final report project #28 optimization of bulk
TRANSCRIPT
Aalto University
ELEC-E8002 Project work course
Year 2016
Final Report
Project #28
Optimization of Bulk Micromachined Sidewalls for MEMS Applications
Date: 18.12.2016
Haverinen Enni
Rehman Abdul
Ukkonen Markus
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Information page
Students
Haverinen Enni
Rehman Abdul
Ukkonen Markus
Project manager
Haverinen Enni
Official instructor
Österlund Elmeri
Starting date
11.1.2016
Approval
The instructor has accepted the final version of this document
Date: 16.12.2016
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Table of contents
Preface
1 Theory and pre-laboratory investigations ................................................................. 4
1.1 Etching Methods: ............................................................................................... 4 1.1.1 Wet etching ................................................................................................. 6 1.1.2 Dry etching ....................................................................................................... 7 1.1.2 Comparison of wet and dry etching methods ............................................ 17
1.2 List of etching parameters and concepts .......................................................... 18
2 Characterization of Etching Results: ....................................................................... 19 2.1 Characterization methods ................................................................................. 19
2.1.1 Characterization methods used in this project .......................................... 19
2.1.2 Other characterization methods................................................................. 24 2.2 Comparison of characterization methods ......................................................... 25
3 Detailed schedule of experimental part and test plan .............................................. 25 3.1 Selected etching parameters ............................................................................. 26
4 Experiments, sample fabrication and characterization............................................ 26
4.1 Lithography ...................................................................................................... 26 4.2 Etching .............................................................................................................. 27 4.3 Wafer preparations before characterization...................................................... 33
4.3.1 Dicing ........................................................................................................ 33 4.3.2 Molding ..................................................................................................... 33
4.3.3 Grinding .................................................................................................... 33 4.3.4 Polishing .................................................................................................... 33
4.4 Characterization results .................................................................................... 34
4.4.1 Selected method and equipment ............................................................... 34
4.4.2 Measurements ........................................................................................... 35 4.4.3 Smoothness analysis ................................................................................. 37
5 Discussion and conclusions .................................................................................... 39
References
Appendix
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Preface
When a combination of integrated circuit manufacturing and micro machining processes, in which
material is formed by etching away micro layers is used to produce electrical systems implanted
with micro mechanical devices, it results in the formation of Micro Electro Mechanical System
(MEMS). MEMS consists of mechanical elements, sensors, actuators, and electrical devices on a
substrate. Silicon is the most common material used in MEMS owing to its semiconductor,
physical and commercial properties. [1] MEMS have numerous applications in the fields of aerospace, automotive and biomedical
engineering as well as wireless and optical communications. Micro-mirrors, gear trains, optical
scanners and pressure sensors are various types of MEMS devices. MEMS can consist of a
combination of components in various scales such as Nano, Micro, and Milli. Pressure, chemical
and inertial sensors (accelerometers, gyroscopes) are the most commonly used sensors in MEMS.
These sensors require actuation in order to perform their desired function. Electrostatic, thermal
and magnetic methods are the most frequently used actuation methods while for the last few years
piezoelectric actuation methods are on the rise. Piezoelectric actuation offers many advantages
over other methods but currently its implementation is quite challenging. [2] This project work contained two parts: theoretical and experimental. In the theoretical part,
various actuation methods using different sources such as books, papers and patents were
investigated and compared. The performance of the methods, different structures and their
fabrication techniques were the key points that were studied. Afterwards different micro-
fabrication etching methods were investigated that were possible to use in the fabrication of an
in-plane piezoelectric actuator. At the end, different key parameters were considered that could
be used to characterize the etching results.
The main goal of the project was to find a suitable etching method that can be used to reduce the
roughness of the material side-walls. In the experimental part, various etching methods such as
Reactive Ion Etching (RIE) and Deep Reactive Ion Etching (DRIE) which were studied and
compared in detail were checked in terms of their practical feasibility. Different parameters such
as the gas flow rate, pressure, operating temperature and power were taken into account to find
the most suitable method. By keeping in view the available facilities RIE was selected as the
method to be done in the laboratory. RIE was used in the preparation of the wafer, afterwards
different parameters were varied and results were measured to check the nature of the material
side-walls.
