uvvis-spectroscopy p bambang
TRANSCRIPT
-
8/6/2019 UVVIS-Spectroscopy p Bambang
1/35
SPECTROSCOPY
Light interacting with matter as an
analytical tool
-
8/6/2019 UVVIS-Spectroscopy p Bambang
2/35
X-ray:
core electronexcitation
UV:
valanceelectronic
excitation
IR:
molecularvibrations
Radio waves:
Nuclear spin states(in a magnetic field)
Electronic Excitation by UV/Vis Spectroscopy :
-
8/6/2019 UVVIS-Spectroscopy p Bambang
3/35
Spectroscopic Techniques and
Chemistry they Probe
UV-vis UV-vis region bonding electrons
Atomic Absorption UV-vis region atomic transitions (val. e-)
FT-IR IR/Microwave vibrations, rotations
Raman IR/UV vibrations
FT-NMR Radio waves nuclear spin states
X-Ray Spectroscopy X-rays inner electrons, elementalX-ray Crystallography X-rays 3-D structure
-
8/6/2019 UVVIS-Spectroscopy p Bambang
4/35
Spectroscopic Techniques and Common Uses
UV-vis UV-vis region Quantitativeanalysis/Beers Law
Atomic Absorption UV-vis region Quantitative analysisBeers Law
FT-IR IR/Microwave Functional Group Analysis
Raman IR/UV Functional GroupAnalysis/quant
FT-NMR Radio waves Structure determination
X-Ray Spectroscopy X-rays Elemental Analysis
X-ray Crystallography X-rays 3-D structure Anaylysis
-
8/6/2019 UVVIS-Spectroscopy p Bambang
5/35
Different Spectroscopies
UV-vis electronic states of valence e/d-orbital transitions for solvated transitionmetals
Fluorescence emission of UV/vis by certainmolecules
FT-IR vibrational transitions of molecules
FT-NMR nuclear spin transitions X-Ray Spectroscopy electronic transitions
of core electrons
-
8/6/2019 UVVIS-Spectroscopy p Bambang
6/35
Quantitative Spectroscopy
Beers Law
Al1 = el1bc
e is molar absorptivity (unique for a
given compound at l1)
b is path lengthc concentration
-
8/6/2019 UVVIS-Spectroscopy p Bambang
7/35
Beers Law
A = -logT = log(P0/P) = ebc
T = Psolution /Psolvent = P/P0
Works for monochromatic light
Compound x has a unique e at different wavelengths
cuvette
source slit
detector
-
8/6/2019 UVVIS-Spectroscopy p Bambang
8/35
Characteristics of
Beers Law Plots One wavelength
Good plots have a range of
absorbances from 0.010 to 1.000
Absorbances over 1.000 are not that
valid and should be avoided
2 orders of magnitude
-
8/6/2019 UVVIS-Spectroscopy p Bambang
9/35
Standard Practice
Prepare standards of knownconcentration
Measure absorbance at max Plot A vs. concentration
Obtain slope
Use slope (and intercept) to determinethe concentration of the analyte in theunknown
-
8/6/2019 UVVIS-Spectroscopy p Bambang
10/35
Typical Beers Law Plot
y = 0.02x
0
0.2
0.4
0.6
0.8
1
1.2
0.0 20.0 40.0 60.0
concentration (uM)
A
-
8/6/2019 UVVIS-Spectroscopy p Bambang
11/35
UV-Vis Spectroscopy
UV- organic molecules
Outer electron bonding transitions
conjugation
Visible metal/ligands in solution
d-orbital transitions
Instrumentation
-
8/6/2019 UVVIS-Spectroscopy p Bambang
12/35
Characteristics of UV-Vis spectra of
Organic Molecules Absorb mostly in UV unless highly
conjugated
Spectra are broad, usually to broad forqualitative identification purposes
Excellent for quantitative Beers Law-
type analyses The most common detector for anHPLC
-
8/6/2019 UVVIS-Spectroscopy p Bambang
13/35
Molecules have quantized energy levels:
ex. electronic energy levels.
energy
hv
energy
} = hvQ: Where do these quantized energy levels come from?
A: The electronic configurations associated with bonding.
Each electronic energy level(configuration) has
associated with it the many
vibrational energy levels we
examined with IR.
-
8/6/2019 UVVIS-Spectroscopy p Bambang
14/35
Broad spectra
Overlapping vibrational and rotational
peaks Solvent effects
-
8/6/2019 UVVIS-Spectroscopy p Bambang
15/35
Molecular Orbital Theory
Fig 18-10
-
8/6/2019 UVVIS-Spectroscopy p Bambang
16/35
2s 2s
2p 2pn
-
8/6/2019 UVVIS-Spectroscopy p Bambang
17/35
C C
hv
C C
H
HH H
HH
max
= 135 nm (a high energy transition)
Absorptions having max < 200 nm are difficult to observe because
everything (including quartz glass and air) absorbs in this spectral
region.
