single step’ investigations of heterogeneous

reactions.

SIMS analyses of soot and hydrocarbons containing a few polycyclic rings have been reported 37,297-302. Simple aromatic molecules related to soot such as 1,2,3,4- tetraphenyl naphthalene

have been used to study and simulate desorption and ionization processes during SIMS 302.

Albers et al 37 studied carbon black and ‘as collected’ diesel soot before and after exposure to a

Pt catalyst using SIMS. They report the ion/C2- ratio for CH-, C2H-, C2H2

- and O-. The CH-

and C2H- are ions reported to provide differentiation between hydrogen containing species

associated with poorly crystalline and highly graphitic structures. C2-/CH- ratio was used as a

probe to investigate the efficiency of the catalyst to remove low crystalline carbon species with

high H/C ratios. C2-/C2H- ratio was used as a measure of bound hydrogen associated with bulk

carbon. An erosion test was performed for up to 10000 seconds (i.e. continuous ion

bombardment of the carbon surface); they suggest that the increasing ratio of C2- /C2H2

- with

erosion time indicates that upper layers of the carbon surface layers are being removed and the

more graphitic layers are being exposed. This interpretation is suspect, since continued ion

bombardment rearranges and decomposes the underlying layers 49,50. Large changes in all the

ratios occurred after approximately 250 seconds. Kirchner et al 297 examined diesel soot using

single particle mass spectrometry and ToFSIMS with a m/Δm of 5000. The diesel soot was

examined ‘as is’ and after exposure to ozone and alpha–pinene. They report strong positive

ion intensities for N+, K+, Fe+ and Ca+. Negative ions were composed of carbon - oxygen

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fragments, NOX products (NO2-, NO3

-) and sulphate fragments (HSO4-). Carbon core products

such as C5, C6, and C7 were less abundant.

Here we attempt to add to the current knowledge base by using the technique of TP –

ToFSIMS (Temperature Programmed Time of Flight Secondary Ion Mass Spectroscopy) to

provide molecular surface information. It is used to identify the type of surface molecular

fragments, their parent surface functional groups that may contribute to the reactivity of the

carbon and their reactivity to rearrangement and eventual gasification. In following the surface

composition with time and temperature, the reactivities of these surface functional groups can

be measured and compared with the gasification rates of soot oxidation.

5.2 Experimental Procedure

5.2.1 Sample preparation and pre-treatment Samples investigated and their treatments for this experiment are shown in Table 5-1. These

were obtained by pretreatment of the three carbon samples described in Chapter 3. Five

samples were chosen for analysis. Two of these samples are ‘as-is’ diesel soots, NIST-0

(forklift soot) and CAT-1 (engine soot from a CAT 3306). The third sample labelled NIST-

ANN is a sample of NIST-0 that received a pre-treatment of 8 hours in a He atmosphere at

700°C. These three diesel soot samples form a subset that allows the study of temperature

change of the functional groups found on the two different engine diesel soots (NIST-0 and

CAT-0). In addition, the NIST-ANN sample provides functional group information of the

cleaned soot surface after 700°C exposure.

Model char carbons, one exposed to NO and NO2 (SC_NOX) and one exposed to air

(SC_AIR), were made from pure sucrose starting material and comprise the remaining two

samples of the five samples analyzed. The sucrose char was created by heating sucrose at a

rate of 1°C/min to 400°C and held for 2 hours under air in a muffle furnace. Then, using the

reactor set-up described in Chapter 3, individual samples were initially annealed in a He

atmosphere for 8 hours at 700°C and then cooled in He. Sample SC_NOX was then prepared

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by exposing one such sample to flowing NOX (4000ppm NO, 1000 ppm NO2, 4.5% O2) at

200°C for 20 minutes. SC_NOX and SC_AIR were both exposed (max. 30 minutes) to air

(79% N2, 21% O2) during the sample mounting. The pure carbon chars allow the investigation

of the N-containing intermediates formed from NOX without interference by fragments

produced from inherent nitrogen in the soot samples. Unlike these pure carbons, the diesel

soots were exposed to NO and NO2 during their formation in the combustion chamber and

subsequent storage in the diesel particulate filter.

Table 5-1: List of Samples used in TPD-ToFSIMS analysis

Sample #: Description NIST-0 NIST as-is

CAT-0 CAT 3306 Diesel soot as-is

NIST-ANN NIST soot annealed in He at 700°C for 8 hrs, air exposure for 30 minutes at 25°C

SC_NOX

Sucrose char annealed in He at 700°C for 8 hrs, dosed with NOX for 30 minutes at 200°C, Air exposure for 30 minutes at 25°C

SC_AIR Sucrose char annealed in He at 700°C for 8 hrs, air exposure for 30 minutes at 25°C

After pre-treatment of the samples, they were mounted for analysis by pressing the carbon

powders into copper foils. The copper foil was pre-rinsed with methanol, acetone and de-

ionized water to remove contaminants and allowed to air dry prior to depositing the carbon. A

pressure of 2000 psi was used to press and immobilize the carbon particles into the ductile

copper foil substrate. The loaded foil sample was promptly placed in the vacuum chamber of

the ToFSIMS to minimize air exposure. Exposure to room temperature air was a maximum of

30 minutes. Although chemistry can occur during this exposure time the data show that

adsorbed molecules desorb during the first temperature ramping step.

5.2.2 TP ToFSIMS experiment description The TP ToFSIMS experiment is comprised of the collection of the SIMS mass spectra at

various times during a temperature program profile. ToFSIMS analysis was performed on

each sample at seven temperatures. These temperatures are room temperature (25°C), 100°C,

200°C, 300°C, 400°C, 500°C and maximum stage temperature (~550°C). A Type K

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thermocouple was mounted to the sample stage for temperature measurement. The

temperature was ramped slowly for each temperature increment, and the pressure inside the

vacuum chamber was monitored to ensure that desorbing gas did not exceed the pressure limits

of the analysis equipment. If pressures inside the chamber were found to rise too rapidly

temperature ramping was stopped until vacuum pressures dropped to acceptable levels.

Temperatures greater than 550°C were unstable due to the heated platform approaching its

maximum power output. A qualitative profile of one step of the typical experimental profile is

shown in Figure 5.2.1. The ToFSIMS spectra are acquired during periods denoted (ta).

Acquisition times (ta) were about 2 minutes in length and total acquisition time for both

positive and negative ions was about 5 minutes. The intervening temperature ramps to the next

temperature are denoted (tr). Occasionally, during the ramp to the new temperature, the

ramping had to be stopped to allow the vacuum to stabilize (ts) and for other operator

interruptions (th). Once the heated stage is at the required temperature further time may be

needed for vacuum stabilization and other operator interruptions. The heating and stabilization

cycle is repeated for all the remaining temperatures.

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Figure 5.2.1: Timing events during typical TP ToFSIMS experiments, ta= acquisition time, tr= ramp time, th = operator interruptions, ts= vacuum stabilization time

It was found that the NIST soot (NIST-0) took a long time (hours) to degas in the vacuum

chamber (i.e. vacuum stabilization) while the sucrose char time was shorter. The shorter

degassing times, the absence of organic adsorbed species and the lower initial N content levels

in the sucrose chars are the primary reasons why NOX dosing was performed on these pure

carbons instead of the diesel soot.

ToFSIMS spectrum collection was performed using an ION-TOF ToF-SIMS IV instrument

(ION-TOF, Munster, Germany) equipped with a 25 keV Ga liquid metal ion gun. Positive and

negative ion spectra were acquired from 0 to 200 m/z over a rastered area of 100 um x 100 um

while maintaining a primary ion dose below the static limit of 1013 ions/cm2. Staying below

the static limit minimizes the chance of analyzing the same region twice so that the measured

ions arise from surface undamaged by the SIMS process.

tr ts + th

ta

ts + th

tr

Tem

pera

ture

Time

ta tr ta

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5.2.3 ToFSIMS spectra, data calibration and peak assignment

All mass fragments are collected simultaneously during ToFSIMS analysis, thus creating a

large data set at each condition. Figure 5.2.2 shows a typical negative ion spectrum observed

at the indicated temperatures for sample NIST-0. Each vertical line in the Figure represents the

signal intensity of one of the masses measured by the ToFSIMS analyzer (note the logarithmic

intensity scale). Distinct fragments up to 200 amu were observed. Small (low m/z) fragments

were the most intense and the intensity decreased for heavy/more complex molecular

fragments (see Figure 5.2.2).

The processing of each individual temperature data set requires scale calibration, selection of a

spatial region of interest, subtraction of the substrate signal (Cu), recalibration of the spectra,

and assignment of the peaks. Mass calibrations are performed by identifying many known, or

expected fragments (e.g. CN-, C-, C2-, C3

-, C4- ), and assigning appropriate elemental

compositions to these fragments. The ToFSIMS software uses these values to calibrate the

entire mass scale. Calibrations for these sets of experiments were stopped at 100 mass units.

Beyond 100 mass units it was very difficult to narrow down the possible molecular formula

assignments. After calibration and with the assistance of the ToFSIMS analysis software

(IONSPEC version 4.5.0.0), each mass peak was assigned a molecular formula that best

describes its peak position and elemental composition of the sample. A spatial region of

interest was selected for an ion image of the data. The region was selected that had the highest

ion intensity and a minimum of Cu signal. The Cu signal was subtracted from the data set and

the data recalibrated with extra care taken to identify all ions containing C, H, O and N only.

In addition sulphur containing carbon compounds and metal containing fragments were

identified. A peak list was generated for each individual temperature from a single sample.

These individual peak lists were then combined to create a master peak list that was applied to

spectra for a single sample. The master peak list was truncated to contain only ions (~67 ions)

containing C, H, O, and N; this was done to make data analysis simpler.

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Figure 5.2.2: Example of TP-ToFSIMS spectra for Negative Ions – Sample NIST-0, Temperatures of spectra displayed: room temperature (~25 °C), 100 °C, 200 °C, 400 °C, and 550 °C. Y-axis: Intensity (log scale), X-axis: mass units (m/z, linear scale)

Room Temperature (~25°C)

200°C

400°C

100°C

550°C

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5.2.4 Data Analysis

An example of signal intensities for the negative ions containing C, H, O, and N of SC_NOX is

shown in Figure 5.2.3 with respect to the analysis temperatures. The labelled ions are those

that represent the highest intensities during the experiment. In this case, the light ions, H-, OH-,

C2-, C2H-, CN-, give the strongest signal intensity and are labelled in Figure 5.2.3, Panel A.

The rest are included, unlabeled, in Figure 5.2.3, Panel B, to illustrate the richness of the data

set. Some ions are observed to increase while others decrease, reflecting the formation and

decomposition of the precursor surface groups. The C2- intensity has the greatest value with

the exception of H- ion and is used as a carbon substrate reference ion for intensity changes

(discussed below).

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10000

100000

1000000

10000000

0 100 200 300 400 500 600

Temperature (°C)

log

Inte

nsity

H-

C2-

C2H-O-

OH- CN-

C-

CH-

Panel A

100

1000

10000

0 100 200 300 400 500 600Temperature (°C)

log

Inte

nsity

Panel B

Figure 5.2.3: Effect of temperature on the intensity of each individual ion for sample SC_NOX negative ions. Panel A = high intensity, low molecular weight ions: Panel B = lower intensity, higher molecular weight ion intensities (unlabeled) to show variety of temperature dependent behaviour.

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5.2.5 Reference ions and relative intensities

SIMS is inherently non-quantitative and ion yield is sensitive to surface composition. A

reference peak is used to normalize the rest of the ion intensities. Ion yields are used to

describe the number of secondary ions generated by a primary ion impact (see reference 295 for

ToFSIMS operation). Secondary ion yields can vary by several orders of magnitude across the

periodic table and are dependent on the chemical state of the surface 303. For example, a

sample could have trace amounts of Na and have high surface coverage of another element

such as Pt; the intensity of Na would be higher because of its greater tendency to create ions.

However, relative compositional information can be extracted by taking the ratio of the

intensity of the component signal with respect to the signal intensity of a chosen standard peak

(i.e. an internal standard) within the spectra. For the negative ion spectra, the C2- intensity is

the highest (with the exception of H- ion). It also is the most prominent ion in pure carbons

and graphite and clearly arises from the basic carbon structure in the absence of functional

groups on the edges of the paragraphitic carbon sheets. The C2- ion intensity is therefore used

as a carbon substrate reference ion for intensity changes of the other mass fragments.

Similarly, the C+ ion intensity is used for an internal standard for the positive ion spectra. This

method of normalization is useful to compare spectra collected at different dates. This is

discussed in more detail in Section 5.3.4.

5.2.6 Plan of data analysis

The data collected using TP-ToFSIMS are extensive and a multifaceted plan was used to

extract the information. In the results section below the data are presented firstly to illustrate

changes in overall surface composition as a function of temperature. Following this, more

detail of the speciation during thermal treatment is presented. In particular, the detailed

changes in composition of the N containing functional groups on the NOX exposed sucrose

char (SC_NOX) are examined. Finally, general data mining of the spectra using principal

component analysis (PCA) to associate groups of ions with each other was used to extract

correlations which might not be obvious to the eye, but which could reveal unexpected trends.

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5.3 Results

5.3.1 SIMS atomic composition change with temperature The atomic composition of the surface was examined to determine any trends in the surface

composition of the carbon. Atomic compositional change in the sample was determined for the

negative ions for each of the samples. First the mole fraction of C, H, O, N was calculated for

each ion fragment in the master peak list (Equation {5-1}). For example, yxj for the H atoms

(x) in ion CH3O2- (j), would be equal to 3/6.

yxj = nxj/ntj {5-1}

where ntj = total of all atoms in the ion j, nxj represents the number of atoms of element x in ion j (i.e. C, H,O, or N)

Following this, the mole fraction of a given element (x) in the complete spectrum at a single

temperature is calculated using the following:

yx sample @ T = [Σ (Ij @ T * yxj)]/ I total @ T {5-2}

Itotal @ T = Σ Ij @ T {5-3}

Where Ij @T is the ion intensity of ion j at the specified temperature, T, and I total is the sum of all ion intensities at temperature T.

Figure 5.3.1 and Figure 5.3.2 show these elemental compositions (C, H, O, and N) as a

function of temperature for SC_NOX and SC_AIR. The reader is reminded that this

information is not a quantitative measure of the atomic composition, but shows clear trends in

the atomic composition relative to temperature. Focusing on sample 3, SC_NOX, mole

fraction changes with increasing temperature, it is observed that C triples from 0.18 to 0.65, H

decreases by a two thirds from 0.6 to about 0.2, O decreases by one-half from 0.2 to ~0.08,

while N content increases ten times from ~0.01 to 0.1. Similar observations can be made for

sample 4, SC_AIR, where C triples from 0.25 to 0.68, H decreases by about one half from 0.5

to about 0.2, O decreases by a half from 0.2 to ~0.1, and N content increase five times from

~0.01 to 0.05. In both cases the amount of C and N increase while H and O decrease with

increasing temperature from 25°C to 550°C.

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0

0.1

0.2

0.3

0.4

0.5

0.6

0.7

0.8

0.9

1

25 100 200 300 400 500 550

Temperature (°C)

SIM

S At

omic

Com

posi

tion

C

H

ON

Figure 5.3.1: Elemental (C, H, O, N) SIMS spectral composition as a function of temperature for SC_NOX negative Ions.

0

0.1

0.2

0.3

0.4

0.5

0.6

0.7

0.8

0.9

1

25 100 200 300 400 500 550

Temperature (°C)

SIM

S At

omic

Com

posi

tion

C

H

O

N

Figure 5.3.2: Elemental (C, H, O, N) SIMS spectral composition as a function of temperature for SC_AIR Negative Ions.

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As can be seen from these figures, the SIMS ion spectra lose H and O and retain C and N

during the temperature program. The differences between these samples is subtle and is more

easily observed in Figure 5.3.3, which plots the relative difference (SC_AIR - SC_NOX) for

each element as a function of annealing temperature. Negative values on the plot indicate that

the element has a greater mole fraction on the non- NOX treated sample (SC_AIR) and positive

values indicate that a greater mole fraction is present on NOX -treated sample SC_NOX. We

observe that the initial mole fraction of carbon is higher on the non-treated sample (SC_AIR)

than on the NOX treated sample (SC_NOX), reflecting a higher concentration of “hetero-

atoms”. At 25°C, carbon content is ~0.35 higher on SC_AIR than on SC_NOX. As

temperature increases the carbon mole fractions approach the same value indicating no

difference in carbon content on the two samples after the surface functional groups have

decomposed. O content is higher initially on SC_AIR and at 300°C, SC_AIR appears to retain

a higher fraction. At higher temperatures, however, the SC_NOX sample appears to retain

more oxygen and overtakes SC_AIR, reaching a maximum of 0.18 at greater than 500°C.