The experimental paper consists of five chapters. Chapter 1 introduces the different types of
etching methods such as wet and dry etching. Chapter 2 gives a detailed explanation about the
parameters that can be used for the characterization of the etching results. Detailed schedule of
test plan and experimental part are presented in Chapter 3. Chapter 4 details the results of
experiments carried out in the laboratory. At last, the conclusions based on results are summarized
in Chapter 5.
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1 Theory and pre-laboratory investigations
1.1 Etching Methods:
In microfabrication, materials on the surface of the wafer are eroded and attacked chemically
and/or physically by etchants during the manufacturing. The etching process might have many
etching steps. The material which is not want to be etched is protected by a mask which prevent
etchant from affecting in unwanted areas. Often the mask is made from photoresist material and
it is patterned by photolithography. In harsh conditions, where normal masks are not suitable,
more resist masks are used (so called hard masks) or etching is done without masks. In photolithography (or optical lithography or UV lithography) photomask and UV light
(produced by UV lamps or lasers) is used to expose the wafer with photosensitive film (also
known as photoresist). By UV-light it is possible to form a photoresist patterns and open areas on
the underlying material which can be then for example etched away. [3] Photolithography has the following steps: Surface is prepared for lithography by baking and priming (or so called adhesion promotion). In
baking step absorbed water is removed and in priming step wafer comes hydrophobic so it protects
the wafer from the cleanroom humidity variations. After preparations, the resist is applied on the wafer by spin coating. The resist can be positive or
negative resist. First a few milliliters of resist are applied on the wafer and then wafer is rotated
so that resist is spreaded over the wafer. Typical resist thickness on the wafer is 1 um. The spin-
coated resist is then usually baked in an oven or hotplate in carefully selected temperature. In
Figure 1 below is shown the spin coating process:
Figure 1: Spin coating process in lithography [3] The resist-covered mask is inserted into the tool, which works as a mask aligner. This tool is also
used to exposure the photoresist by UV-light. If the wafer and the photomask has intimate contact,
the photolithography is so called contact lithography. If there is a gap (for example size of 3 - 50
um) between wafer and mask, lithography is called proximity lithography. [3]
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After UV-light exposure, the wafer is ready for etching. After the etching process, the rest of
photosensitive film is removed from the wafer. In the following figure 2 can be seen
photolithography steps:
Figure 2: Photolithography process. [3] Etching methods can be divided roughly in two categories: wet etching and plasma etching (or so
called dry etching). Both etching methods have a same procedure: first the etchants are transported
to the surface by diffusion or flow and then etchant reacts with the surface. Finally, the product
species are removed by diffusion or flow. The basic reactions in wet and plasma etching can be presented by the following formulas: Wet etching: liquid etchant + solid → soluble products
Plasma etching: gaseous etchant + solid → volatile products
Both etching methods, plasma and wet etching, can be also divided into isotropic and anisotropic
etching. In isotropic etching the etchant etches into the surface of the substrate horizontally and
vertically. Anisotropic etching profile is more vertical or totally vertical. Most of the wet etchants
results in an isotropic profile, accept potassium hydroxide (KOH), which is anisotropic wet
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etchant for silicon. That’ is why the wet etchants are not usually used when the directionality is
important. In plasma etching, the profile can be isotropic or anisotropic, depending on used
etching parameters Anisotropic etching can be used to create fine structure fabrication. Isotropic
etching can’t be used in fine structure fabrication, because the isotropic etching results
undercutting in the material below the mask. This is sometimes desirable but often it is not. This
phenomenon can be prevented by using the larger mask than desired width. [3] In the following chapter, wet and dry etching methods are presented more specifically. In this
project, the main goal is to results anisotropic and smooth sidewalls in silicon. Both dry and wet
etching can be used in this purpose. However, in this project we focus on dry etching, due to
available time and its easiness compared with wet etching. During the wet etching, large number
of chemicals are used and it requires better knowledge of chemistry and safety. For that reason,
wet etching was dropped out in this project.