Ethane
-
8/6/2019 UVVIS-Spectroscopy p Bambang
18/35
C C
hv
Example: ethylene absorbs at longer wavelengths: max = 165 nm = 10,000
=hv
=hc/
-
8/6/2019 UVVIS-Spectroscopy p Bambang
19/35
hv
n
n
C O
n
The n to pi* transition is at even lower wavelengths but is notas strong as pi to pi* transitions. It is said to be forbidden.
Example:
Acetone: n max = 188 nm ; = 1860
n max = 279 nm ; = 15
-
8/6/2019 UVVIS-Spectroscopy p Bambang
20/35
C C
C C
C O
C O
H
> 135 nm
> 165 nm
n > 183 nm weak
> 150 nm
n > 188 nmn > 279 nm weak
A
180 nm
279 nm
C O
-
8/6/2019 UVVIS-Spectroscopy p Bambang
21/35
C C
HOMO
LUMO
Conjugated systems:
Preferred transition is between Highest Occupied Molecular Orbital(HOMO) and Lowest Unoccupied Molecular Orbital (LUMO).
Note: Additional conjugation (double bonds) lowers the HOMO-
LUMO energy gap:
Example:
1,3 butadiene: max = 217 nm ; = 21,000
1,3,5-hexatriene max = 258 nm ; = 35,000
-
8/6/2019 UVVIS-Spectroscopy p Bambang
22/35
O
O
O
Similar structures have similar UV spectra:
max = 238, 305 nm max = 240, 311 nm max = 173, 192 nm
-
8/6/2019 UVVIS-Spectroscopy p Bambang
23/35
Lycopene:
max = 114 + 5(8) + 11*(48.0-1.7*11) = 476 nm
max (Actual) = 474.
-
8/6/2019 UVVIS-Spectroscopy p Bambang
24/35
Metal ion transitions
Degenerate
D-orbitals
of naked Co
D-orbitalsof hydrated Co2+
Octahedral Configuration
E
-
8/6/2019 UVVIS-Spectroscopy p Bambang
25/35
Co2+
H2O
H2O
H2O
H2O
H2O
H2
O
Octahedral Geometry
-
8/6/2019 UVVIS-Spectroscopy p Bambang
26/35
Instrumentation
Fixed wavelength instruments
Scanning instruments
Diode Array Instruments
-
8/6/2019 UVVIS-Spectroscopy p Bambang
27/35
Fixed Wavelength Instrument
LED serve as source
Pseudo-monochromatic light source
No monochrometer necessary/ wavelength selection occurs
by turning on the appropriate LED 4 LEDs to choose from
photodyode
sample
beam of light
LEDs
-
8/6/2019 UVVIS-Spectroscopy p Bambang
28/35
Scanning Instrument
cuvette
Tungsten
Filament (vis)
slit
Photomultiplier
tube
monochromator
Deuterium lamp
Filament (UV)
slit
Scanning Instrument
-
8/6/2019 UVVIS-Spectroscopy p Bambang
29/35
sources
Tungten lamp (350-2500 nm)
Deuterium (200-400 nm)
Xenon Arc lamps (200-1000 nm)
-
8/6/2019 UVVIS-Spectroscopy p Bambang
30/35
Monochromator
Braggs law, nl = d(sin i + sin r)
Angular dispersion, dr/d = n / d(cos r)
Resolution, R = / = nN,
resolution is extended by concave
mirrors to refocus the divergent beam at
the exit slit
-
8/6/2019 UVVIS-Spectroscopy p Bambang
31/35
Sample holder
Visible; can be plastic or glass
UV; you must use quartz
-
8/6/2019 UVVIS-Spectroscopy p Bambang
32/35
Single beam vs. double beam
Source flicker
-
8/6/2019 UVVIS-Spectroscopy p Bambang
33/35
Diode array Instrument
cuvette
Tungsten
Filament (vis)
slit
Diode array detector
328 individual detectors
monochromator
Deuterium lampFilament (UV)
slit
mirror
-
8/6/2019 UVVIS-Spectroscopy p Bambang
34/35
Advantages/disadvantages
Scanning instrument
High spectral resolution (63000), /
Long data acquisition time (several minutes)
Low throughput
Diode array
Fast acquisition time (a couple of seconds), compatible withon-line separations
High throughput (no slits)
Low resolution (2 nm)
-
8/6/2019 UVVIS-Spectroscopy p Bambang
35/35
HPLC-UV
Mobile
phase
HPLC
Pump
syringe
6-port
valveSample
loop
HPLC
column
UV
detector
Solvent
waste