Turning to the hydrogen content, SC_NOX exhibits a larger H fraction throughout though

there are changes in the relative composition with temperature. H content at 25°C is about

0.18 on SC_NOX and drops linearly to 0 at 200°C. It then rise to a maximum value of ~0.3 at

a temperature of 300°C followed by a second linear decrease in the ratio. The H datum point

at 300°C deviates from this linear line and shows a higher H content on SC_NOX of ~ 0.3

higher than SC_AIR. Interestingly, the N content is higher on SC_AIR at 25°C. It indicates

that these N - containing species on SC_AIR are possibly weakly adsorbed, possibly formed

during air exposure, and are readily desorbed upon temperature increase. Above 100°C, large

amounts of N are retained on SC_NOX as seen by the increase in the N mole fraction to

difference values of 0.5 at temperatures of 400°C and higher. The nitrogen content, though a

minor component of the SIMS spectra, could contain valuable information about the

mechanism of NO2 oxidation of carbon, particularly in view of the contrast between the

behaviour of these two “pure” carbons. The data indicate that N from NO2 is retained in the

char during oxidation. This observation is supported by previous reports 45,304 that have

reported that N accumulates in carbon chars as it oxidizes. The overall atomic composition is

not markedly different between NO2 and O2 exposure, however examination of the molecular

intensities show a strong difference between the two. In the upcoming sections, we will

identify the ions that are responsible for the elemental compositional changes described here.

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-0.4-0.3-0.2-0.1

00.10.20.30.40.50.6

0 100 200 300 400 500 600

Temperature (°C)

(SC_

NOX

- SC_

AIR)

/ SC

_NO

X

C

H

O

N

Figure 5.3.3: Effect of NOX treatment on sucrose char. Difference in elemental mole fractions between NOX treated sucrose char (SC_NOX) and non-treated sucrose char (SC_AIR). Positive values indicate higher mole fractions in SC_NOX. Negative values indicate higher mole fractions in SC_AIR.

5.3.2 SIMS elemental compositions of diesel soots

The elemental composition changes on the diesel soot samples NIST-0, CAT-0, and NIST-

ANN are similar to the sucrose char samples. Mole fraction changes of NIST-0 with

increasing temperature from 25°C to 550°C show that C increases from 0.22 to 0.62, a change

of three times. H decreases from 0.4 to about 0.1. O decreases similarly from 0.35 to ~0.08.

N content increases by three times from ~0.05 to 0.15 at 500°C and then remains constant

(Figure 5.3.4).

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0

0.1

0.2

0.3

0.4

0.5

0.6

0.7

0.8

0.9

1

25 100 200 300 400 500 550

Tem perature (°C)

SIM

S A

tom

ic C

ompo

sitio

n

C

N

O

N

Figure 5.3.4: Elemental Composition Change (C, H, O, N) with Temperature of NIST-0 Negative Ions.

Similarly, CAT-0 mole fraction changes with increasing temperature from 25°C to 550°C

show C increases about 3 times from 0.22 to 0.62. H decreases from 0.48 to about 0.15, about

1/3. O decreases from 0.28 to ~0.1, and N content increases five times from ~0.02 to ~ 0.1

(Figure 5.3.5).

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0

0.1

0.2

0.3

0.4

0.5

0.6

0.7

0.8

0.9

1

25 100 200 300 400 500 550

Tem perature (°C )

SIM

S A

tom

ic C

ompo

sitio

n

C

H

O

N

Figure 5.3.5: Elemental Composition Change (C, H, O, N) with Temperature of CAT-0 Negative Ions.

NIST-ANN mole fraction changes with increasing temperature (Figure 5.3.6) from 25°C to

550°C show C increases approximately three times from 0.22 to 0.7 at 500°C and remains

constant. H decreases by four times from 0.55 to about 0.15, O decreases four times from 0.18

to ~0.05, and N content increases by six times from ~0.02 to ~ 0.12.

For each of these samples, relative changes in the elemental compositions are subtle. The

relative change in carbon composition is the same from sample to sample. H and O show

slight changes with the greatest variation observed in the nitrogen content. These changes

between samples are examined more closely below.

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0

0.1

0.2

0.3

0.4

0.5

0.6

0.7

0.8

0.9

1

25 100 200 300 400 500 550

Temperature (°C)

SIM

S A

tom

ic C

ompo

sitio

n

C

H

ON

Figure 5.3.6: Elemental Composition Change (C, H, O, N) with Temperature of NIST-ANN Negative Ions.

-1

-0.8

-0.6

-0.4

-0.2

0

0.2

0.4

0.6

0.8

0 100 200 300 400 500 600

Temperature (°C)

(NIS

T-0

- NIS

T-A

NN

)/NIS

T-A

NN

CHON

Figure 5.3.7: Effect of thermal annealing at 700 °C in He on NIST diesel soot. Difference in elemental mole fractions between non-treated NIST diesel soot (NIST-0) and thermally annealed NIST soot (NIST-ANN). Positive values indicate higher mole fractions in NIST-0.

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The effect of annealing on the NIST diesel soot can be observed by examining the relative

difference in mole fraction between the NIST as-is sample (NIST-0) and the annealed NIST

sample (NIST-ANN) (Figure 5.3.7). Positive values indicate higher fractions of that element

in sample NIST-0 than in NIST-ANN. The opposite observation is seen with negative values.

C has a higher mole fraction in NIST-0 at low temperatures up to 300°C, hitting a maximum of

0.2 at 100°C. From 300 °C to 500 °C, NIST-ANN has a 0.1 higher fraction of C. At 550 °C

the two samples are equal. O mole fraction is constantly 0.4 to 0.6 higher on the NIST-0

sample from 25°C to 500 °C. At 550 °C the O content drops to 0.2. N content is higher on the

NIST-0 sample and drops with temperature from 0.6 to 0.2 between 100°C to 300°C. N

content on the NIST-0 sample remains constant until 550 °C where the N content is 0.18 more

than the annealed sample. H content is higher on the annealed sample, NIST-ANN, for all

temperatures. It increases on the annealed sample from 0.4 to 0.8 (25°C to 200°C), and goes

through a minimum of 0.4 at 300 °C. It increases to 0.6 and gradually decreases to zero

difference in H content between the two samples at 550 °C. By contrast with the sucrose char

behaviour, and though the two NIST soots begin the experiment with a different surface

composition, there is no strong contrast between the thermal behaviour of elemental species,

particularly N, on the two samples.

-3.5

-3

-2.5

-2

-1.5

-1

-0.5

0

0.5

1

0 100 200 300 400 500 600

Temperature (°C)

(SC

_NO

X - N

IST-

0)/S

C_N

OX

CHON

Figure 5.3.8: Difference in elemental mole fractions between NOX -treated sucrose char (SC_NOX) and non-treated NIST diesel soot (NIST-0). Positive values indicate higher mole fractions in SC_NOX. Negative values indicate higher mole fractions in NIST-0.

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A comparison between the ‘as-is’ diesel sample NIST-0 sample and NOX - treated sucrose char

sample, SC_NOX, shows a contrast, however. The relative differences are plotted with

increasing temperature (Figure 5.3.8), similarly to Figure 5.3.7. Again positive values indicate

a higher relative fraction on the SC_NOX sample. C has a value of –0.25 from 25 °C to 200°C

and then shifts to zero from 400 to 500 °C. O is at –0.6 at 25°C and increases to about zero

from 200 to 500°C indicating no relative difference. At 500°C the value becomes +0.25

indicating that the oxygen content is higher on the SC_NOX. H content is constantly higher on

SC_NOX at a value of 0.4 from 25°C to 500°C and drops slightly to 0.25 at 550°C. The

relative retention of H and O with increasing temperature is similar on the two materials. A

large contrast is seen in the N content, however. The initial N contents are very different,

owing to the native N in the engine-produced soot, with a difference value of –3 at 25°C. This

drops to –1 at 400°C and higher. As mentioned previously, the absolute fraction changes of N

in the ions are small, however, in one NOX exposure cycle the sucrose was able to retain N

contents similar to those in the engine produced carbon.

-1.2-1

-0.8-0.6-0.4-0.2

00.20.40.60.8

0 100 200 300 400 500 600

Temperature (°C)

(NIS

T- 0

- C

AT-

0)/N

IST-

0

CHON

Figure 5.3.9: Difference in elemental mole fractions between non-treated NIST diesel soot (NIST-0) and CAT 3306 diesel soot (CAT-0). Positive values indicate higher mole fractions in NIST-0. Negative values indicate higher mole fractions in CAT-0.

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The relative difference between mole fractions of the two engine soots (NIST-0 minus CAT-0)

is shown in Figure 5.3.9. The initial SIMS-based compositions are very similar for the two

samples; however as temperature increases some differences emerge, particularly in their H

content. The difference in H content is –0.1 and continues to decrease to a minimum of –1 at

500°C, but recovers at 550°C to nearly zero. This is odd behaviour and deviates from the trend

of decreasing H – content and may be due in part to temperature instability of the heated stage

used in the ToFSIMS analysis. This indicates that H content is higher on the CAT-0 sample

during the middle temperature range. O content is retained less well by the NIST soot as

shown by the persistent decrease in O content difference with temperature and the O content on

the CAT-0 soot eventually exceeding that on the NIST soot. Again, these two soots have

higher initial N contents, with the NIST-0 soot being consistently greater than the CAT-0.

These differences persist as temperature is raised, indicating little or no contrast in the retention

of N in these two materials.

5.3.3 General SIMS atomic change observations

A few general features are observed in the atomic changes of all the samples. The results are

no surprise, O and H content in all cases decreases with temperature while C and maybe N

content increase with temperature. The retention of N content fraction supports the

observation of Ashman and others 45,304. Interestingly, the direct involvement of NOX exposure

in the incorporation of N in sucrose char is a new finding. The two diesel soots have different

atomic compositions: CAT-0 has higher H content while NIST-0 has consistently higher N

content. However, the N retention differences are minor in the materials, which did not see an

incremental NOX exposure.

The atomic compositional data provide information during the TP experiments that real

changes are occurring to the carbon surface. The next step involves narrowing down possible

reactive groups on the carbon surface by identifying the molecular ion fragments that

contribute to these atomic changes in the carbon with temperature.

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5.3.4 SIMS molecular fragment changes

The distribution and identity of the molecular ion fragments and their individual behaviour

with temperature reveals much richer information about the identity of the functional groups on

the carbon surface and their reactivity. This additional information reveals a strong contrast

between the NO2 and O2 samples. Although ToFSIMS spectra were collected for both positive

and negative ions, the negative ion spectra gave greater molecular information. Although

metals, which are measured more easily in positive SIMS, are known to influence the oxidation

of carbon, the primary focus here will be on the C, H, O, N containing organic ions revealed in

negative ion spectra.

To begin, examples of calibrated, assigned non-normalized peaks behaviour are shown for

sample NIST-0 (Figure 5.3.10). Ions selected for this overview are based on (1) the magnitude

of their intensity changes, (2) ions that can be associated with surface functional groups

identified in the literature by other techniques (eg. CN-, OH-, O2-, CO2

-) 16,86,292,293, and (3)

possible molecular surface groups (NO-, NO2-, CO-) 27,28,35,78 that could affect carbon

reactivity. The C2- ion was used as a reference for the intensity measurements since C2

- ions

are the highest intensity peak for all temperatures (with the exception of H) and has been

shown to arise from graphite and the basic graphitic carbon structure in the soot. The raw C2-

intensity is observed to increase with temperature (see Figure 5.3.10 panel a). Conversely, OH-

ions decrease with temperature (see Figure 5.3.10 panel b). NO2- levels (Figure 5.3.10 panel c)

drop rapidly with temperature and are undetectable at 200°C and higher. The maximum

intensity of the NO2- ion is one order of magnitude less than the C2 - ion. CO2

- ions also

decrease with temperature and are two orders of magnitude less than C2- (Figure 5.3.10 panel

d). The CO- ion intensity (Figure 5.3.10 panel e) is very low and gives an example of an ion

near background levels. The CO- ion decreases with temperature and disappears into the

background at higher temperatures. O2- intensity is similar to OH- in intensity and is observed

to decrease with temperature. S- is shown because of its close proximity in mass. Although it

initially has a similar magnitude with the O2- ion, it is observed to remain relatively constant

with temperature, exhibiting a small maximum near 300°C.

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mass / u23.95 24.00 24.05

4x10

2.04.06.0

Inte

nsity

4x10

2.04.06.0

Inte

nsity

4x10

2.04.06.0

Inte

nsity

4x10

2.04.06.0

Inte

nsity

4x10

2.04.06.0

Inte

nsity

4x10

2.04.06.0

Inte

nsity

4x10

2.04.06.0

Inte

nsity

Spectrum ParameterSample ParameterSample:

Comments: ; ;

Origin:

File: PI dose:

Area / µm²: 371 x 371 um„

1.0x10ƒ… ions/cm„

Polarity:

Time / s:

negative

150 TOF-SIMS IV

File:NIST_B1.dat

File:NIST_D.dat

File:NIST_F.dat

File:NIST_H.dat

File:NIST_J1.dat

File:NIST_L2.dat

File:NIST_N1.dat

mass / u16.95 17.00 17.05

4x10

1.0

2.0

3.0

Inte

nsity

4x10

1.0

2.0

3.0

Inte

nsity

4x10

1.0

2.0

3.0

Inte

nsity

4x10

1.0

2.0

3.0

Inte

nsity

4x10

1.0

2.0

3.0

Inte

nsity

4x10

1.0

2.0

3.0

Inte

nsity

4x10

1.0

2.0

3.0

Inte

nsity

Spectrum ParameterSample ParameterSample:

Comments: ; ;

Origin:

File: PI dose:

Area / µm²: 371 x 371 um„

1.0x10ƒ… ions/cm„

Polarity:

Time / s:

negative

135 TOF-SIMS IV

File:NIST_B1.dat

File:NIST_D.dat

File:NIST_F.dat

File:NIST_H.dat

File:NIST_J1.dat

File:NIST_L2.dat

File:NIST_N1.dat

(a) Sample NIST-0: C2

- (b) Sample NIST-0: OH-

mass / u45.95 46.00 46.05

3x10

1.02.03.04.0

Inte

nsity

3x10

1.02.03.04.0

Inte

nsity

3x10

1.02.03.04.0

Inte

nsity

3x10

1.02.03.04.0

Inte

nsity

3x10

1.02.03.04.0

Inte

nsity

3x10

1.02.03.04.0

Inte

nsity

3x10

1.02.03.04.0

Inte

nsity

Spectrum ParameterSample ParameterSample:

Comments: ; ;

Origin:

File: PI dose:

Area / µm²: 371 x 371 um„

1.0x10ƒ… ions/cm„

Polarity:

Time / s:

negative

150 TOF-SIMS IV

File:NIST_B1.dat

File:NIST_D.dat

File:NIST_F.dat

File:NIST_H.dat

File:NIST_J1.dat

File:NIST_L2.dat

File:NIST_N1.dat

mass / u43.95 44.00 44.05

2x10

0.5

1.0

1.5

Inte

nsity

2x10

0.5

1.0

1.5

Inte

nsity

2x10

0.5

1.0

1.5

Inte

nsity

2x10

0.5

1.0

1.5

Inte

nsity

2x10

0.5

1.0

1.5

Inte

nsity

2x10

0.5

1.0

1.5

Inte

nsity

2x10

0.5

1.0

1.5

Inte

nsity

Spectrum ParameterSample ParameterSample:

Comments: ; ;

Origin:

File: PI dose:

Area / µm²: 371 x 371 um„

1.0x10ƒ… ions/cm„

Polarity:

Time / s:

negative

150 TOF-SIMS IV

File:NIST_B1.dat

File:NIST_D.dat

File:NIST_F.dat

File:NIST_H.dat

File:NIST_J1.dat

File:NIST_L2.dat

File:NIST_N1.dat

(c) Sample NIST-0: NO2

- (d) Sample NIST-0: CO2-

CO2

25°C

100°C

200°C

300°C

400°C

500°C

550°C

25°C

100°C

200°C

300°C

400°C

500°C

550°C

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99

mass / u27.96 27.98 28.00 28.02 28.04

1x10

1.02.03.04.0

Inte

nsity

1x10

1.02.03.04.0

Inte

nsity

1x10

1.02.03.04.0

Inte

nsity

1x10

1.02.03.04.0

Inte

nsity

1x10

1.02.03.04.0

Inte

nsity

1x10

1.02.03.04.0

Inte

nsity

1x10

1.02.03.04.0

Inte

nsity

Spectrum ParameterSample ParameterSample:

Comments: ; ;

Origin:

File: PI dose:

Area / µm²: 371 x 371 um„

1.0x10ƒ… ions/cm„

Polarity:

Time / s:

negative

150 TOF-SIMS IV

File:NIST_B1.dat

File:NIST_D.dat

File:NIST_F.dat

File:NIST_H.dat

File:NIST_J1.dat

File:NIST_L2.dat

File:NIST_N1.dat

mass / u31.92 31.94 31.96 31.98 32.00 32.02 32.04

3x10

0.5

1.0

1.5In

tens

ity

3x10

0.5

1.0

1.5

Inte

nsity

3x10

0.5

1.0

1.5

Inte

nsity

3x10

0.5

1.0

1.5

Inte

nsity

3x10

0.5

1.0

1.5

Inte

nsity

3x10

0.5

1.0

1.5

Inte

nsity

3x10

0.5

1.0

1.5

Inte

nsity

Spectrum ParameterSample ParameterSample:

Comments: ; ;

Origin:

File: PI dose:

Area / µm²: 371 x 371 um„

1.0x10ƒ… ions/cm„

Polarity:

Time / s:

negative

150 TOF-SIMS IV

File:NIST_B1.dat

File:NIST_D.dat

File:NIST_F.dat

File:NIST_H.dat

File:NIST_J1.dat

File:NIST_L2.dat

File:NIST_N1.dat

(e) Sample NIST-0: CO- (f) Sample NIST-0: S- and O2

- Figure 5.3.10: Example of identified peaks from TP- ToFSIMS data

Absolute intensities in SIMS often vary substantially (1) from sample to sample, (2) with the

overall composition of the sample due to so-called “matrix” effects and (3) over time due to

subtle variations in the spectrometer settings. In order to “normalize” the data for proper

comparison between different spectra and samples, the C2- ion from the basic carbon structure

was used as an internal reference to scale the intensities of the negative ions arising from the

attached functional groups. Such use of internal standards is common in SIMS investigations 49. Thus a normalized value N(x) for negative ion species x is given by

)()(

2)( −=

CIxIxN T

{5-4}

I(x) = intensity of component x at T

I(C2-) = intensity of C2

- ion at T N(x)T = Normalized intensity of ion x at temperature T

The normalized intensity ratios (N(x)T) are shown as a function of temperature for several key

ions in the panels of Figure 5.3.11. Each panel includes the results from all of the carbon

CO

O2

S

25°C

100°C

200°C

300°C

400°C

500°C

550°C

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samples. A general trend for all samples and most ions is that the normalized intensity of these

ions associated with surface functional groups decrease with temperature. This indicates that

surface coverage of functional groups responsible for these ions is decreasing on the surface.