1.1.1 Wet etching
In wet etching liquid etchants are used to remove material on the surface of the substrate. Almost
every material can be etched by wet etching except for example Gallium nitride (GaN) or
diamond. Wet etching can be divided into two categories: metal etching and insulator etching.
Metal etching is based on electron transfer and insulator etching on acid-based reaction. Wet
etching is done in tank, where is also temperature and heating controls. This tank is filled with
water and certain etchants. Wafers are immersed in that tank for a certain etching time. After
immersion, the wafers are transferred to rinsing. Wet etching can be also done by the spray tool
without immersing the wafer in liquid. The disadvantage of this method is that only one wafer
can be etched at once compared with immersion, where multiple wafers can be etched at the same
time. Advantage of spray method is that the needed number of chemicals is lower than in
immersion. Isotropic and anisotropic etching are both possible with wet etching. Typical anisotropic wet
etchants in silicon and silicon dioxide etching are potassium hydroxide (KOH),
tetramethylammonium hydroxide (TMAH) and ethylenediamine pyrocatechol (EDP). In
anisotropic etching the etch rates depends on different silicon crystal planes. For example, KOH
etches 200 times faster silicon (100) crystal planes than silicon (111) planes. Wet etching can be
done with or without the mask and the etchants are selected based on this. [3, 4] The comparison between KOH, TMAH and EDP etchants can be seen in the table below.
Tetramethylammonium hydroxide (TMAH) and ethylenediamine pyrocatechol (EDP) are weak
anisotropic etchants. This can be seen from etch rate ratios for example between (100) and (111)
orientations. Potassium hydroxide (KOH) is strongly anisotropic. In this project the selectivity of
(110)/(111) orientations needs to be very high. From table 1 can be seen that KOH has the highest
etch rate ratio (600), which means high selectivity.
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Table 1: Typical anisotropic wet etchants and their etch rates ratios, etch rates, disadvantages and
advantages. [5]
Most common isotropic wet etchants for silicon are a mixture of different acids, for example
mixtures of nitric acid (for example Hydrofluoric Nitric Acetic (HNA), used with silicon),
hydrofluoric acid (HF, usually used with silicon dioxide) and acetic acid. Etch rates can be
controlled by using different concentrations of etchants. In the following Table 2 advantages and disadvantages of anisotropic and isotropic wet etching
can be seen: Table 2: Advantages and disadvantages of isotropic and anisotropic etching [6]
Isotropic Wet Etching Anisotropic Wet Etching
Advantages High selectivity Simple Low cost
Orientation specific etching (can be also
disadvantage, depending on application) Etch rates can be controlled Specific and smaller etch patterns Low cost
Disadvantages Contamination Pollution Extremely dangerous
(especially Hydrofluoric Acid
HF) Etch rates varies highly by
etchant concentration and
temperature
Etch rates varies by etchant concentration
and temperature Undercutting Contamination
1.1.2 Dry etching
In dry etching, the material on the surface of substrate material is etched by the etchant gases or
plasmas instead of liquid etchants. The etching reactions are based on chemical reactions
(chemical dry etching, vapor phase etching) and/or high kinetic energy of the particle, like the
electron, photon or ion beams (physical dry etching, ion bombardment). With dry (anisotropic)
etching it is possible to etch devices with high packaging density. The most common dry etching methods are plasma based methods like Reactive Ion Etching
(RIE) and Deep Reactive Ion Etching (DRIE). In this work, RIE will most likely be used. Other
dry etching methods are for example ion beam etching (IBE), chemically assisted ion-beam
etching (CAIBE), reactive ion-beam etching (RIBE), magnetically enhanced ion etching (MIE),
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magnetically enhanced reactive ion etching (MERIE), plasma etching (PE) and barrel etching.
These methods are not included in this experimental paper. [3,7]
1.1.1.1 Reactive Ion Etching (RIE)
Reactive Ion etching (RIE) is a dry directional etching process which utilizes ion bombardment
to remove material from the surface. RIE method is mostly preferred for etching in the vertical
direction as it provides a much stronger etch, while giving the flexibility for directional etching.
RIE is a combination of chemical (reactive) and physical (bombardment) processes. It uses
chemically reactive plasma to remove material deposited on wafers. Plasma is initiated in the system by applying a strong RF electromagnetic field to the wafer platter.