The exception to this trend is the CN- ion. Examining samples SC_NOX and SC_AIR,

annealed char dosed with NO2 and annealed char respectively, it is observed that CN- intensity

is similar at low temperature (25°C). CN- intensity for sample SC_AIR declines gradually

with temperature as the samples are heated. Singular behaviour is shown for the NO2 dosed

sample (SC_NOX) where the CN- intensity instead goes through a peak (400°C) before

declining. The ultimate CN- intensity of the NO2 dosed sample (SC_NOX) is about double

that of the CN- intensity on the non-dosed sample (SC_AIR).

The CNO- curve for SC_NOX is also distinct. The intensity for CNO- for SC_NOX gradually

rises and reaches a maximum at 300°C. For all the other samples, the CNO- peak decreases

linearly with increasing temperature. This result indicates that there is some kind of chemistry

occurring on the surface of the SC_NOX sample.

With these principal ions, we observe ion intensity decreasing with increasing temperature with

some of the ions showing some variability between samples. It is observed that some of the

ions have varying slopes with temperature. Possibly these changes may lead to information on

the rate of change of functional groups on the surface. Some of the functional groups on the

surface could kinetically control the reaction of the carbon and would be represented by the

molecular fragments (ions) generated in the ToFSIMS analysis. This kinetic rate change of the

molecular fragments on the surface is further discussed in Section 5.3.5.

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101

Figure 5.3.11: Effect of temperature on Individual Ion intensity ratio for each sample. (Intensity scale x100) where 0= NIST-0, 1= CAT-0, 2= NIST-ANN, 3= SC_NOX, 4= SC_AIR

Earlier it is shown that atomic nitrogen is present in the samples of SC_AIR and SC_NOX

making it difficult to determine the source of the nitrogen. Despite this uncertainty, there is

substantial contrast between the behaviour of the N-containing ions on SC_AIR versus

SC_NOX. Figure 5.3.12 illustrates this for the prominent ion (CN-) ion. The ratio of I(CN-

)/I(C2-) for the SC_AIR sample is constant for all temperatures and may slightly decrease at

temperatures greater than 300°C. By contrast, SC_NOX shows the opposite behaviour for the

ratio and increases with temperature up to a ratio of I(CN-)/I(C2-) of ~ 3 , an increase of ~

12 times over SC_AIR at 550°C. Similar comparisons of the carbon – NO type ions (C3NO-

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and CHNO-) for SC_NOX and SC_AIR (Figure 5.3.13) show further contrasting behaviour.

The N = I/C2- ratio for these ions from SC_NOX goes through a maximum at intermediate

temperatures while the ratio for the same ions from SC_AIR decreases. The data would

suggest that there is an effect of NOX dosing on the sucrose char leading to nitrogen fixation on

the carbon surface possibly through a carbon - NO type intermediate.

Figure 5.3.12: Effect of NOX exposure on sucrose char. Comparison of the CN- ion between SC_NOX and SC_AIR.

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103

Figure 5.3.13: Effect of NOX exposure on sucrose char. Comparison of the CHNO- and C3NO- ion between SC_NOX and SC_AIR

The temperature dependences of the various N-containing ion fragments from the NOX treated

sample (SC_NOX) show a rich variety of behaviour. This is illustrated in Figure 5.3.14, where

the normalized intensity values N(x)T/N(x)25°C where N(x)T is I(x)T /I(C2-) T are grouped from

top to bottom in order of increasing oxidized state. The value of N(x)T can be viewed as the

pseudo concentration of the ion on the surface at that temperature and the ratio N/No (short-

hand for N(x)T/N(x)25°C) gives an indication of the amount of change in concentration of the

ion fragment precursor observed on the surface as the temperature is increased from 25°C. The

concentration of highly oxidized carbon-free ions disappears quickly before 300°C (NO-, NO2-,

NO3-) while the concentration of CHNO- containing ions remains constant or goes through a

maximum in intensity between 200 and 400°C indicating some type of chemistry occurring on

the surface in this temperature range. All of the CHN- type ions with the exception of the

C6H3N- ion increase with temperature while only ions containing NH- decrease. This

observation of the loss of oxygen containing ions and the increase in CHN- type ions gives

excellent evidence towards the surface enrichment of nitrogen on the carbon surface possibly

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caused by the reaction of NOX with carbon leaving behind N and liberating or forming a C-O

grouping on the carbon surface, as discussed in Section 5.3.8.

0%

10%

20%

30%

40%

50%

60%

70%

80%

90%

100%

25 100 200 300 400 500 550

Temperature (°C)

N/N

o

NH_3

NH_2

NH

C_6H_3N

C_3N

CHN

CN

C_3NO

CNO

CHNO

CH_2NO

C_2HNO_3

NO

NO_2

NO_3

CxHyN

CxHyOzN

NHy

Figure 5.3.14: Change in nitrogen containing ions during temperature ramping, Nitrogen, oxygen, hydrogen and carbon containing ions only shown, where N=I(x)/I(C2

-), Sample: SC_NOX. The order of the ions in the figure is identical to the list in the right hand margin.

A similar treatment for the C, H and O – containing (no N) is shown in Figure 5.3.15. Also

similar to the presentation of N-containing ions in Figure 5.18, the ion ratios N/No are ordered

from top to bottom in order of reduced to more oxidizing type of ions. The N/NO ratios for the

oxygen rich ions in the lower region of the figure decrease with increasing temperature

indicating that the carbon surface is depleting the precursors for these ions. The top region

contains ions with high H/C ratio (>0.6); these are also observed to decrease. In the middle the

opposite is observed for reduced ions with lower H/C ratio (<0.6) such as C4-, C3

-, C8-, C4H2

-,

C5H3- and others where the N/No ratios generally increase with temperature. In the

temperature range of this study, the oxygen containing ions being removed from the carbon

surface likely represent the functional groups of a carboxylic acid, lactone or carboxylic

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105

anhydride as identified by DRIFTS and TPD 35. At temperatures greater than 300°C, the ratio

of N/No for the ion fragments of CO2-, CHO2

-, CH3O-, and CHO- is negligible indicating that

these ion fragments may represent less stable functional groups such as carboxylic acid or

lactones.

Figure 5.3.15: O depletion of C, H, O only containing ions during temperature ramping. Sample:(SC_NOX) The order of the ions in the figure is identical to the list in the right hand margin.

This observation of increasing N content with higher temperatures suggests that N bonding

with the carbon structure is very stable and thus, suggests that the N is being incorporated into

the heterocyclic structure of the carbon. The mechanism of how this is happening is not clear.

One notional mechanism is that at low temperatures, the NO2 molecule can bond to the carbon

surface through either the oxygen atom or the nitrogen atom and then through some unknown

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106

rearrangement pathway the N is being incorporated into the carbon structure. Further analysis

of the ion fragments may reveal a potential reaction mechanism. Thus, the next step is to

identify the rate that the parent functional groups are leaving the surface and to identify if any

similarities exist that can help identify the surface groups and a possible reaction pathway.

5.3.5 Rate analyses of ion fragment data TP-ToFSIMS produces a rich source of data that are abundant with information. Through

further analysis it is possible to extract from this data quantitative measures of reactivity for

each of the individual ion fragments. The reader should be aware that these ion fragments can

be contributed from more than one surface functional group and thus the individual ion

reactivity can represent a number of surface functional groups with similar behaviour. By

understanding the rate of disappearance from the surface of these ion fragments, it may be

possible to (1) group ions together and to deduce the structure of the surface groups involved

and (2) evaluate the individual reactivities with respect to the specific gasification rates

required for low-temperature soot applications. Three methods were employed to extract

kinetic information from the large data sets:

A. Kinetic values are determined from spectra at each individual temperature; time of

reaction is assumed to be equal to the overall acquisition time of 5 minutes (referred

to as the “Integral Method”).

B. Kinetic values are derived from data collected during the acquisition time of a

single polarity (the “Differential method”).

C. Kinetic values from B are analyzed using a mathematical method called PCA

(principal component analysis) (the “Alternative Method”).

5.3.5.1 Method A - Integral method of rate analysis In this method, destruction rates of the individual ions were calculated from the total intensity

change between two temperatures. Specifically, the rate of change for an ion was calculated by

the following:

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107

Ro,SIMS25

21

N(x) *t N(x) - N(x)

=Δ=

T

TT {5-5}

where Ro,SIMS is the integral rate of ion x , ∆t is the difference between the time of the start of

the acquisition and the end of the acquisition (~5 minutes). The choice of this value is

discussed below. Both the positive and negative ions were evaluated in this manner.

Various values of the reaction time ∆t can be chosen from the data. Referring to the

experimental diagram in Figure 5.2.1, the ramp from one temperature to another, two time

values are recorded. The first is the time from the last data acquisition at temperature T1 to the

time of next data acquisition at temperature T2. This time increment includes the times

required for ramp, hold, stabilization, and acquisition periods (Figure 5.2.1). This value can be

estimated using the difference in the time stamp for when the spectra were saved for each

temperature (~ 50 minutes). This time value represents a minimum rate of the removal of

surface groups from the carbon over the interval at the temperature T2. An alternative value of

the rate can be estimated by assuming that all the reaction occurs at the higher temperature and

during the acquisition time of both the positive and negative spectra (~ 5 minutes). This

provides the best available lower limit to the time value and thus provides a maximum rate or

turnover frequency. This “maximum rate” method is easy to calculate and was used to obtain

an overall picture of the types of rate behaviour.

The shapes of the integral rate (Ro,SIMS) versus T plots enable a visual method (correlation-

inspection technique) to compare the rate behaviour of the ions containing C, H, O, and N.

Examples are shown of plots comparing rates for pairs of ions (Figure 5.3.16); in three of the

panels (Figure 5.3.16, a-c), the ions proportionally correlate. In one plot the behaviours of the

two ions are anti-correlated (the rate of one goes up while the other goes down) (Figure 5.3.16,

d). In the three plots with similar shaped curves the majority of the data are proportional. As

can be appreciated attempting to compare each individual ion against another ion would be

very tedious by graphical methods. The notion of correlation was used to automate the

comparisons of the entire data set, as described below.

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108

-0.0060

-0.0050

-0.0040

-0.0030

-0.0020

-0.0010

0.00000 100 200 300 400 500 600

Temperature (°C )

[Ro,

SIM

S] I

on1

(dia

mon

d)

-0.0040

-0.0035

-0.0030

-0.0025

-0.0020

-0.0015

-0.0010

-0.0005

0.0000

[Ro,

SIM

S] I

on2

(squ

are)

CHO_2

C_3H_2

a-0.0045-0.0040-0.0035-0.0030-0.0025-0.0020-0.0015-0.0010-0.00050.0000

0 100 200 300 400 500 600

Temperature (°C )

[Ro,

SIM

S] I

on1

(dia

mon

d)

-0.0060

-0.0050

-0.0040

-0.0030

-0.0020

-0.0010

0.0000

[Ro,

SIM

S] Io

n2 (s

quar

e)

C_4H_3

C_2H_2O_2

b

-0.0060

-0.0040

-0.0020

0.0000

0.0020

0.0040

0.0060

0 100 200 300 400 500 600

Temperature (°C )

[Ro,

SIM

S] I

on1

(dia

mon

d)

-0.0040

-0.0035

-0.0030

-0.0025

-0.0020

-0.0015

-0.0010

-0.0005

0.0000

[Ro,

SIM

S] Io

n2 (s

quar

e)

CHN

O

d-0.0100

-0.0080

-0.0060

-0.0040

-0.0020

0.0000

0.0020

0.0040

0 100 200 300 400 500 600

Temperature (°C )

[Ro,

SIM

S] I

on1

(dia

mon

d)

-0.0050-0.0040-0.0030-0.0020-0.00100.00000.00100.00200.00300.0040

[Ro,

SIM

S] I

on2

(squ

are)

CNO

C_5H_3

c

Figure 5.3.16 (a-d): Examples of positive and negative correlations for ion pairs of Integral rate versus Temperature. Units: h-1 panels (a,b): positive, panels (c,d): negative

In this automated procedure, the correlation coefficient (ρ) between each of the ions for the

integral rate Ro,SIMS as a function of T was calculated. The correlation function in Excel was

used, which is based on Equation {5-6 (a-c)}. It provides a mathematical method of

comparing the curve shapes regardless of magnitude. These values are collated in a correlation

matrix of all the ions. The matrix is n X n (n = 67, the number of identified ions) and half of

these values are used (~4500). The data set is reduced by extracting all the correlation

coefficients that fall within a certain range, for example between 0.9 <ρ<1 and –1<ρ<-0.9.

Further reduction of the data set was achieved by considering only the ions containing C, H, O,

and N resulting in a total of ~90 ion comparisons. Positive values of the correlation coefficient

indicate that two ions have similar proportional curves while negative correlations indicate

proportionally opposite curves with respect to T. An example of positive and negatively

correlating ions was shown in Figure 5.3.16. Note the primary and secondary axis scales are

not the same.

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109

yxyx

YXCovσσ

ρ•

=),(

, {5-6a}

where: 11 , ≤≤− yxρ {5-6b}

∑ −−−=

n

iyixi yx

nYXCov

1))((1),( μμ {5-6c}

Equation 5-6: Equation for correlation coefficient (ρ) used to determine similar curve shapes

A combination of the calculated correlation coefficients and visual inspection is used to group

the ions into similar kinetic characteristics as given by their rate versus temperature curves.

Mathematical manipulations of the matrix could have been used to associate subgroups for this

identification step, but this was not done here. A rigorous independent mathematical

evaluation of the entire data set by principal component analysis, (PCA), was performed and is

described in section 5.3.4.5. Here, however, a single ion curve was chosen and all ion curves

with correlation coefficients greater than 0.7 were grouped with that ion. Each curve shape

was visually compared as a check to ensure that the curves were similar. In cases where the

curve shape would fit another grouping better the ion was moved.

All of the 67 CHON ions were thus divided into five different groups based on their curve

shapes (Figure 5.3.17). For clarity, these ion groupings are referred to as “Sets” to avoid

confusion with the word “group” used often in this document. The Sets do not take into

account if the Ro,SIMS value is a positive or negative. The integral rate measure is admittedly

complex and is only one method to search common surface precursors for the various SIMS

ions. The integrated rate measure, Ro,SIMS, measures the net destruction rate of the yield-

weighted suite of precursors for that particular ion. In other words, changes to the rate at which

the surface ion precursors are formed from surface reactions contribute in combination with the

destruction of these same surface species. A correlation therefore only signifies that there is a

similar temperature dependence of this net destruction rate, which could appear in addition to a

constant formation or destruction rate. Hence, negative values of Ro,SIMS indicate accumulation

of the precursor for that ion and positive values imply net destruction. Since the Ro,SIMS values

are approximate derivatives of the ion intensities, an ion with positive values of Ro,SIMS which

shows a maximum in its Ro,SIMS (T) (destruction rate) curve is correlated in this procedure with

an ion with negative values whose accumulation rate is minimized at the same temperature.