In each cycle, the electrons are accelerated by a strong electrical field between the electrodes. The electrons are accelerated upwards and downwards in the chamber, as a result of which the
electrons occasionally collide with the walls of the chamber and the wafer plate. During these
collisions, many large ions move very little in response to the RF electric field. The electrons that
flow in the upward direction are absorbed by the chamber walls and are released out of the ground.
While, the electrons that are deposited on the wafer plate builds up a negative charge on the plate
due to the DC isolation. Due to the presence of large number of positive ions compared with free
electrons, the plasma develops a slightly positive charge. Because of the large voltage difference,
the positive ions are attracted towards the wafer plate, where they collide with the samples to be
etched. The ions react chemically with the materials on the surface of the samples, resulting in
the etching of the material. Masks are used to cover the parts of the sample that do not need
etching. Various process parameters, like pressure, gas flows, and RF power effects the RIE
process. [8] There are different etching gases that suit for different situations. Silicon is easily etched by
halogens: fluorines, chlorines and bromines. [3,9] Highly anisotropic, high resolution and
enhanced structure are few advantages of the RIE process while low etch rate, low level of
selectivity and surface damages are the few disadvantages.
Figure 3: RIE setup. [9]
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RIE processes make etching independent of the crystal orientation possible. The etch rates
achieved in RIE processes are also higher than those of the most wet chemical etchants. RIE is
mainly used for surface processing, whereas the ICP is fitted with a deep silicon trench etch
process. The DRIE process is high rate anisotropic silicon etch process using fluorine based gases. It is
dry etch micromachining method, where high density plasma (HDP) and inductively couple
plasma (ICP) are used. Deep trenches of high aspect ratio and 90° sidewall angle can be achieved
using a low-pressure, high density plasma source. Vertical sidewalls, fine resolution and high
aspect ratio are few advantages of the DRIE while the use of high plasma power, single wafer at
a time and specialized hardware are the few disadvantages. [10] DRIE can be mainly divided into two categories: Bosch process: This process was developed by German company - Robert Bosch in 1994. Cycling two-steps
process occurs between deposition and etch steps. [10] First step is the standard isotropic plasma
etch process while the second step consists of passivation layer deposition. In this process, a
fluorine based plasma chemistry combined with a fluorocarbon plasma process is used to etch
silicon and to provide sidewall passivation and improved selectivity to masking materials. A
complete etch process travels between etch and deposition steps many times to achieve deep
vertical etch profiles. The process depends upon the source gases being broken down in a high-
density plasma region before reaching the wafer, which has a small but controlled voltage drop
from the plasma. This technique cannot be performed in reactive ion etch systems (RIE), as these
have the wrong balance of ions to free radical species. Fast pumping, fast response mass flow
controllers, separation between wafer and ICP region, short mixed gas line and high efficiency
wafer cooling are the fundamentals of a good Bosch etching system. [11] Cryogenic process: It is a single step process in which etch gas and passivation gas are released at the same time. This
process is done at cryogenic temperature i.e. <-110°C [10]. This process uses SF6 to provide
fluorine radicals for silicon etching. The silicon is removed in the form of SiF4. The main
difference between Bosch and Cryogenic process is mask protection and in the mechanism of
sidewall passivation. Rather than using a fluorocarbon polymer, this process relies on forming a
blocking layer of oxide/fluoride (SiOxFy) on the sidewalls together with cryogenic temperatures.
The low temperature operation also assists in reducing the etch rate of the mask material, which
is normally either photoresist or silicon dioxide. [12]
1.1.1.2 Photoresist and lithography
Photoresist mask is the most common mask and can be used for RIE. However, during etching,
the photoresist mask is slowly consumed. If the etching deepness is under 100 µm, 1 µm
photoresist mask should be enough. [13] DRIE, on the other hand, has some problems with photoresist masks. Photoresist masks have poor
selectivity compared to hard masks which means deep etching needs thick photoresist mask.
However, thick photoresist masks have some cracking issues: >1.5 µm photoresists are prone to
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cracking. Table 3 shows the cracking of five different photoresists during cryogenic DRIE. [13,
14] Table 3. Cracking of photoresist during cryogenic DRIE. [13]
Hard masks do not have cracking issues because their coefficients of thermal expansion are close
to silicon’s coefficient of thermal expansion. Three hard masks were tested in study [13]: silicon
oxide (SiO2), aluminum (Al) and aluminum oxide (Al2O3). None of them suffered cracking.
However, mask material did effect on surface quality. The aluminum mask caused micromasking
and formation of silicon “grass” under highly anisotropic etching conditions at the bottom of the
etched surface while Al2O3 led to smooth results (Figure 4). Silicon oxide also leads to excellent
quality. Selectivity of SiO2 is about 150:1 which is high in comparison with the photoresist mask.
Selectivity of Al2O3 is 32:1 for pure SF6 inductively coupled plasma but the study achieved the
selectivity of 66 000:1 with SF6/O2 plasma. Conclusion: For RIE, photoresist mask is fine. For DRIE, if the etching is shallow enough (<100
µm), a thin (<1 µm) photoresist mask should be enough. If we need to etch deeper, hard mask
should be chosen. Both silicon oxide and aluminum oxide are viable materials but silicon oxide
has lower selectivity which means a thicker mask is needed. .
Figure 4. Effect of masking material on the quality of etched surfaces. a) Al, b) Al2O3 [14]
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1.1.1.3 Parameters in RIE and DRIE and how they affect to etching
results
In Micronova, there are two different RIE etchers: inductively coupled plasma etcher Oxford
Plasmalab 100 and reactive ion etcher Oxford Plasmalab 80. Both etchers can be used to etch
silicon. In the following table 4 is presented the key specifications of these two etchers. Table 4: The key specifications of Oxford Plasmalab 100 and 80. [15, 16, 17]
Inductively Coupled Plasma
Etcher Plasmalab 100 Reactive Ion Etcher Plasmalab 80
Power sources Two sources: - ICP source 2 kW - CCP source 300 W
RF power: 20 - 250 W
Etch and process gases - BCl3, Cl2, SiCl4, SF6, H2 and
O2/N2/Ar SF6, CF4, O2, Ar and CHF3
Operating Temperature From - 150 °C to + 400 °C -
Typical etch rate for silicon
/ maximum etch rate Typ. 2 - 3 μm/min / max. 8 μm/min 300 nm/min
Substrate size Max. 100 mm wafer Up to 240 mm, optimized
for 100 mm
Pressure range 1 - 100 mtorr 5 - 250 mTorr
In this project work, there is a need for suitable etching parameters which can be used in the
process. In this chapter, the main processes parameters, for example etch gases and their flow
rates, temperatures, pressures and power of sources are briefly explained. Etching gases, gas flow rate and gas compositions Reactive ion etching process is an anisotropic process due to directional ion bombardment and it
is not dependent on crystalline structure. For silicon, suitable etching gases are fluorines, chlorines
and bromines (halogens). Fluorine is more reactive gas on silicon than chlorine and bromine. This
is due to fact that fluorine radicals react strongly with silicon while chlorine and bromine radicals
don’t etch silicon spontaneously. When fluorine etchant gases (for example SF6 and CF4) are used,
fluorine radicals might etch also sidewalls and make the etch profile less anisotropic. This can be
prevented by using less reactive etchants or passivation layer, which are protecting the sidewalls.
Advantage of more reactive etchant gases is that the etching rate is higher. [13] In deep reactive ion etching processes (cryo and Bosch) inductively coupled fluorine based
plasmas are used. To achieve anisotropy, passivation layers are used. In Bosch process passivation
is separate process step while in cryo-process passivation and etching occurs at the same time. By
cryogenic-process it is possible to produce smooth sidewalls. [13]
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Typical etchant gases are presented in the following table 5. Under the table are also brief
description of used gases in etching process for silicon. Also, effects of gas flow rates,
temperature, system power and pressure are briefly explained. Table 5: Examples of different solids and etch gases and their products. [18]
Sulfur hexafluoride (SF6): The most typical feed gas in generation of active species which is
used in silicon etching. Sulfur hexafluoride forms positive and negative ions (SF5+ and F-) and
neutral fluorine radicals (F*). Oxygen (O2): Oxygen is used in cleaning in the plasma ashing, which is removing the photoresist
(carbon based) from an etched wafer. Oxygen also removes organic matter and the contaminant
from the wafer. It can be also used as an etchant in combination with other etchant gases. In this
case, oxygen can be used for example with sulfur hexafluoride (SF6) or carbon tetrafluoride (CF4).