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110

This procedure can identify possible correlation of part of an ion’s reaction pathways with

another, even if their intensities versus temperature is different. For example, if the Ro,SIMS

value is negative but is becoming less negative with temperature because of a greater

destruction rate, this component is correlated with an ion with positive Ro,SIMS values (net

destruction rates) which are increasing with temperature. Referring to Figure 5.3.17, Sets V, I

and II are similar in that they have a tendency towards increasing Ro,SIMS values with increasing

temperature, indicating an overall lower net rate of accumulation on the surface (negative

value) or higher rate of removal (positive value). The variations in this overall behaviour are

distinctive enough to be grouped separately, with Set I showing a two-stage behaviour with an

early maximum, while Sets II and V show monotonic increases, but with the increase in Set V

taking place at significantly higher temperatures. The remaining classes show more distinct

contrast. Set III curve goes through a maximum at intermediate temperatures, while Set IV

shows the opposite effect and goes through a minimum at intermediate temperatures. The ions

are assigned to their Sets in Table 5-2. An additional column is added here that shows ions

that do not fit any of the above sets. The ions in each column are sorted in order of decreasing

intensity.

Figure 5.3.17: Identified curve shapes for rate versus T plots grouped into Sets for sample SC_NOX. y-axis is rate, x-axis is temperature

V

I II III

IV

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111

Table 5-2: Integral rate sets, SC_NOX, Ions in bold are suspect.

CHON Total Ions 67 Curve Type I II III IV V No trend

Total 5 41 16 4 0 1 Oxidized 4 25 1 3 0 1 Reduced 1 16 15 1 0 0

Ion CNO H CN C_2O CO C_4HO O C_4 C_3HO C_3NO C_2H C_4H C_3O C_5H_3 OH C_3 C_7H_2 C_4O CH C_3H C C_3N CH_2 C_5 C_2HO CHN O_2 C_6H CHO_2 C_6 C_3H_2 C_4H_2 C_2H_2O_2 C_5H C_2H_3O_2 C_7H C_2H_3O CHNO C_3H_3O_2 C_8H C_3H_3 C8 C_2H_3 NO_3 NO_2 NH_2 CH_3 CO_2 C_4H_3 CH_3O C_3H_5O_3 C_6H_3N O_2H C_5H_2 NH_3 C_3HO_2 NH C_3H_3O C_3H_5O CHO C_2HNO_3 C_4H_3O NO CH_2NO

C_4H_5O C_2HO_2 C_4H_5

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112

Set II has the majority of the ions showing the greatest tendency towards lower accumulations

on the surface. It contains many of the negative ions with the highest intensities such as C, O,

and H. The set has 25 oxidized species and 16 reduced ion species indicating a possible net

loss of oxygen containing ions with temperature. Set III contains primarily reduced species

(16) with only one oxidized species (CHNO) showing similar behaviour. Set IV has ions with

decreasing rates with temperature although two of the ions (C2O- and C3O-) could be classified

to have a minimum in rate (not shown).

The contribution of each of the sets to the total intensity with temperature was determined

(Figure 5.3.18). For each set, the total set ion intensity was calculated by summing the

intensities of each ion contained in the set. Set II contributes more than 90% of the intensity at

room temperature and drops with increasing temperature to a final contribution of ~70% at

550°C. Set III contributes only 5% to the total intensity at 25°C but increases to 30% at

550°C. Sets I and IV, both go through maximums of less than 2% at intermediate

temperatures.

00.10.20.30.40.50.60.70.80.9

1

25 100 200 300 400 500 550

Temperature (°C)

Set

frac

tion

inte

gral

VIVIIIIII

II

III

I0.95

0.96

0.97

0.98

0.99

1

25 100 200 300 400 500 550

Temperature (°C)

Set

frac

tion

inte

gral

VIVIIIIII

II

III

IV

00.010.020.030.040.050.060.070.080.090.1

25 100 200 300 400 500 550

Temperature (°C)

Set

frac

tion

inte

gral

VIVIIIIII

I

II

Figure 5.3.18: Contribution of each integral rate set with Temperature, Top left: All Sets, Top right: Magnification of top fraction showing Sets II, III, and IV. No contribution from Set V. Bottom centre: Magnification of bottom fraction showing Sets I and II. Sample: SC_NOX

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113

5.3.5.2 Method B - Kinetic values derived from time-dependent isothermal acquisition.

The data files accumulated on the ToFSIMS apparatus preserve the time of each ion pulse

during the analysis. Thus, the ion intensity changes with time at constant temperature can be

reconstructed from the data set. While this is normally used to verify that the surface has not

been damaged and the acquisition time remained within the so-called “static limit” 295, this also

allows measurement of isothermal kinetics of the change in surface functional group. This is

similar, from a reaction kinetics point of view, to an isothermal batch reactor with data

collection over an accurately known time. We used this aspect of the data to measure

isothermal kinetics for ions with sufficient intensity. This direct measure gives relative rates at

specific surface compositions and temperatures and provides a method for further analysis.

Data from the entire sample were used in order to increase the signal / noise ratio and further

averaging over ten-primary ion pulses was performed to improve the count statistics. Finally,

the ions’ intensities were normalized to the C2- ion as before. Typical results are shown in

Figure 5.3.19 for CH–. A linear fit equation and its statistics are calculated for each of the ions

using the LINEST function in Excel. Statistics for the linear regression correlation coefficient

(r^2), standard errors for y (s (y)), slope (sem), and intercept (sb) are calculated. This

information is used to estimate a first order rate constant or turnover frequency (k) for an ion

from the ratio of the slope and y-intercept of the linear Equation {5-7}.

k (1/h) = Δ N(x)/Δ t *1/N(x)o = slope/y-intercept {5-7}

k0.1(1/h) = k * sites/C where sites/C = 0.1 {5-8}

Where N(x)o is the normalized intensity at time = 0, k represents the TOF of an ion under

differential conditions, and k0.1 represents the gasification rate of a single ion based on TOF

values calculated under differential conditions.

Equation {5-8} is used to convert the value to a bulk reactivity that can be related to the

gasification rate (RG) presented earlier in Chapter 4. Error bars are based on the calculated

standard error of y from the linear regression. Again, here the rates are net destruction rates

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114

and the k values (or TOF) can have both positive and negative values that reflect the dynamic

balance between the formation and destruction of the ion fragment precursors.

CH

1.541.561.581.6

1.621.64

0 20 40 60 80 100 120

Time (s)

Ra

tio

(I/

C2

-)

Figure 5.3.19: Time-dependent isothermal intensity changes in normalized intensity (CH- /C2-) for CH- at

25°C for sample SC_NOX negative ions. Top (a): All data during data collection, Bottom (b): The same date averaged over 10 primary ion pulses.

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115

Finally, a plot of the k values against temperature is created. Examples of these plots are

shown for CH-, CN-, CHN- and NO-, for SC_NOX negative ions. CH- ions (Figure 5.3.20a)

have negative values and indicate that surface concentrations of this type of ion are increasing

with temperature. The maximum rate of increase is seen at 200°C. Above this temperature the

CH- ions accumulate on the surface at a lower rate.

The NO- data show the opposite behaviour to the CH- ions. The k values are positive and pass

through a maximum at 300°C indicating a net loss of NO- molecule precursors on the surface

of the carbon (Figure 5.3.20b). Above 300°C the rate of loss from the surface is decreasing

until at 500°C there appears to be a net gain on the surface. CHN- and CN- ions have similar

patterns (Figure 5.3.20c,d). Their positive k values go through a maximum at 100°C and then

gradually decrease in a similar manner but with different magnitudes. This similarity between

the curve shapes is interesting and can provide information on ion fragments that are being

removed in a similar way.

CH

-0.25

-0.20

-0.15

-0.10

-0.05

0.000 100 200 300 400 500 600

Temperature (°C)

k 0.

1 (1

/h)

Figure 5.3.20a

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NO

-2.00-1.50-1.00-0.500.000.501.001.502.00

0 100 200 300 400 500 600

Temperature (°C)

k 0.

1 (1

/h)

Figure 5.3.20b

CHN

-0.40

-0.20

0.00

0.20

0.40

0.60

0 100 200 300 400 500 600

Temperature (°C)

k 0.

1 (1

/h)

Figure 5.3.20c

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CN

-0.10

-0.05

0.00

0.05

0.10

0.15

0 100 200 300 400 500 600

Temperature (°C)

k 0.

1 (1

/h)

Figure 5.3.20d

Figure 5.3.20: Effect of temperature on differential rates for CH-, NO-, CHN-, and CN- ions (Sample SC_NOX)

A similar analysis is performed as per the “Integral Method”. Curve shapes of rate versus

temperature are grouped using both the correlation coefficient and visual comparisons. The

ions are sorted into the same curve shape groups as in the “Integral Method” (Figure 5.3.21)

and shown in Table 5-3. Generally, it is difficult to identify simple universal trends in the

differential data. In all of the differential groups there is a mix of species that have different

degrees of oxidation. As discussed later, this method was compared with the integral method

used for the analysis with the PCA method as well statistical relevance of the ion.

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Table 5-3: Differential rate sets, SC_NOX. Ions in italics are suspect.

CHON Total Ions 67 Curve Type I II III IV V No trend

Count 9 22 9 9 13 5 Oxidized 6 11 4 5 7 1 Reduced 3 11 5 4 6 4

Ion C_3H_3 H C_4 CN C_3H_3O_2 C_6 CO_2 O C_4H CNO NO_2 C_2H_3 C_3O C_2H C_3 C_2HO NH_2 C_5H C_5H_2 OH C_3N C_3H_2 CH_3 C_3NO C_4O CH NO_3 C_2H_3O CH_3O C_7H_2 C_3H_5O C C_8 CHN C_3HO C_2HO_2 CH_2 C_2HNO_3 C_4H_2 C_3H_5O_3 C_4H_5 C_2O NO C_3HO_2 C_6H_3N CO O_2 CH_2NO C_4H_5O NH CHO_2 C_7H C_3H CHO C_2H_2O_2 C_4H_3O C_2H_3O_2 C_8H C_6H C_4HO C_4H_3 O_2H NH_3 C_5H_3 CHNO C_3H_3_O C_5

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-3.5E-02-3.0E-02-2.5E-02-2.0E-02-1.5E-02-1.0E-02-5.0E-030.0E+005.0E-03

0 100 200 300 400 500 600

T (°C)

k0.1

Ion1

(dia

mon

d)

-4.0E-01-3.5E-01-3.0E-01-2.5E-01-2.0E-01-1.5E-01-1.0E-01-5.0E-020.0E+00

k0.1

Ion2

(squ

are)

C_2H O_2

-0.20

-0.15

-0.10

-0.05

0.000 100 200 300 400 500 600

T (°C)

k0.1

Ion1

(dia

mon

d)

-0.10

-0.05

0.00

0.05

0.10

0.15

k0.1

Ion2

(squ

are)

CH CN

Figure 5.3.21: Examples of positive (top panel) and negative (bottom panel) correlations for Sample (SC_NOX) negative ions.

5.3.5.3 Comparison between integral and differential method

A comparison between the ions found in the integral and differential rate sets revealed that

very few of the ions correlated between the two methods. The sets created using the integral

rate data tend to be more chemically distinct than those from the differential rate sets. Only 20

of the 67 analyzed ions (34%) were in the same sets when comparing the integral and

differential methods. Combining Sets V and I from the differential method and comparing this

to Set I in the integral method raises the percentage of matching ions to 51%. The greatest

number of matches was seen with ions with the highest absolute intensity. A possible

explanation is that the samples are not changing quickly enough during the isothermal testing

period (differential rates method) to observe any measurable changes in the kinetic behaviour.

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Perhaps longer acquisition times might make it possible to measure these rates more precisely.

Of the two methods it appears that the integral method is more precise in giving a separation in

kinetically and chemically distinct ions, a possible result of the larger measurable differences

in the intensities between the temperatures during the analysis. In order to determine which

functional groups are accumulating on the surface of the carbon further analysis is needed.

An additional sorting of the ions in the integral method into categories with net positive only,

negative only, positive and negative rates was performed (Table 5-4). All ions with a positive

rate are reported in the table. Ions in this category have a majority of the rate values greater

than zero. In the positive rate category, 6 out of the 8 ions are from Set III where the ion

intensity goes through a maximum in rate with temperature. The six ions are CN-, CHN-, C4-,

C4H-, C4H2-, and C3N-. The other two ions (CNO-, C3NO-) are from Set I, where the rate

increases, and then drops and increases again.

The second category shows a near 50/50 distribution of both negative and positive rates with

increasing temperature. Two ions, C5H3- and C4O-, belong to Set I, C6

- and C8- belong to Set

III and the remaining ion C7H2- to Set III.

In the case of the negative rates, only the ions with the highest negative rates, but not

necessarily the highest absolute intensity are shown. The ions with the highest negative rate

values are primarily oxygen containing species at 200°C and all of these ions belong to Set II

(C4H5O-, C3HO2-, C3H3O2

-, C2HNO3-, C3H5O3

-, and C6H3N-). Since these ions have their

highest rate at this low temperature these ions might be weakly adsorbed species. In the case

of C2HNO3- the rate is highly negative (high rate of removal) at 200°C and drops to nearly zero

for the higher temperatures. Between the temperatures of 100 to 200°C, the parent group of

the ion may be removed or the surface reorganized. This ion may represent the base fragment

of NO2- and/or NO3

- weakly adsorbed onto a carbon site. The majority of the remaining ions

not discussed would primarily have negative rates and be comprised primarily of ions from Set

II.

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Table 5-4: Max negative and positive rate categories, SC_NOX

Ion [Temperature of

highest rate ((+) or (-))

rate)]

Positive Negative (high) Positive and negative

CN (300) C4H5O (200) C5H3 (300)

CHN (300) C3HO2 (200) C4O (300)

CNO (300) (I) C3H3O2 (200) C6 (300)

C4 (300) C2HNO3 (200) C7H2 (300)

C4H (300) C3H5O3 (200) C8 (300)

C3N (300) C6H3N (200)

C4H2 (300)

C3NO (300) (I)

5.3.5.4 Statistical relevance of ions used in sets.

The inclusion of ion fragments into an ion set for both the integral and differential methods

was determined statistically. In the case of the integral method, the error of each ions intensity

was calculated using counting statistics (i.e 1/C1/2, where C is the number of counts or

intensity). Errors that would propagate into the ion rate values were determined using standard

error calculations for addition/subtraction and multiplication/division operations

(i.e. )222 ssss cbay++= and )()()(

222

cs

bs

ass cba

yy ++= ).

A visual inspection of the ion rate versus temperature curves with error bars indicated that 8

ions were suspect. These ions were removed from the ion sets and the average rates of the sets

calculated (section 5.3.7). It was found that inclusion of these suspect ions did not change the

shape of the rate curves or their magnitudes.

Rates in the differential method use isothermal data. Linear regression of the isothermal data

gives a goodness of fit. The value r2 gives the confidence that the straight line represents the

data. An error estimate on the slope (rate of change) gives directly the uncertainty in the rate

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of change in intensity. Dividing this uncertainty by the average value gives the uncertainty in

dN/N*dt. Similarly the uncertainty in dN/No*dt is the uncertainty in the rate of change of the

intensity divided by the original N. The F-statistic was used to test if the isothermal data for an

ion was a random scatter of points with zero slopes. The F-statistic is a ratio of the variance

explained and the variance unexplained. An ion was included, if an ion for any temperature

was found to have the F statistic greater than the F critical value for an alpha of 0.1. This gives

90% confidence that the data are not a random scatter of points with zero slopes. Ten ions

were found suspect. However removal of these ions does not change the randomness of the

chemical species within the sets of the differential method. Why this difference exists is

unclear. This difference could be attributed to the time span being evaluated. The differential

method gives a snapshot of the surface reaction at a constant temperature while the integral

method consists of the reaction history during the ramp between analysis temperatures. This

would suggest that continuous ToFSIMS measurements may help clarify this difference

between the two analysis methods.

5.3.5.5 Method C - PCA method of analysis of data

Principal component analysis (PCA) uses multi-variant statistical techniques to help reduce and

simplify large data sets. PCA has recently been used to analyze ToFSIMS data, for example

protein analysis 305-307, forensic work 301 and has been used in fields of chemistry 308,309,

genomics 310 and others to interpret datasets. Large datasets such as TOF-SIMS spectrum can

be visualized as a multi-dimensional space. Comprehension of dimensions greater than three is

difficult and thus it is useful to reduce the dimensionality. This reduction can be accomplished

with the use of multi-variant techniques such as PCA that can retain a large amount of the

original information of the data set. PCA is an excellent tool for evaluating combinations of

variables that highlight possible trends in the data that may not be obvious by visual

examination.

Descriptions on the mathematics behind PCA can be found in the following references: 305,306,311-313. The input into PCA is a matrix (X) where the rows are samples (i.e. spectra at

temperature = T) and the columns are variables (i.e. ions). The inputs into each cell in the

matrix are the calculated rates for each ion at the given temperature. Prior to analysis, the data

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must be pre-processed to allow for comparisons. A few types of pre-processing are described

in the literature: mean centering, auto-scaling and others 310-313. Mean centering involves

subtracting the mean value for the columns x-bar from original data set X to create the mean

centred data set. The data set is thus centred on the origin allowing for differences in the

sample variances to be more prominent than the sample means. Mean-centering was found by

Wagner et al. 306 to be the most informative method to analyze their data to determine protein

structures.