The mixture of these gases results a silicon oxyfluoride (SiOxFy) passivation layer. By adding or
removing the amount of oxygen (more specifically oxygen flow rate) it is possible to effect on
the etch rate. In the other hand, using too much oxidation might result over passivation. [19] Argon (Ar): While oxygen is capable of surface modification, argon is used only in surface
cleaning. Because oxygen oxidizes some materials (silver, copper etc.), argon is used instead of
it. [19] Carbon hydro trifluoride (CHF3): can be used to produce passivation layer when fluorine
contain plasma is used. Hydrogen is used to catalyze for example CF, which is polymeric
precursor and it forms HF with fluorine radicals, which decreases reactions with sidewalls. [13] Etchant gas flow effects on the etch rate of silicon. For example, in case of SF6, higher SF6 flow
rate and power of plasma produces more fluorine radicals and thus silicon etch rate increases.
Especially in Bosch process where higher temperatures and separate passivation and etching steps
are used, extremely high speed mass flow controllers are required. [13] Temperature is the one of the main parameters in the etching process and it affects in many ways
to the etching results, for example, selectivity, the etch rate and the profile are all dependent on
substrate temperature. Temperature also affects the reactions during the etching, for example the
probability of radicals to react with sidewalls is temperature dependent. Temperature also affect
on production of the passivation layer and its quality in case of using the
tetrafluoromethane/oxygen (CF4/O2) gas mixture. The passivation layer is more stable in
cryogenic temperatures (T < - 100 °C), but lower temperature can cause also over passivation
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with the high oxygen flow rate and a low bias voltage. Higher temperatures produce more
isotropic etching profile. One option to enhance the anisotropic etching is to use helium backside
cooling which prevents radicals to react with sidewalls. [20] Power of plasma and substrate: affects highly to etch rate of silicon. [13] Plasma pressure affects to selectivity of silicon oxide and silicon, anisotropy and etch rate. [21] Figure 5 contains process parameters and how they effect on etch rate, profile, selectivity and
sidewall roughness. In our project, it is important to result in the anisotropic etching profile with
smooth vertical sidewalls. From Figure 5 it can be seen that to achieve smooth sidewalls, etch
rate needs to be small (less etch gas) and pressure and etch coil power need to be low.
Figure 5: General process trends for controlling process results. [18]
1.1.2.4. RIE etching parameters examples
The etching parameters which were used was selected based on a few found studies, which are
presented in this chapter. The main criteria for the parameters was that they are suitable for Oxford
Instruments PlasmaLab 80 RIE etcher (see table 4 in page 10 above). Used etcher limited also
available power and temperature range selection, for example cryogenic temperatures were not
available in our project. It was also known that PlasmaLab 80 RIE etcher was not optimal to etch
deep structures. Micronova has another etcher, PlasmaLab 100, which is inductively coupled
plasma etcher (ICP-RIE etcher) and more suitable for etching deep structures. Unfortunately,
during this etching process the etcher was out of use due to malfunction.
Process parameter study example 1 This process parameter example is based on article “Anisotropic Si deep beam etching with
profile control using SF6/O2 Plasma” (Zou, H) [22]. In this study, a single crystal silicon etching
was done by traditional reactive ion etcher by using SF6 and O2 as process gases. Also, PlasmaLab
80+ was used in this case. Study was focus on how oxygen concentration and system pressure
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effect on the etch profile and rate. Table 6 contains parameters, which were used in this study.