Autoscaling means that the columns of X are adjusted to zero mean and unit variance by

dividing each column by its standard deviation. Here, the rates of ions leaving the surface are

being investigated. Recall that the ion rate is normalized with respect to the initial ion intensity

at T= 25°C. Ion intensities are a function of the ionization potential in SIMS (i.e. some ions

are more easily ionized and detected). Thus the ion rate’s magnitude will also be affected by

the ionization potential of the ion (recall the rate is normalized to T= 25°C). By auto-scaling

all of the ion rate magnitudes to similar levels the chance of biasing one ion over another is

reduced. In other words, some ions may leave the surface in the same manner (i.e. curve shape

with temperature may be similar (correlate)) but may have different magnitudes of rate. These

ions leaving the surface in the same manner could potentially be from the same surface groups

on the carbon.

The PCA method involves statistically determining the variance within the input matrix by

determining the direction of the greatest variation within the data set. This can be visualized

graphically as an axis rotation to capture the direction of greatest spread within the dataset 311,313, (see figure in Graham et al. 311). The singular value decomposition (details can be found

in 306,313 and references therein) of the resulting variance covariance matrix is determined and

used to determine scores (describes relationship between samples in the new axis system) and

loadings (describes relationship between principal components associated with these sample

scores) as shown in Equation {5-9}:

X =PTT + E {5-9}

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Where X is the auto-scaled data matrix, P is the matrix of scores and T is the matrix of

eigenvectors called loadings. The cross product of PTT contains most of the original variance

in X with the remaining variance (mostly noise) relegated to the residual matrix E.

Typically, 1 to 5 or higher principal components can be identified that will describe 100% of

the variance in the data set. Score plots can be made that describe the relationship between the

samples in the new coordinate system. Loading plots are used to describe the effect of the

principal component with the original peak data (variables). The first PC (principal

component) describes the direction of the greatest variation in the data set. The second PC

describes the direction of the second greatest variation.

5.3.5.5.1 PCA Results SC_NOX negative ions:

PCA was applied to the integral rate values of sample SC_NOX negative ions. About 60% of

the variance can be explained using a single PC, 80% with 2PC’s and 95% with 3PC’s (Figure

5.3.22, c). The biplot (Figure 5.3.22,b) gives information on the relationship of the scores and

loadings with PC1 plotted on the x-axis and PC2 located on the y-axis. The plot shows that the

variables tend to positively correlate with the high temperatures of 400 °C, 500 °C and 550 °C.

The 400 °C score datum point is not seen and is located in the centre of the loading data

variables. The 500 °C and 550 °C data points are located in the centre far right quadrant. The

loading plot (Figure 5.3.22,a) has PC1 on the x-axis with PC2 on the y-axis. Ellipses are

drawn that represent the sets discussed above in the integral rate section. Set I type ions are

found in the centre of the plot. Set II type ions are found spread in a curved band from the

upper right quadrant to the lower right quadrant. It contains the majority of the ions. Set III

type ions are found in a curved band spreading from the upper left quadrant to the upper right

quadrant. The majority of the ions in the upper left quadrant contain ions found in Set III. It

would appear that this Set could be split into two subgroups. This is shown by the addition of

dashed circles in Set III region. Set IV type ions are found from the centre of the graph to the

lower right quadrant. Set IV and Set III are located in opposite sides of the plot suggesting that

these two rate curves are anti-correlated. This is confirmed by re-examining the integral rate

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curves (Figure 5.3.21) shown above where the rate curves versus temperatures are mirror

images. The ions tend to group in the same regions as the correlation-inspection method with

the following exceptions. C5H3- and C7H2

- found in Set I and IV respectively using the

correlation inspection method are moved to Set III. These ions fit this Set better chemically

(i.e. reduced ions). CO- is found to be in the same region as Set IV ions, which are chemically

very similar. Although the agreement is excellent between the two grouping techniques, the

task of assigning boundaries to the Sets would be difficult without the initial correlation

inspection groupings.

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Figure 5.3.22: PCA Loading Plots for Sample SC_NOX negative ions: Loading plot (a) and Biplot (b) of PC1 versus PC2 (▼- scores, ♦ - loadings), Cumulative variance captured by each PC (c). Loading plots indicate identified sets within the ToFSIMS data.

a

b c

I II

IV

III

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Positive ions (~ 240 ions) for sample SC_NOX were examined using PCA. Three PC’s were

found to account for nearly 92% of the variance (Figure 5.3.23, c). The biplot shows that the

variables (loadings) are strongly correlated to the temperature from 300 to 500°C. The loading

plot of PC1 versus PC2 (Figure 5.3.23,a) shows the groupings (ellipses) of ions for the positive

ions. Sets were based on similar kinetic behaviour (i.e. same region of the loadings plot) and

attempting to group chemically similar ions in the same region. Seven groups are identified

with the set to right side of the plot containing the majority of the ions.

PCA was performed for the C, H, O and N containing ions for all samples and polarity of ions

(positive and negative). For these samples, loading plots, biplots and variance explained

versus PC plots can be found in the Appendix with plots for SC_AIR negative ions (Figure

5.3.24) shown below for reference. For all cases (positive and negative ions), there is a clear

trend of the majority of the ions grouping in a curved band on the right hand side of the PC1

versus PC2 loading plot. The ions in this set contain a mixture of reduced and oxidized ions

and tend to correlate with the higher temperatures (400°C and 500°C) used in the experiment.

As this is a first attempt to use this analysis method, the technique was not applied to all of the

PCA plots. However the PCA plots are included in the Appendix to show the variation of ions.

Additional analysis would require the intensity information collected during the ToFSIMS

experiments.

PCA alone is not capable of classifying ions into sets. It is a powerful tool to help group like

ions but does not provide enough information to determine the location of the boundaries of the

group making the assignment of these group boundaries a difficult task that requires further

assistance. Additional identification is needed along with the investigators judgement to

classify the boundaries in these regions where the group is not well defined. In this case, the

correlation inspection technique (used in Method A) was employed to examine the ion curves

in these undefined regions of the loading plot. Individual ions near an anticipated Set

boundary were compared and sorted based on their curve shapes, chemical states and the

investigators judgement. This method was found to be effective in the reduction and grouping

of the ion kinetic behaviour.

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Figure 5.3.23: PCA Loading Plots for Sample SC_NOX positive ions: Loading plot (a) and Biplot (b) of PC1 versus PC2 (▼- scores, ♦ - loadings), Cumulative variance captured by each PC (c). Loading plots indicate identified groupings within the ToFSIMS data.

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Figure 5.3.24: PCA Loading Plots for Sample SC-AIR negative ions: Loading plot (a) and Biplot (b) of PC1 versus PC2 (▼- scores, ♦ - loadings), Cumulative variance captured by each PC (c). Loading plots indicate identified groupings within the ToFSIMS data.

II

III III

I

IV

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5.3.6 Effect of temperature on individual ion sets, SC_NOX For each group of ions for SC_NOX, the individual raw ion intensities at a single temperature

(T) were summed to get the total raw ion intensity for the Set at that temperature (T) (Figure

5.3.25a). These raw total ion intensities are further normalized to the C2- reference ion to give

the normalized Set ion intensity at T and are shown in Figure 5.3.25b. Set II starts at its

maximum intensity and gradually drops until it reaches its minimum intensity at 550°C. Set III

starts at its minimum intensity and increases to its maximum intensity at 550°C. Set I intensity

rises from 25 °C until it reaches its maximum intensity at 300°C, where it then decreases until

it reaches its minimum value at 550°C. Set IV rises from 25°C to it maximum intensity at

100°C and then gradually declines to its minimum intensity at 550°C. Each of the normalized

Set ion intensities is related to the pseudo concentration of the ions in that group. This makes

it possible to relate each Set to a possible concentration of the surface functional groups on the

carbon surface that are a probable source of the Set ions.

The change in surface functional groups (normalized surface conversion) represented by each

Set of ions with temperature is shown in Figure 5.3.25c. It shows that Set II increases the

fastest and its maximum surface conversion reaches 0.96. Positive conversion values indicate

depletion on the carbon surface while negative conversion values indicate accumulation on the

surface. Set IV conversion is initially negative from 25°C to 200°C indicating creation of

parent surface functional groups of these ions. It increases in conversion at a slower rate and in

a similar manner to Set II. Set I decreases to its minimum at 300°C and a negative value of ~

0.39 and then increases to positive conversion to a maximum of 0.95 at 550°C. Set III

decreases in conversion and mirrors the decrease in conversion of Set I to 300°C. It decreases

to 0.4 at 400°C and then increases to 0 at 550°C.

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0

500000

1000000

1500000

2000000

2500000

3000000

0 100 200 300 400 500 600

Temperature (°C)

Raw

Inte

nsity

(II,

III)

0

5000

10000

15000

20000

25000

Raw

Inte

nsity

(I, I

V)

Set II

Set III

Set I

Set IV

0

5

10

15

20

25

0 100 200 300 400 500 600

Temperature (°C)

Nor

mal

ized

Inte

nsity

, (N

(x) (

II)

0

0.1

0.2

0.3

0.4

0.5

0.6

0.7

0.8

0.9

N(x

) (I,

III, I

V)Set II

Set I

Set III

Set IV

-2

-1.5

-1

-0.5

0

0.5

1

1.5

0 100 200 300 400 500 600

Temperature (°C)

Surf

ace

Con

vers

ion

base

d on

N(x

)

Set I

Set II

Set III

Set IV

Figure 5.3.25: Top (a): Effect of temperature on the non-normalized intensity of each individual Set, Centre (b): Effect of temperature on the normalized Set intensity, Bottom (c): Surface conversion of each Set with temperature

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Based on these results the following observations can be made.

1) Set II ions dominant the surface of the carbon due its high magnitude of

intensity. This set is a mixture of reduced and predominantly oxidized ions

(C*-O ions).

2) Set II ions drop in relative intensity faster than the other groups and reach a

stable surface concentration at temperatures above 400°C. This suggests the

surface oxygen level drops to a stable concentration during the temperature

programming. Works by Fanning30, Jeguirim288, Muckenhuber35,78 indicate that

between temperatures of 100 – 400°C carboxylic acid groups are unstable and

react or desorb. This suggests that the carbon surface is covered with oxygen

containing parent surface groups, possibly carboxylic acid groups.

3) Set IV ions have the lowest surface concentration and decline in surface

concentration in a similar way as Set II ions. Set IV ions consist primarily of C-

O ions. The slower rise in conversion of these surface species suggests that the

parent group containing the C-O group is more strongly bonded than the Set II

oxygen containing parent surface group. From previous work of others, the

temperature range of this desorption suggests that these ions may represent

lactones 16,24,30,35,78.

4) Set III ions increase in surface concentration with temperature up to 400°C.

Above 400°C the surface concentration decreases back to the same level as the

initial concentration at 550°C. The creation of reduced surface groups is

expected with the removal of oxygen containing groups and greater exposure of

the base carbon structure. This set contains CN- type groups. Chu and Schmidt

(1993) 271 report that during the NOX - carbon reaction CNx polymers are

formed on the surface of the carbon. Results from this work suggest that their

observation may be correct due to the increase of CN- and atomic nitrogen

increase in the surface region of the carbon.

5) Set I ions go through a maximum in surface concentration at a temperature of

300°C and then decline. This indicates the formation of surface intermediates

up to 300°C and their reaction or desorption.

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These observations suggest that during TPD under vacuum there is rapid desorption of weakly

bonded oxygen - containing molecules at low temperatures between 100 to 300°C (Set II,

possibly carboxylic acid groups). A second slightly stronger bonded oxygen group (Set IV)

desorbs from 200 to 400°C (Set IV, possibly lactones). Set I ions suggest that an intermediate

is formed on the surface of the carbon (CNO- type surface groups). Above 300°C these CNO-

groups react or desorb from the surface of the carbon. Set III parent surface groups have two

distinct regions with different rises in temperature. The first region mirrors the rise seen in Set

I from 100 to 300°C. This could be due to the formation of the reduced ions being produced

from the same reaction pathway. Above 300°C the ion surface concentration rises linearly

with temperature primarily due to the decomposition of Set I type parent surface groups.

200-300°C

Set II carbon oxygen products (CO)

Set II and Set IV C-O products (desorbed) + Set III and Set I (adsorbed)

Above 300°C

Set I desorbs rapidly (~340°C)

Set III desorbs slowly (~400°C)

5.3.7 Reactivities of surface ion precursors

5.3.7.1 TOF of ion sets leaving carbon surface In this section, the ToFSIMS data are used to derive net reactivities of the surface species

involved. These reactivities are then compared with the reactivity requirements required of a

low temperature particulate filter. The reactivity values are estimated by using the ToFSIMS

data to determine a site-specific rate of decomposition. This value is translated into an

equivalent carbon oxidation rate under the assumption of a site density on the carbon, as

discussed in Chapter 2. The assumption is made that the ions leaving the surface during

ToFSIMS analysis are a surrogate for the functional groups on the surface. Furthermore, the

functional groups desorbing from the surface during temperature ramping give possible

information on the carbon site reactivity under these analysis conditions. By using the grouped

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sets, the site specific or “instantaneous” rate (ri, sims) of the ion sets that have sufficient

reactivity to meet the required reactivity of particulate filters are determined.

ri, sims = a

i

NdtdN 1

∗ {5-10}

where dt = 5 minutes, the time of acquisition

and Na = (Ni(t) + Ni(t+1))/2

ri, sims (average) = set

ions

ionsimsi

n

r∑ ,

{5-11}

rg, sims = - simsir , (average) * fs {5-12}

where fs = carbonsites (site density)

Note, ri, sims is an instantaneous rate or TOF. It is not the same as RO,SIMS (normalized to a

constant temperature) that was used earlier for comparison purposes with other ToFSIMS data.

By knowing the specific rate of the functional groups on the carbon surface we can compare it

to the gasification rate needed for filter regeneration and determine if any of the functional

groups (ion sets) have a sufficient TOF.

Earlier in Chapter 4 and Chapter 2 we presented the gasification rate for particulate filter in the

gasification rate plot (Figure 4.3.3, Figure 2.2.5). Figure 5.3.26 presents a similar gasification

plot based on the values of rg, sims. The ri, sims values for the individual Sets are multiplied by an

assumed number of reactive sites per carbon to provide a carbon based reaction rate. The

figure shows that the gasification rate of Sets II and IV increase with temperature while Sets I

and III show a minimum in rate at 300°C. Above 300°C, Set I has a higher rate than Set III.

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-0.04

-0.02

0

0.02

0.04

0.06

0.08

0 100 200 300 400 500 600

Temperature (°C)

rg,s

ims

(1/h

) (av

erag

e)

Set I Set II Set III Set IV

Figure 5.3.26: Effect of Temperature on the gasification rate for each ion Set leaving the carbon surface. Sample SC_NOX: NOX dosed sucrose char negative ions

Figure 5.3.26 includes all ions that fit into the Set. No ions were excluded because sufficient

information to set criteria for elimination of an ion from a group is not known. The error bars

represent one standard deviation of the ion rates at a specified temperature for the ions in that

ion group (Set). All ions were included for the following reasons:

1) The ions yields are uncertain. As discussed earlier, some ions can create higher

intensities in SIMS even though the surface group concentrations are low. For example

if we consider the ion intensities of the two ions in Set II (H- and C4H5-), the intensity

of the H- ion is 1300000 at 25°C and 130000 at 550°C. The intensity of the C4H5- is

130 at 25°C and 4 at 550°C. The difference in magnitude between intensities of the

two ions is great. However, the change in intensity with temperature is similar in

magnitude. The library for mass fragments from mass spectroscopy of solid surfaces is

small unlike the available large database for gas phase molecules and thus information

on ion yields is small. Additionally the effect of temperature on ion yields is not

known for all compounds.

2) All individual ion rates have a percent deviation greater than 30% indicating that the

ion rate is changing with temperature. This was found by calculating the amount of

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change in rate with temperature by taking a single ion and averaging the rates over the

temperature range and then calculating the %deviation = stdev/average. For example,

if the % deviation is small (e.g. 10%), there is no change in rate of the ion with

temperature. However, what is considered a small deviation is difficult to determine

and thus an arbitrary number of 20% was chosen. All ions are greater than 30%

deviation suggesting changes in rate with temperature. The maximum deviation is

840%. CN- and CHN- have deviations of 550% and 500%, respectively.

Earlier we defined the steady state rate needed to achieve steady state conversion of the soot in

the exhaust stream at 200°C. The criterion used in early chapters to define an acceptable

carbon gasification rate, RGo, was 0.5 h-1 at a temperature of 200°C. Temperature programmed

oxidation reactivity data shown earlier (Chapter 4) indicate that the RGo of 0.5 at 200°C is

difficult to achieve even under highly favourable conditions such as high NO2 reactant

concentrations and the use of catalysts with intimate contact with carbon. Application of the

same criterion to the Set rates (rg, sims) shows that none of the Sets show sufficiently high rates

to meet the required carbon gasification rate. Similarly to the observed carbon gasification

rates these surface functional group reactivities only show sufficient reactivity at temperatures

greater than 400°C. The highest gasification rate at 200°C is 0.04 by Set II, this is only 2% of

the required reactivity. For most sets the specific rate reaches a maximum of 0.04 only at

temperatures greater than 400°C. All of the sets are below the criteria level and likely are

contributing to a similar reaction pathway.

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5.3.7.2 Individual ion reactivities The specific rates of selected ions were examined in a similar manner, i.e. the “gasification

rate” of a specific ion is calculated using the individual ion specific rate and correcting for site

density. The calculated gasification rates of the ions are plotted on the gasification plot using a

linear scale for the y-axis (Figure 5.3.27). As seen for the Set results above, the gasification

rates are well below the criteria turnover frequency of 0.5 for all temperatures. The SIMS

reactivities are in substantial agreement with these measurements.

For all temperatures, the Rg, sims of NO-, NO2

-, OH-, CO2-, CO- and CN- type functional groups

do not have rates that are sufficient to meet the criteria level; this indicates that these ions may

not limit the reaction rate. The sum of the rates of CO- + CO2- rises with temperature linearly.

The data indicate that all surface groups with sufficient reactivity have been removed from the

carbon leaving the less reactive groups.

Figure 5.3.27: Specific gasification reaction rate of individual ions for sample SC_NOX. The lines are included to make it easier for the reader to locate the data points and are not intended to show trends.

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5.3.8 Surface mechanistic considerations The surface reaction of carbon with oxidants as discussed earlier is not clear. In addition,

predicting molecular reactions using ToFSIMS is difficult. The technique is highly destructive

and the creation of the fragmentation pattern is not fully understood. Models using computer

simulation are in their early stages and are breaking new ground into the understanding of the

fragmentation patterns 314,315. Although it is difficult to identify the parent surface groups, here

an attempt is made to postulate surface reaction mechanisms that are supported by observations

in the literature. Surface reaction mechanisms have been proposed based on in-situ FTIR,

DRIFTS measurements 78, TPD-MS 35,79,316, reactor measurements 45,97,288 and have been used

to deduce surface reaction mechanisms. In this section we utilize the ToFSIMS data along

with PCA analysis to deduce the surface reactions occurring during the TP–ToFSIMS

experiment.

Although, the SIMS process is highly complex, there are clearly trends in the TP-ToFSIMS

data that can provide information on surface species and reaction sequences. For example, one

possible reaction sequence involves three possible surface states (Figure 5.3.28). This includes

an initial surface composition containing a number of functional groups (initial surface state -

S1, S2, S3…) that can decompose or react to form a variety of functional groups at

intermediate temperatures (intermediate surface state - I1, I2, I3…). These intermediate

functional groups can follow other reaction pathways to form a number of functional groups at

the final treatment temperatures (final surface state - F1, F2, F3…). In addition, gas phase

products (G1, G2) can be produced by reaction or desorption (e.g. carbon oxides, nitrogen

oxides, water and others). A notional surface composition for each of these states can be

surmised based on the general observations of the TP-ToFSIMS data and is summarized

below:

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Figure 5.3.28: Reaction Scheme 1

a) Low temperatures: (25°C to 200°C) (Initial Surface Composition) (S1,S2,…)

a. Surface consists of mainly oxygen containing functional groups

b. Oxidized nitrogen species are present on the surface

c. Atomic nitrogen composition is lowest at these temperatures

d. Greater number of oxidized ion species than reduced ions

b) Intermediate temperatures (Intermediate Surface Composition) (I1, I2,…)

a. Reduction in oxidized species indicating loss of oxygen containing functional

groups

b. Increase in NO ion fragments relative to starting state indicating formation of

NO containing surface functional groups

c) Higher temperatures (Final Surface Composition) (F1, F2,..)

a. Further reduction in oxidized species indicating loss of oxygen containing

functional groups and surface containing primarily reduced species.

b. Increase in atomic nitrogen composition indicating surface enrichment of

nitrogen.

c. Decrease in NO containing ion fragments relative to intermediate temperatures

indicating loss of NO containing surface functional groups

G2G1

S2

S3

I1

I2

I3

F1

F2

F3

Increasing Temperature

S1

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Using information from detailed rate analysis and published literature, the number of possible

surface functional groups can be deduced for the oxygen and nitrogen reaction pathways. This

information is discussed below and used to postulate a reaction mechanism.

5.3.8.1 Summary of oxygen dosed sample observations The oxygen reaction pathway is found from examining the SC_AIR sample TP_ToFSIMS

data. This sample was annealed at 700°C for 8 hours and cooled under a helium atmosphere.

The sample was exposed to air (20% oxygen) at room temperature (~25°C). For this sample,

PCA was used to segregate the ion fragments into groups with similar rate behaviour.

However, detailed rate analysis was not performed (i.e. segregation of ion fragments into

similar rate behaviour groups).

A cursory comparison of the PCA biplots for the negative ions of the sucrose char samples

(SC_AIR and SC_NOX (Figure 5.3.24b, and Figure 5.3.22b, respectively)) shows that the

curved ion band found on the right of the plot is shifted relative to temperature. This curved

ion band was attributed to Set II in the SC_NOX detailed rate analysis and was found to

contain primarily oxygen containing-ion fragments. While this ion band on SC_NOX is

centered over 400°C, it is shifted on the SC_AIR sample to a region between 400°C and

500°C. This would indicate a temperature delay in the evolution of the oxygen –containing

functional groups on the air-exposed sample and that the presence of NOX or different

intermediates may improve the evolution temperature. Further experimentation and analysis is

needed to confirm this observation.

The literature is populated with many studies on possible oxygen containing species on carbon.

Muckenhuber et al. 35 and references therein discuss the decomposition temperatures of various

oxygen containing species found on carbon. From this information the oxygen species being

desorbed from the SC_AIR sample between the temperatures of 400°C and 500°C may

correspond to oxygen containing functional groups such as carboxylic acids, lactones, and

carboxylic anhydrides. These surface species are formed during the air exposure or are formed

by reaction of the oxygen with carbon during the temperature ramping. Similarly these surface

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groups may be formed during the reaction of NOX with carbon. This reaction is discussed

below.

A review of the literature for SIMS fragmentation information on model compounds found

mostly positive ion spectra 301,309,317. Many of the positive ions from these model compounds

are similar to those measured on the SC_AIR sample. An attempt to relate the ToFSIMS data

to model compounds was not successful but some ion fragments for the positive ions were

similar to dibutyl phthalate 301, nitro-cellulose 301, polysaccharide coatings 317, and bisphenol-A

polycarbonate 318 and polyethyleneterephthalate (PET) blends 319. However, this comparison is

not perfect and is difficult due to the large number of ions; in addition the molecular

assignments on the SC_NOX sample may not be entirely correct at the molecular weights

greater than 100amu due to the numerous ion possibilities. Further experimentation is needed

on model compounds and analyzed using PCA to determine the source of the ions on the

carbon surface.

5.3.8.2 Summary of NO2 dosed sample observations, SC_NOX

The most interesting information is from the NOX dosed sample (SC_NOX sample). This data

were analyzed using PCA and detailed rate analysis to identify similarly desorbing ion

fragments. The TP-ToFSIMS data clearly show the carbon surface composition is changing

with temperature and can be classified into at least three observed surface states as in Scheme 1

(Figure 5.3.28) (initial surface composition-low temperature, intermediate surface

composition-intermediate temperatures and final surface composition - high temperature.).

5.3.8.2.1 Initial surface composition, SC_NOX

In the starting state (i.e. low temperatures), the SIMS indicates primarily oxygen containing

groups and oxygen containing nitrogen groups. With the application of the temperature ramp

between 25°C and 200°C, ToFSIMS data show an evolution of the oxygen containing groups.

Also in this temperature range some ions, such as the NO2- ion, show a large desorption spike.

Looking at the NO2- ion gasification rate with temperature, it is observed that the NO2

- rate is a

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maximum at 100°C and then drops rapidly to zero at 200°C. Similarly, the ion C2HNO3- is

observed to have a low gasification rate at 100°C and a high gasification rate at 200°C and then

drops to zero at 300°C. This would indicate that the ion is reducing its population on the

surface of the carbon at a desorption temperature between 100°C and 200°C. To determine the

exact temperature of desorption the TP-ToFSIMS experiment would have to be performed at

shorter temperature intervals. For these cases, the NO2- ion fragment and possibly the NO3

- ion

fragment may represent molecular NO2 adsorbed to the carbon. A related observation was

made by Azambre et al 316, who examined the reactivity of diesel soot with flowing 1000ppm

NO2/bal Ar (60mL/min) at temperatures between 25°C and 200°C using TGA, FTIR and TPD-

MS. The TPD-MS results showed that molecular NO2 is weakly bonded to the carbon surface

and is desorbed at ~60°C, while a weak desorption signal was also seen around 200°C.

Likewise, Jegurim et al 288 report that a sharp desorption peak of NO2 is observed with a

maximum at 110°C indicating that a significant quantity of NO2 was sorbed on the carbon

surface during the adsorption step and was completely desorbed by 200°C. An additional two

peaks attributed to NO and CO2 are observed simultaneously and have maximum desorption

peaks at 150°C. Additionally, Muckenhuber et al. 78 and Azambre et al. 316 suggest NO2 forms

an acidic functional group on the soot samples, which decomposes at about 140°C into CO2

and NO 78. This evidence supports the observation that the oxygen containing nitrogen ions

released during TP-ToFSIMS below 200°C are likely to arise from weakly bonded nitrogen

oxides. Based on prior IR assignments, the initial surface composition of the carbon is likely

to contain adsorbed NO2 and NO with oxygen species such as lactones, carboxylic acids, and

carboxylic anhydrides. These NO containing functional groups would need to react with the

carbon to account for the increase in N content in the final state.

5.3.8.2.2 Final surface composition, SC_NOX

The TP_SIMS experiment suggests that the surface of the carbon is enriched with nitrogen

after exposure to nitrogen oxides however the mechanism for this enrichment is uncertain with

little evidence in the literature. There are reports that can help identify the carbon – nitrogen

surface functionalities 45,86,97,304. Biniak et al. 86 used XPS to identify the surface functional

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groups of a commercial activated carbon (D43/1) after each individual treatment. The

treatments included de-ashing and high temperature annealing (1000K) under vacuum (10-2 Pa)

followed by oxidation with nitric acid at 353K or ammonia treatments at >1000K. The surface

is reported to contain primarily pyridinic structures after the initial high temperature anneal and

subsequent low temperature nitric acid treatment. This suggests that this low temperature acid

treatment was inadequate to modify the surface and possibly high temperatures are needed to

cause N to be incorporated into the ring. In addition, Kaptejin et al 304 used XPS to study

nitrogen functionality development during burnoff on model chars (sucrose and

phenolformaldehyde) after high temperature (1373K) exposure in N2 followed by CO2 (900°C)

and O2 (580°C) exposure. After the high temperature exposure in N2, they report the presence

of pyridinic nitrogen, pyridones, and oxidic nitrogen species on the edge of the graphene

structure with quaternary nitrogen incorporated in the structure. Suzuki et al. 97 also observed

the incorporation of N during the reaction of C + NO at 600°C by XPS and reaction studies.

However, XPS results on the initial surface composition of the SC_NOX (pre-dosed NOX

samples) were below the detection limit (>0.1%) of the XPS. This indicates that, at least in the

initial surface state, the N- containing ions measured by ToFSIMS in this study were primarily

from the carbon surface. The inability to measure N using XPS is interesting. This may be

due to the TOFSIMS experiment only examining a single turnover of the carbon surface during

a single adsorption step. While in other studies 45,97,304 the carbon surface experiences several

turnovers and may have accumulated sufficient N on the surface to be detectable by XPS. An

interesting experiment would be to perform successive ToFSIMS, NO2 treatment, ToFSIMS

cycles followed by XPS to track the N enrichment on the carbon surface.

Additionally during the O2 exposure of these chars, Kapteijn observed that N accumulates with

burnoff 304. A similar observation was reported by Ashman et al. 45 for coal char oxidation in

2%O2/bal He at 873K with N retention as primarily pyridinic N. These reports indicate that the

N containing ions detected by the ToFSIMS in the final state are likely from nitrogen

incorporated into the carbon ring and are probably retained as pyridinic N or pyrollic N. In

order to better understand how the N is incorporated into the carbon structure an understanding

of the intermediate state is also needed.

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5.3.8.2.3 Intermediate surface composition, SC_NOX

The intermediate state holds the key to understanding how nitrogen is retained into the carbon

surface. The TP-ToFSIMS rate grouping data show that NO containing ion fragments are

being formed around 400°C with a shift to N-containing ions with increasing temperatures

along with a reduction of NO2 ions. This implies that the NO2 observed at the initial state is

also decomposing leaving behind C-NO type functional groups. These C-NO functional

groups eventually decompose/react to create CN type functional groups that may represent N

attached to the edges of or incorporated into the graphene structure.

IR based temperature studies report the presence of C-NO2, C-NO, C-NCO and anhydride type

structures around 400°C 31,78. Muckenhuber et al. 78 have interpreted DRIFTS bands at

1610cm-1 and 1230cm-1 as characteristic of N=O and C-O vibrations in C-ON=O at 400°C.

They also suggest that at 400°C, an acidic functional group is the transition state (C(=O)ONO).

From this group, NO is split and the C(=O)O functionality remains on the surface.

Jeguirim et al using reactor studies observed the rapid formation of NO 288. They postulate the

C(NO2) complex from their proposed mechanism (Equation 5-13 (a-c)) is probably unstable

and rapidly decomposes. They also suggest that a relationship exists between excess CO2

released at 300°C and additional NO2 adsorbed on the carbon surface may indicate that NO2

interacts with oxygen complexes formed during O2 pretreatment. This data supports the

observation of lower temperature loss of oxygen functionality from the PCA TP-ToFSIMS

data discussed earlier (O2 summary above). However, Jeguirim et al also report that

pretreating the carbon with O2 prior to NO2 exposure results in earlier desorption of the carbon

oxygen complexes 288. Recall that the SC_NOX sample was thermally annealed in He prior to

NO2/NO/O2 exposure and was further exposed to air during the transfer to the vacuum

chamber. However, the TP-ToFSIMS data suggest that oxygen need only be present on the

surface with NO2 to cause earlier desorption. The extent of earlier desorption cannot be

determined without additional analysis and experimentation.

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-C* +NO2 -C(NO2) {5-13a}

- -C(NO2) -C(O) + NO {5-13b}

- -C(O) + NO2 -C(ONO2) {5-13c}

Equation 5-13 (a-c): Reaction mechanism proposed by Jeguirim et al 288

5.3.8.3 Hypothetical surface and reaction pathway Here, a generalized reaction pathway and a hypothetical surface composition are proposed to

explain the observations from the TP-ToFSIMS data for the NOX dosed sample. In the initial

surface composition the carbon edges are likely populated with oxygen containing functional

groups such as lactones, carboxylic acids, and carboxylic anhydrides. In addition, the dosing

with the NO/NO2/O2 mixture forms weakly adsorbed NO2 and possibly NO on the carbon

surface. As the temperature is increased from the starting state to the intermediate state

(300°C-400°C)) the adsorbed NO2 has at least two possible reaction pathways: 1) weakly

adsorbed species are desorbed into the gas phase (100°C-200°C), and 2) there is rearrangement

on the carbon surface where C-NO type functional groups and C-O type functional groups are

formed (200°C-400°C). These C-O type groups either remain on the surface or are desorbed.

Further increasing the temperature to the final state (500°C-550°C) causes the C-NO

containing functional groups to be further reduced to CN- containing functional groups. At

this final stage the carbon structure consists of primarily pyridine-N, and possibly quaternary N

type structures. How the NOX adsorbed in the initial step gets to the final stage is uncertain.

The following reaction mechanisms are proposed for an NO2 –carbon reaction; although NO is

not discussed it is reported to play a role in N-ring formation 97.

In the initial state the NO2 has three possible configurations for bonding to the carbon surface

(Figure 5.3.29). These are by forming a chelated bond, non-chelated bond and/or bonding

through the N atom in the NO2 molecule. These structures are supported by DRIFTS data,

although the DRIFTS assignment of between 1485cm-1 and 1330 cm-1 for NO2 bonding to

carbon via the N atom is vague 78.

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NO O

+N

O

O

N+

OH

O

Chelated Non-chelated Bonding via N - atom

Figure 5.3.29: Examples of NO2 bonding to carbon

One possible reaction pathway is to consider the NO2 bonds to the carbon surface at an

armchair site (Figure 5.3.30). One of the oxygen atoms on the NO2 molecule could be

transferred to a neighboring carbon site. This oxygen would cleave the ring structure and

produce carbon monoxide. It is speculated that the dangling N – O structure would close the

ring by bonding via the nitrogen. This could occur at intermediate temperatures where the TP-

ToFSIMS results show the greatest value of NO type ion fragments. As temperature increases,

the remaining oxygen bonded to the nitrogen is removed by some unclear mechanism leaving

behind the nitrogen incorporated into the carbon ring structure. The nitrogen is incorporated

into carbon structure as either a five or six membered ring. However, assuming that the

DRIFTS assignment by Muckenhuber et al. 78 is correct, the peak representing NO2 bonded via

the nitrogen atom disappears after heating from room temperature to above 100°C. This

suggests that the weakly adsorbed NO2 species may be bonded via the nitrogen atom.