Presented parameters were suitable for our case too, because parameters are available to use in
PlasmaLab 80 which is etcher used in this project. These parameters are also resulting in the
anisotropic etching, with is desirable in our case. Table 6: Parameters used in study example 1. [22]
Process parameter study example 2 This example is based on Pierpaolo Spinelli’s doctoral dissertation “Light trapping in solar cells
using resonant nanostructures” [21]. In this study silicon was etched by using SF6 and CHF3 as a
process gas. Also, PlasmaLab 80+ plasma etcher was used in this study. First the variation between pressure and power in the system was studied while gas (CHF3, SF6
and O2) concentrations were constant (case 1). Secondly, the variation of SF6 and O2
concentrations was studied while CHF3 concentration was constant (case 2). The main
conclusions of this study were that plasma pressure affects to SiO2 and Si selectivity, anisotropy
and the etch rate. Also, system power has an impact on the etch rate. In this study, it was also
noticed that presence of CHF3 gas yields smoother surfaces after etching but also it decreases
selectivity of Si and SiO2. Also, presence of SF6 increases etch depth and presence of O2 creates
a passivation layer on the vertical Si surface, which prevents plasmafrom etching along the
horizontal directions. In Tables 7 and 8 below is presented used parameters in this study. Some of the parameters are
not suitable in our case, for example in table x power 350 W due to our equipment own power
limits (maximum power is 250 W). Table 7: Case 1 parameters
CHF6 17 sccm
SF6 20 sccm
O2 14 sccm
Plasma Pressure 20, 60 and 100 mTorr
Power 150, 250 and 350 W
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Table 8: Case 2 parameters
CHF6 25 sccm
SF6 15 sccm and 25 sccm
O2 No O2 and O2 with 10 sccm flow rate
Plasma Pressure 7 mTorr
Power 150 W
Process parameter study example 3 This study example is based on study “Anisotropic Reactive Ion Etching Using SF6/O2/CHF3 Gas
Mixtures” (Jansen, H et al.) [23]. In this study gas (SF6, O2 and CHF3) concentrations, pressure
and power varied and their effect on anisotropy and surface smoothness was studied. From the following tables, can be seen different test runs and used parameters. In Table 9 is
presented variable settings which were used in this study. In Table 10 is shown used variables in
each test runs and in Table 11 the test results. In our project, the main goal is etching smooth and
anisotropic (when A is close to 1, etching results in vertical sidewalls) etching profiles. In Tables
10 and 11 test runs which are suitable for this project are marked with red boxes.
Table 9: Variable settings in study example 3. [23]
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Table 10: Test runs and used variables in study example 3. Suitable test runs for this project are
marked with red boxes. [23]
Table 11: Test results in study example 3. Suitable test runs for this project are marked with red
boxes. [23]
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As a summary, in table 12 is shown usable parameter variables in our project. Also, selectivity,
etch rate, surface smoothness and anisotropy is shown in the same table. Table 12: Summary of suitable parameter variables based on study example 3.
Run
no. SF6
[sccm] O2
[sccm] CHF3
[sccm] Pressure
[mTorr] Power
[w] Etch rate
[um/min] Anisotropy Surface
7 20 14 17 60 140 0.42 0.980 Smooth
8 40 14 17 60 60 0.31 0.960 Smooth
16 40 14 17 140 140 0.58 0.940 Smooth
27-
32 30 10 12 100 100 0.43 -
0.45 0.94 -0.97 Smooth
In a project meeting we decided to use process parameters which was used in example 3 with a
few modifications. The main criteria for the selected parameters was that they produce highly
anisotropic and smooth vertical sidewalls. The selected parameters are explained more in chapter
“3.1 Selected lithography and etching parameters”.