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C-

O+

N+

O

O-

N-

O-

N2-

O+

C-NH

N+O

-

ON

+

O

O

N

O-

O

OH

NH

OR

+

+

Figure 5.3.30: Reaction Scheme 2 - Generalized surface reaction mechanism with NO2 bonding via nitrogen atom to the carbon surface

A second possible mechanism is that in the initial state, NO2 is bonded to an armchair site via

the oxygen atom (Figure 5.3.31- Scheme 3). In this case, as temperature increases the oxygen

bonds to an adjacent carbon and is cleaved leaving a C-O bond and a C-NO bond. This is

consistent with the TP-ToFSIMS for NO type fragments and follows the reported IR data 31,78

for the presence of C-NO bonds. Further rearrangements allow for the evolution of CO, CO2

or H2O from the carbon surface and eventual N-incorporation within the carbon structure as a

five-member or six-member ring. Although additional evidence is needed, the weakly bonded

NO2 fragments at the initial state may be attributed to NO2 bonded via the nitrogen atom.

These proposed reaction pathways are consistent with the TP-ToFSIMS data and the literature

for each surface state. Another possible reaction pathway is the formation of a C-NO3 group

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on the surface that follows a similar pathway as reaction schemes 2 and 3. Although these TP-

ToFSIMS data provide supporting evidence for possible reaction pathways further

investigations are needed to clarify the intermediate states. Recommendations for future

studies are discussed below.

CH2

O+

N-NO

O

NO

O+

O+

N

C-

O+

NH C-

O++

+

Figure 5.3.31: Reaction Scheme 3 - Generalized surface reaction mechanism of NO2 bonding via the oxygen atom to the carbon surface

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5.4 Conclusions

1) Nitrogen content on the carbon surface increases during temperature ramping in a

vacuum environment after pre-dosing with NOX.

2) Two reaction pathways are proposed for NO2 bonding to an armchair site at low

temperatures and eventually forming pyridine –N or quaternary N in the carbon ring.

Intermediate surface structures contain NO type functional groups.

3) Large dataset of ions created during TP-ToFSIMS can be simplified to a few kinetic

sets by using principal component analysis (PCA), correlation inspection (C-I) with

integral rate method.

4) Sets using integral rate method are both kinetically and chemically distinct. It is

possible to narrow down TP-ToFSIMS sets to a few possible functional groups using

other reported analytical techniques for carbon.

5) Identified that there are four distinct sets for sample SC_NOX. Set II loses oxygen

quickly and reaches a stable surface concentration at approximately 300°C. Set IV is

initially created at low temperature and is then removed at a slower rate than Set II. Set

IV is identified to be possibly carboxylic acid, lactone, or carboxylic anhydride groups.

Set I are surface intermediates with a maximum concentration at 300°C. Set IV

represents the reduced structure and has two regions: 1) an initial increase in surface

concentration that mirrors Set I followed by 2) a linear increase in surface

concentration.

6) Initial surface composition changes of NOX functional groups (between 25°C and

200°C) occur within the area of relevance for low temperature soot filter regeneration.

7) Further investigation is needed to determine if the PCA, correlation- inspection method

used here can help group ion fragments for fingerprinting the parent functional groups

on the carbon.

8) Ion groupings produced using the integral method are different from thos e of the

differential method. The reason is unclear but it is suspected that time period of

analysis may play a role.

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5.5 Recommendations for future work

1) Collect ToFSIMS spectra of model compounds to help isolate and identify surface

species on the carbon surface.

2) Track N accumulation on the carbon surface with reaction turnover using successive

ToFSIMS and NO2 dosing cycles. As well, monitor the surface concentration of N

using XPS. This, of course, will not be possible until the N concentration reaches the

detection limit of the XPS.

3) Simultaneously monitor evolved gas phase components and surface concentrations

(ToFSIMS and/or XPS) to complete mass balance and deduce surface reaction

mechanism.

4) Use a carbon source that has fewer contaminants than the materials used here such as

pure graphite.

5) Continuously acquire ToFSIMS spectra to determine if the integral and differential

methods can create similar ion groupings.

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6 Conclusions and Recommendations

The objective of the thesis was to understand the limiting factors of carbon oxidation at

temperatures of 200°C. An initial literature survey was performed to test if selected catalytic

materials can oxidize carbon at a rate necessary to maintain a steady state carbon oxidation that

would be necessary for soot outputs of a modern diesel engine equipped with a diesel

particulate filter. The literature survey reveals that few catalysts can meet this criterion.

Selected carbon samples impregnated with alkali catalyst at loadings of K/C of 1/50 mol ratio

were evaluated in this thesis and found to not meet this criterion. The results of this thesis are

similar to literature catalysts with higher K/C ratios and with K on different supports.

Additionally, the selected catalysts were evaluated in a gas atmosphere with high NO2 content

(1%) that is higher than concentrations seen in engine exhaust; this was also found to not meet

the criteria. However, the data show that catalyzing the C-O2 reaction shows a greater

improvement in reactivity over catalyzing the C-NO2 reaction. Further studies are needed to

clarify if the catalyst is only creating NO2 for the C-NO2 reaction or is directly involved in

catalyzing the C-NO2 reaction in the reactant gas mixture (1% NO2, 1.5% NO, and 4.5% O2).

Additional screening experiments were performed to identify if thermal annealing of the

carbon would affect its reactivity through changes in its morphology. Extended thermal

anneals under inert atmospheres followed by oxidizing conditions indicate that the carbon

reactivity decreases. This study provides an upper limit to reactivity losses (maximum 40%)

that are contributed by thermal annealing in a non-reactive gas atmosphere. However, these

conditions are not experienced by diesel particulate filters and suggest that thermal annealing is

a minor contributor to carbon reactivity losses in DPF systems. This loss of reactivity could be

attributed to either morphology changes or to loss of reactive functional groups on the carbon

surface. To further explore this possibility the experimental technique of TP-ToFSIMS was

used to examine the surface groups on the carbon. Published literature on this technique as

applied to carbons was not found making this the first reported study to apply this technique to

determine the reactivity of carbons.

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TP-ToFSIMS showed that the carbon surface changes with temperature. The data clearly show

that carbon exposed to NOX has a higher N content on the surface as temperature increases in a

non-reactive gas atmosphere. Using the rate of change of the ion fragments and PCA to group

the ions with similar rate trends, the large quantity of ion fragments was separated and grouped

into four ion sets. Each of the sets corresponds to distinct chemical species with similar

kinetics. Set II loses oxygen quickly and reaches a stable surface concentration at approx.

300°C. Set IV is initially created at low temperature and is then removed at slower rate than

Set II. Set IV is identified as possibly representing lactone type surface groups. Set I ions are

surface intermediates with a maximum concentration at 300°C. Set IV represents the reduced

carbon surface and has two regions: an initial increase in surface concentration that mirrors Set

I followed by a linear increase in surface concentration. Identification of the source of the ion

fragments was attempted but was difficult due to the limited information on ion fragmentation

patterns from carbon surfaces. Further work is needed identifying ion fragments produced

from the carbon surface during SIMS. One method is SIMS studies of model compounds to

create ion fragments that can be related to the carbon surface. However, even without this

detailed information it was possible to deduce a reaction mechanism for the interaction of NO2

with the carbon surface.

Using this TP-ToFSIMS data, two reaction pathways are proposed for NO2 bonding to an

armchair carbon site at low temperatures that rearranges and eventually forms pyridine –N or

quaternary N in the carbon ring. Although, the intermediate steps for incorporation of N into

the carbon ring are not proven here there are three clear observations: 1) At low temperatures

NO2- ions are present and disappear at temperatures greater than 200°C. 2) The TP-ToFSIMS

clearly identified NO type functional groups as surface structures at intermediate temperatures

around 300°C to 400°C. 3) N is clearly accumulating and forming a stable structure on the

carbon surface and is incorporated into the carbon ring.

A few questions arise from this observation of N incorporation into the carbon ring. Does the

increasing N content on the carbon surface affect the reactivity of the carbon? Furthermore

only select fragments were examined in the TP-ToFSIMS data. The other inorganic ion

fragments may affect the rate of the carbon surface and may provide further insight into the

carbons’ reactivity. In summary, no rate processes meet the steady state gasification criteria

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during reactivity studies or surface functional group studies and the reason for this is not

understood. However this study clearly shows that the technique of TP-ToFSIMS can provide

pertinent reactivity data and chemical surface information of the reactions of oxidants with the

carbon surface and provide clues towards reaction mechanisms.

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298. Gong B; Pigram PJ; Lamb RN Identification of inorganic nitrogen in an Australian bituminous coal using X-ray photoelectron spectroscopy (XPS) and time-of-flight secondary ion mass spectrometry (TOFSIMS). International Journal of Coal Geology 1997, 34, 53-68.

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300. Peled E; Golodnitsky UA; Yufit V Effect of carbon substrate on SEI composition and morphology. Electrochemica Acta 2004, 50, 391-395.

301. Mahoney CM; Gillen G; Fahey AJ Characterization of gunpowder samples using time-of-flight secondary ion mass spectrometry (TOF-SIMS). Forensic Science International 2006, 158, 39-51.

302. Solumko V; Delcorte A; Garrison BJ; Bertrand P Sputtering of a polycyclic hydrocarbon molecule: TOF-SIMS experiments and molecular dynamic simulations. Applied Surface Science 2004, 231-232, 48-53.

303. Vickerman JC ToF-SIMS- An Overview. In ToF-SIMS: Surface Analysis by Mass Spectroscopy, Vickerman JC, Briggs D, Eds.; M Publications and SurfaceSpectra Limited: 2001.

304. Kapteijn F; Moulijn JA; Matzner S; Boehm HP The development of nitrogen functionality in model chars during gasification in CO2 and O2. Carbon 1999, 37, 1143-1150.

305. Wagner MS; Graham DJ; Ratner BD; Castner DG Maximizing information obtained from secondary ion mass spectra of organic thin films using multivariate analysis. Surface Science 2004, 78, 570.

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309. Cheng F; Gamble LJ; Grainger DW; Castner DG X-ray photoelectron Spectroscopy, Time of Flight Secondary Ion Mass Spectrometry, and Principal Component Analysis of the Hydrolysis, Regeneration, and Reactivity of N- Hydroxysuccinimide- Containing Organic Films. Analytical Chemistry 2007, 79, 8781-8788.

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311. Graham DJ; Wagner MS; Castner DG Information from complexity: Challenges of TOF-SIMS data interpretation. Applied Surface Science 2006, 252, 6860.

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323. Li XK; Liu L; Li Zh H; Wu D; Shen Sh.D The characterization of ultrafine carbon powders by SAXS and Raman spectra. Carbon 2000, 39, 623.

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332. Dresselhaus MS; Dresselhaus G Carbon. In Light Scattering in Solids, Guntherodt G, Ed.; Springer: Berlin, 1982; pp 3-58.

333. Fityk curve fitting free software V5.0, 2005, http://www.unipress.waw.pl/fityk, last accessed July 10, 2008

334. Amin A; Philip CA; Girgis BS Influence of reacting atmosphere on isothermal decomposition of ammonium metavanadate. Collection of Czechoslovak Chemical Communications 1994, 59, 1086-1095.

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8 Appendix Information The appendix contains the following:

8.1) Appendix A contains the preparation method of the catalyst impregnated carbons

and screening experiments using image analysis.

8.2) Appendix B contains scanning electron microscopy images of the sucrose char and

NIST soot.

8.3) Appendix C contains exploratory experiments using Raman spectroscopy

8.4) Appendix D contains principal component analysis plots of negative and positive

ions for NIST, CAT, SC_AIR and SC_NOX samples.

8.5) Appendix E contains the certification data of the NIST soot and the specification

sheet of the sucrose precursor used to make the sucrose char.

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8.1 Appendix A: Soot impregnation technique and procedure The following describes the preparation of carbons impregnated with catalyst used in the

reactivity studies. A variety of element precursors and wetting agents were used to disperse

the catalytic materials over the carbon surface. In addition, an experiment is described that

was used to quickly evaluate many catalysts at once under the same operation conditions.

Catalyst Preparation

NIST SRM 2975 (NIST) soot samples used for oxidation trials were wetted using a 90%-

ethanol--10%-water solution with dissolved catalyst precursors, with the exception of some

trials. Prior to impregnation with catalyst, it was determined that NIST soot samples favorably

absorbed solutions up to 2.1 times their own mass. Accordingly, solutions of KOH, FeNO2,

NH4VO3 and CeNO3 catalyst solutions were produced such that the impregnation solutions

would contain ratios of catalyst to carbon atoms of 1:50 up to 1:1000.

Initially each catalyst was dissolved in water to a predetermined concentration. This solution

was subsequently mixed with the correct amount of ethanol to produce solutions that could be

used to impregnate carbon to the predetermined catalyst-to-carbon ratio. The solution was

stored in a polypropylene bottle for later application to impregnate NIST soot samples.

Carbon samples were wetted using a micropipette filled with the prepared catalyst solutions.

Once the soot samples were wetted, they were dried in an oven for two hours at 65°C, ramped

at 1°C/min from room temperature until the final temperature was reached.

Table 8-1 below summarizes the samples that were prepared. It describes the solution that was

made and how much solution was added to each soot sample.

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Table 8-1: Catalyst impregnated carbon samples prepared for image analysis experiments

Sample Code Ion Ratio Solution Preparation μL Solution added to mg Amount Soot

T1 Na+ 1:50 26.0g NaOH pellets added to water to make 100ml solution; 5.55ml of resulting solution mixed with 50ml Ethanol

90.6μL to 34.9mg

T2 K+ 1:50 34.47g KOH pellets added to 100 ml water; 5.55ml of resulting solution mixed with 50ml Ethanol

106μL to 40.8mg

T3 V+ 1:125 3.75g of NH4VO3 added to 100mL of water in presence of 5.0mL 18.0M HCl

50.8μL applied three times to 24.2mg

T4 Fe3+ 1:150 4.7938g Fe(CO3)3 added to 100 ml water; 5.55ml of resulting solution mixed with 50ml Ethanol

8.34μL to 32.1mg

T5 Ce3+ 1:150 Added 221μL of Ce(NO3)3 solution to 779μL of water and mixed with 9.0mL of Ethanol

D2 K+ 1:230 1.8269g K2CO3 added to 20 ml water; 1 ml of resulting solution mixed with 9ml Ethanol

154.8μL to 61.9mg

Eth. -- -- Ethanol solution; no catalyst -- Diol. -- -- 1,4-Butandiol used in a mixture with

ethanol to wet soot --

N4 Std. -- -- Standard Soot. --

Image Analysis Experiment

The initial experiment (Experiment 1) was a broad test to determine oxidation temperatures of

the different soot-catalysts samples. A bench test was completed where less than 1mg of soot

from several different dried catalyst samples was taken and spread on a quartz plate over an

area less than one square centimeter. The procedure resulted in a relatively small area on the

quartz plate that was covered with a thin film of the soot layer. This was repeated several

times until several different soot-catalyst samples were on the plate.

Photographs of the quartz plate were taken using the following procedure. The sample loaded

quartz plate was placed on a white sheet of paper that was marked to locate the quartz plate for

later images. An enclosure was placed over the quartz plate and located based on markings on

the white background paper. The enclosure consists of two holes on the side of the enclosure

and a hole on top to locate the camera. The two holes on the side of the enclosure were used to

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provide light from two light sources. The above equipment was used to minimize the light

contrast and allow the photos to be taken in a similar manner.

A photograph was taken of the quartz plate before being exposed to temperature in the oven.

The quartz plate was placed in the oven and heated to the required temperature and held for a

constant time and then cooled. The quartz plate was transferred to the photo equipment and a

photo taken. The procedure was repeated until all temperatures were evaluated.

Figure 8.1.1: Sample location for Image Experiment 1

The results of the first screening experiment (Experiment 1) to 425ºC were quite significant

(sample locations in Figure 8.1.1; images after temperature exposure Figure 8.1.3). Soot

samples that contained sodium, potassium and vanadium were each oxidized over 90% in the

regions of interest (see circled areas in Figure 8.1.1). In contrast, the control samples of soot

without metal catalyst (i.e. N4 Standard and N4 + Ethanol) showed no visible sign of

oxidation. Thus, observed oxidation was a result of some catalytic activity. The remaining

samples, including the [1:150] Ce+ showed some signs of oxidation, but it was not significant

when compared to sodium, potassium or vanadium, less than 10% (approximately) compared

to the other catalysts studied.

T1 T2 T3

T4 T5 N4

D2 Eth Diol

Quartz plate

Soot-Catalyst Samples

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In the second ramp, the temperature was raised up to 450ºC. Sodium, potassium and vanadium

showed continued signs of oxidation. The N4 Std. soot, which did not oxidize, was thus used

as a benchmark for comparison between soot that had oxidized and had not oxidized in the

previous run. Iron impregnated soot showed some further signs of oxidation while the cerium

impregnated soot began to show signs of initiation of oxidation. However it is difficult to say

conclusively that both these samples did in fact oxidize. The grounds for this reasoning are

that in the 425ºC and 450ºC ramps, there was a noticeable contrast between the focus and

darkness of the overall picture, especially between the N4 Std. samples. Since it is probable

that the N4 Std. soot did oxidize between 425ºC and 450ºC, then the contrast between these

two samples is likely a result of lighting and focus. On similar grounds, the difference between

the iron and the cerium, samples may be attributed to lighting and focus.

The table below summarizes the results of the analysis of the images that were taken of the

quartz plates. The results were used to select the catalysts for the reactor oxidation

experiments found in Chapter 4.

Table 8-2: Estimate of oxidation for Experiment 1 Image Analysis (Peak Temperature 425 ºC)

Sample Code Ion Ratio Rough Estimate of Oxidation

T1 Na+ 1:50 >90% T2 K+ 1:50 >90% T3 V+ 1:125 >90% T4 Fe3+ 1:150 <10% T5 Ce3+ 1:150 <10% D2 <5%

Eth. -- -- None Diol. -- -- None

N4 Std. -- -- None A second image reactivity experiment (Experiment 2) was performed using a similar procedure

as Experiment 1. For this experiment, only sodium, potassium, and vanadium were used, since

it was these three samples that showed the greatest sign of oxidation during the first

experiment.

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The first step was to 350ºC, but unlike the previous experiment it was held at that temperature

for 30 min and not one hour (Table 8-3). There was evidence to show that all three samples

oxidized. Of the three samples, the potassium - impregnated sample showed the greatest

oxidation. The sodium and vanadium also showed signs that oxidation had taken place (See

Figure 8.1.2 below for photo images of Experiment 2).

Table 8-3: Estimate of oxidation for Experiment 2 Image Analysis (Peak Temperature 350 ºC)

Sample Code Ion Ratio Rough Estimate of Oxidation

T1 Na+ 1:50 >40% T2 K+ 1:50 >70% T3 V+ 1:125 >20%

N4 Std. -- -- None

The experiment was repeated with a peak temperature of 325ºC. Oxidation of all three soot

samples had significantly decreased. Despite this, the soot sample with the potassium catalyst

continued to show signs of oxidation. As the images show, potassium was the most oxidized

sample. Sodium and vanadium impregnated soot samples also showed some signs of

oxidation, though not to the same extent as potassium samples.

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Figure 8.1.2: Photo Images of Experiment 2

At Room Temperature At 350oC

At 325oC

T1 (Na) T2 (K) T3 (V)

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Figure 8.1.3: Photo Images of Experiment 1

At Room Temperature After First Ramp at 425oC

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After Second Ramp at 450oC

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Conclusions and Analysis

Experiments showed that of the several different catalysts used to oxidize soot, potassium

acted as the best catalyst. It appears that potassium loadings at concentrations higher

than (Catalyst/Carbon mole ratio) 1:50 will likely result in lower oxidation temperatures

(from comparison of samples T2 and D2). It may also be worthwhile to determine

whether OH- had played any role in oxidation of the carbon. Although experiments run

to compare, methanol, ethanol and butanediol, showed no influence of OH- groups, none

of these solutions had free OH-. Both the sodium and potassium solutions were prepared

using hydroxide solutions that contained a free OH- ion.

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8.2 Appendix B: SEM photos Scanning electron microscopy photos show the morphology of the carbon tested in this study:

1) Sucrose char has a smooth surface that has low surface area as confirmed by BET (12m2/g) (Figure 8.2.1).

2) CAT diesel soot consists of small particles of about 1 um diameter particles

suggest high surface area (Figure 8.2.2)

3) NIST diesel soot consists of larger particles than the CAT diesel soot with particles ranging in size from 2um to 25 um (Figure 8.2.3)

Figure 8.2.1: Sucrose char

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Figure 8.2.2: CAT diesel soot

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Figure 8.2.3: NIST diesel soot

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8.3 Appendix C: Raman experimental procedure and results

Raman spectroscopy was used to determine qualitatively the presence of edge sites. A

description of the technique, experimental procedure and results are found here. The Raman

experiments were abandoned early in this thesis due to the observation of laser exposure on

this instrument changing the D/G peak ratio. It was concluded that local heating was being

caused by the laser exposure and light adsorption properties of the black carbon. An

unsuccessful attempt was made to find a spinning sample stage to minimize these effects.

Described below are the investigations performed before abandoning this experiment.

8.3.1.1 Objective Use Raman Spectroscopy to identify edge groups on carbon structures. It is expected that the

results will show a relationship between reactive edge carbons to less reactive basal plane

carbon atoms.

8.3.1.2 Background

One of the key parameters of this study is obtaining the number of available edge sites on the

carbon. Understanding the relationship of active edge sites on the carbon structure to bulk

carbons is key to determining the maximum edge site reactivity. A technique that is popular in

investigating carbon structures and reported to give information on carbon disorder is Raman

spectroscopy 124,125,320-326. A description of the Raman spectroscopy technique can be found in

a recent review on the applications of Raman 327. The application of Raman to graphite and

amorphous carbon is found in review articles by Ferrari 126 and Pimenta et al. 127. The structure

of diesel soot has also been examined 128,328, and more recently its reactivity 329.

The pioneering work of Tuinstra and Koenig 124 showed that variations in Raman spectra were

observed in different carbon materials. In this initial work, they observed a shift of the

intensities between the 1350 cm-1 and 1600 cm-1 wave number peaks. These wave numbers

have been assigned as the G peak and the D peak respectively. These peaks are interpreted to

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indicate the amount of graphitic characteristics (G peak ) or bulk carbon and the D peak as the

disordered carbon peak 123,125,330,331. In carbons, the disordered peak has been suggested to

indicate the presence of edge carbons 125. G peak at 1585 cm-1 is the fundamental mode of the

graphite crystal. The D’ peak at 1620cm-1 is suggested to be sensitive to the composition of

the material in contact with the surface layers of the graphite (modifies their electronic

environment) 330,332. The 1360 cm-1 (D band – ‘disorder’ band) indicates edge vibrations.

Compagnini et al 125 provide evidence of the correlation of this feature with the graphite edge.

The ratio of intensity of D/G peak gives an indication of the amount of disorder in the carbon

structure. A direct relationship between the amounts of carbon edge sites to the intensity of the

D peak has not been reported. Although Compagnini looked at creating edge sites by using an

Ar ion gun, they found that the intensity ratio of D/G increases with ion influence 125. A survey

of the literature did not reveal a quantitative relationship between the peak areas or peak ratios

to the number of actual edge carbons.

8.3.1.3 Analytical Equipment

University of Toronto’s Institute of Optical Science, laser spectroscopy department in-house

designed Micro-Raman spectrometer using a con-focal microscope for imaging and beam

focusing with an argon laser operating at 514 nm was used for analysis. Laser power was

adjustable; two settings, 200mA and 150mA settings were used. The lower setting was used

because it caused less destruction of the carbon. The spectrometer was equipped with filters to

help diffuse the laser power and with variable pinhole and slit widths to help improve data

collection. A video camera is installed to help focus the beam.

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8.3.1.4 Experimental

1) Examine sucrose chars and NIST diesel particulate matter using Raman Microscopy

2) Adjust power, filters, pinhole and slit size to optimize data collection and prevent

damage to the sample.

3) Select appropriate magnification lenses and filters.

4) Place sample on slide and place under microscope.

5) Adjust stage as close as possible to microscope.

6) Switch lens system to camera. Turn on camera and light.

7) Focus area of interest by backing the stage away from the lense (coarse adjustment)

8) Switch lens system to detector. Turn off camera and light.

9) Activate the scan mode and adjust to maximum intensity using fine adjustment knob

10) Select appropriate number of scans and scan delay time

11) Run scan accumulation mode.

12) Switch lenses system to camera. Turn on camera and light.

13) Check for damage on the material. Material damage is observed by discoloration of

material.

8.3.1.5 Instrument setup

A series of initial setup experiments were performed to qualify the instrument by examining

the sample to find the D and G carbon peaks as found in the literature. Secondly, experiments

were performed to determine if the laser caused damage to the carbon structure. Through the

use of optical filters, changing the laser power and sample exposure time, the laser was

optimized to minimize damage to the carbon. Sample damage was obvious through the

increasing D peak intensity with exposure time and by the appearance of a dark spot on the

sample when viewed with the video camera and the laser turned off.

Analysis of spectral data was performed using the peak fitting program (Fityk). Fityk is a

shareware program 333. The peaks were corrected by fitting a baseline curve. The baseline was

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subtracted from the original data and then the baseline corrected curve was fitted with

Gaussian or Lorentzian type peaks. In all cases the data could be fitted with two or three

peaks. The program is able to integrate the area of the individual fitted peaks and provide peak

heights and peak area. A graph of peak height versus peak area for all samples shows that

there is no clear correlation between these two parameters. In this analysis the peak areas are

used. Table 8-4 contains a list of the samples investigated using the Raman technique.

Table 8-4: Sample designation of Raman Samples. # indicates file of Raman spectra and that the measurement was repeated on a different part of the sample.

Sample Name

SCV3a_# SCV5_# SCV6_# SCVM_# SC# DS DS450

Description Ammonium metavanadate impregnated sucrose char (Dried at 125°C in air)

SCV3a exposed above 200°C (473K)

SCV3a exposed above 260°C (533K)

Mechanical mixture of V2O5 and sucrose char

Sucrose char exposed to 400°C in air (SC3, SC2, same sample different area)

NIST diesel soot

NIST diesel soot exposed to 450°C

Ammonium metavanadate is not the active form of V2O5 and samples SCV5 and SCV6 are

thermally treated in air to convert the ammonium metavanadate into reaction intermediates in

the reaction formation pathway of V2O5. V2O5 is not formed until temperatures of 400°C are

reached. During the heat up of the sample the intermediate vanadium compounds are likely

changing the carbon characteristics and likely converting the carbon into CO or CO2.

8.3.1.6 Results

One of the parts of this project is to characterize the active sites of the carbon. Raman

spectroscopy has been used to compare the disordered carbon peak to the graphite peak. The

disordered peak has been proposed to indicate edge site characteristics.

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Raman studies on vanadium impregnated sucrose char, non-catalyzed sucrose char and diesel

soot (Table 8-4) have been performed. The disordered/graphite peak ratios (D (1350cm-1)/G

(1600 cm-1) were calculated by fitting the collected data with Gaussian peak shapes using a

shareware program 333. Screenshots of the fitted data are shown in Figure 8.3.1 and Figure

8.3.2.

Figure 8.3.1: Raman spectra of SCV3a x-axis: wavenumber, y axis: intensity, dots= data, solid line fitted peaks

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Figure 8.3.2: Raman Spectra of SCVM_4 x-axis: wavenumber, y axis: intensity, dots= data, solid line fitted peaks

A comparison of the diesel soot and the sucrose char indicates that there are some differences

between materials (Figure 8.3.3). These differences may later explain any reactivity

differences between the model sucrose char and the diesel soot. The most observable

difference is the lower Raman intensity of diesel soot compared to the char. This difference

could be attributed to higher graphitic and crystalline character of the char or more interference

in diesel soot preventing the photons from reaching the detector

The effect of the soluble organic fraction (SOF) on the disordered carbons was considered as a

possible cause of the low intensity of the NIST soot. A sample of the NIST soot was heated to

450°C in air to oxidize the hydrocarbon (SOF). It is suspected that oxidizing the hydrocarbons

in air may affect the carbon sites by possibly creating disorders or exposing disorders. Results

show (Figure 8.3.3) that the adsorbed hydrocarbon does not affect the D/G ratio. A repeat

measurement of the DS 450 sample shows that the D/G ratio measurement varies by more than

25%.

Vanadium impregnated sucrose char was used to test if Raman would be able to measure the

catalysts occupying edge sites of carbon. An initial sample was made by impregnating sucrose

char (SC) with ammonium metavanadate (SCV3a). Ammonium metavanadate forms three

decomposition products: ammonium tetravanadate at 453K, ammonium hexavanadate at 503K

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and V2O5 at 623K 334. Samples of SCV3a were exposed to 473K (SCV5) and 533K (SCV6).

The further exposure to temperature of V2O5 was not performed. In addition, a mechanical

mixture of V2O5 and sucrose char was made. The Raman spectra show features of the V2O5

below 1000cm-1 (Figure 8.3.3). This was confirmed by performing a baseline on the V2O5.

The data from the vanadium-impregnated samples is not clear. Ammonium metavanadate

appears to improve the D/G ratio when compared to non-catalyzed sucrose char. This

exposure to higher temperatures either causes the destruction of the edge sites or changes their

Raman feature. A baseline of ammonium metavanadate exposed at the different temperatures

was not performed and thus the effects on Raman features from ammonium metavanadate

cannot be discounted. Further Raman studies are needed to clarify this.

In addition, Raman spectra have not been taken of the reacted carbons. Samples of partial

reacted carbons need to be analyzed by Raman to determine if the D/G ratio has changed due

to reaction or by wetting of the catalysts; these changes in the Raman spectra may be correlated

to reaction data.

Correlation of the Raman data to oxygen chemisorption data is proposed as a means to quantify

the Raman data. It may be possible to perform these experiments similarly to those used to

determine the amount of loosely held carbon oxides. Exposure of the sample to He and

increasing the temperature of the reactor to high temperatures to remove the weakly held

oxygen groups and then cooled. An oxygen pulse can be passed over the sample to reoxidize

the sites and then reheated. This may require more sensitive analytical equipment. Further

thought is need to on how to perform this experiment.

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0

0.5

1

1.5

2

2.5

3

3.5

4

scv3

a_3

scv3

a_2

scv3

a_1

scv5

_1

scv6

_2

scvm

_4 sc3

SC2

Ds450

_2

DS450_

1DS-1

D/G

Rat

io

0

5000

10000

15000

20000

25000

30000

35000

40000

Are

a

D/G Fityk D Fityk G

Figure 8.3.3: D/G peak ratios of Raman spectra

8.3.1.7 Conclusion

It was observed that exposure of the carbon to the laser gradually created an increase in the

intensity of the D and G peaks similar to others127. This is suspected to be a result of localized

heating of the carbon surface and reaction with oxygen in the air. Changes in peak heights

were observed by changing the laser power and length of time exposure of the carbon surface

to the laser. Attempts to reduce this effect were not successful. A possible solution would be

to perform the experiment under non-reactive gas conditions (i.e., under He or AR only

conditions). In addition sample spinning is necessary to prevent self-heating as discovered by

others more than 30 years ago.

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8.4 Appendix D: PCA plots

Figure 8.4.1: PCA Loading Plots for Sample CAT-0 negative ions: Loading plot (a) and Biplot (b) of PC1 versus PC2 (▼- scores, ♦ - loadings), Cumulative variance captured by each PC (c). Loading plots indicate identified groupings within the TOFSIMS data.

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Figure 8.4.2: PCA Loading Plots for Sample NIST-ANN negative ions: Loading plot (a) and Biplot (b) of PC1 versus PC2 (▼- scores, ♦ - loadings), Cumulative variance captured by each PC (c). Loading plots indicate identified groupings within the TOFSIMS data.

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Figure 8.4.3: PCA Loading Plots for Sample SC_NOX negative ions: Loading plot (a) and Biplot (b) of PC1 versus PC2 (▼- scores, ♦ - loadings), Cumulative variance captured by each PC (c). Loading plots indicate identified groupings within the TOFSIMS data.

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Figure 8.4.4: PCA Loading Plots for Sample SC_AIR negative ions: Loading plot (a) and Biplot (b) of PC1 versus PC2 (▼- scores, ♦ - loadings), Cumulative variance captured by each PC (c). Loading plots indicates identified groupings within the TOFSIMS data.

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Figure 8.4.5: PCA Loading Plots for Sample NIST-0 negative ions: Loading plot (a) and Biplot (b) of PC1 versus PC2 (▼- scores, ♦ - loadings), Cumulative variance captured by each PC (c). Loading plots indicates identified groupings within the TOFSIMS data.

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Figure 8.4.6: PCA Loading Plots for Sample NIST-0 positive ions: Loading plot (a) and Biplot (b) of PC1 versus PC2 (▼- scores, ♦ - loadings), Cumulative variance captured by each PC (c). Loading plots indicate identified groupings within the TOFSIMS data.

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Figure 8.4.7: PCA Loading Plots for Sample CAT-0 positive ions: Loading plot (a) and Biplot (b) of PC1 versus PC2 (▼- scores, ♦ - loadings), Cumulative variance captured by each PC (c). Loading plots indicate identified groupings within the TOFSIMS data.

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Figure 8.4.8: PCA Loading Plots for Sample NIST_ANN positive ions: Loading plot (a) and Biplot (b) of PC1 versus PC2 (▼- scores, ♦ - loadings), Cumulative variance captured by each PC (c). Loading plots indicate identified groupings within the TOFSIMS data.

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Figure 8.4.9: PCA Loading Plots for Sample SC_NOX positive ions: Loading plot (a) and Biplot (b) of PC1 versus PC2 (▼- scores, ♦ - loadings), Cumulative variance captured by each PC (c). Loading plots indicate identified groupings within the TOFSIMS data.

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Figure 8.4.10: PCA Loading Plots for Sample SC_AIR positive ions: Loading plot (a) and Biplot (b) of PC1 versus PC2 (▼- scores, ♦ - loadings), Cumulative variance captured by each PC (c). Loading plots indicate identified groupings within the TOFSIMS data.

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8.5 Appendix E: Certification and specification sheets

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