1.1.2 Comparison of wet and dry etching methods
From the following Table 13, can be seen the comparison between wet and dry etching. Table 13: Wet and Dry Etching [7]
Parameter Wet Etching Dry Etching
Materials that can be etched Almost all materials Only certain materials
Etch rate Fast (typical 1 um/min) Slow (0.1 um/min)
Linewidth control Poor Very good
Selectivity Can be very high Poor
Radiation damage No damage Might be severe
Chemical cost High Low
Equipment cost Inexpensive Expensive
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1.2 List of etching parameters and concepts
Selectivity: It is the ratio of etch rates in two materials. When selectivity is high, underlying
material stays unharmed during the etching and when it is poor, etch removes both materials: the
top layer and underlying material. For example, when two similar materials are etched, selectivity
can be very poor and etchant works similarly in both materials. When selectivity is very high,
underlying material works as an etch stop: etching stops entirely when material is reached. High
selectivity is often very important in etching processes. Etch bias: Etched depth in underlying material, for example, isotropic etchant has a large etch
bias. Etch rate and time: Etch rate = Etched depth / etch time (e.g. µm/min) Linewidth (or Critical Dimensions; CD): Deviation in etching results compared with designed etching results [%]. Especially critical in the
integrated circuits. Profile: The profile of the etching result, measured from a top view of the object by SEM or optical
measurements. Temperature and etchant concentration in wet etching: Temperature and etchant concentration are the main parameters during the etching process. By
heating and higher concentration, it’s possible to enhance the etching. Used temperature can also
limit usage of photoresist materials as a mask. Passivation layer: In dry plasma etching, passivation layer is used to enhance process anisotropy
because it enhances directionality of the etching. Isotropic and anisotropic etching:
Figure 6: Isotropic and anisotropic etching profiles. [4] The anisotropy A can be defined by the following formula:
𝐴 = 1 − 𝑉
𝐻 (1)
Where H is denoted as the etch depth and V as a maximal undercut of the mask or lateral extension
of the sidewall. When A is one, no mask undercut occurs and sidewalls are perfectly vertical. [23]
19
2 Characterization of Etching Results:
2.1 Characterization methods
In this work, the quality of the etched sidewalls is important and it needs to be characterized.
There are different characterization methods that can be used to find out the crystal quality of an
etched surface. Some of the most common methods are discussed in this chapter.
2.1.1 Characterization methods used in this project
In this project, the main usable characterization methods are scanning electron microscopy
(SEM), transmission electron microscopy (TEM) and atomic force microscopy (AFM). These
methods are practical and easy to use, except TEM, which requires more preparation before the
characterization. For that reason and the lack of time TEM and AFM were dropped out from our
project, but these methods are presented in this chapter with SEM. Also, other characterization
methods are presented briefly although they are not so suitable for our purposes.
Scanning electron microscopy (SEM) Scanning electron microscopy (SEM) is a basic electron microscopy technique. Instead of light,
SEM is based on the electron beam which is used to scan a sample to produce an image of the
sample. With this technique, it is possible to get information about microstructural or chemical
composition of the sample. SEM is used widely for example in nanotechnology, because it has
much better resolution (around 1 nm at its best) than traditional light based microscopes. This is
due to the shorter wavelengths of electrons compared with light wavelengths. [24] Structure of scanning electron microscope is shown in Figure 7. It consists of an electron gun,
anode(s), a series of electromagnetic lenses, coils for scanning and apertures. Samples are placed
in sample stage which in inside of the vacuum chamber. In the vacuum chamber, there is also X-
ray and scattered electron -detectors. Microscope has electronics for signal processing which is
used to display graphs and images on a monitor. [24]
Figure 7: Structure of scanning electron microscope
20
In SEM system electron gun is used to produce a high current and small spot size electron beam.
Electron guns are divided typically in two main types which are thermionic and field-emission
electron guns. Thermionic electron gun is based on a heated filament, which emits electrons which
are then accelerated toward the anode. The field-emission electron gun is based on very sharp and
single-crystal tungsten tip, which is used to extract electrons. In this type of electron gun, two
anodes are used. First anode is used to regulate field strength and emission current at the tip and
another anode is used to accelerate the electrons to their final operating voltage. With the field-
emission electron gun it is possible to produce much higher light source and lower energy
dispersion than wit thermionic electron gun, but the thermionic gun can be used without ultra-
high vacuum in contrast to field-emission gun where high-vacuum is required. The electromagnetic lenses are used to focus and demagnify the electron beam. These lenses
consist of soft-iron shell whose inside contains copper coils, which generates a magnetic field.
By changing a field strength, it is possible to change focal point and change spot size. To get high
resolution it is very important to reduce the diameter of the electron beam. In addition to lenses,
apertures are used to exclude scattered electrons and control spherical aberrations. Electron beam
scanning is produced by scan coils, which are used to move the electron beam along the x- and y-
axis over the surface of the sample. Therefore, with scan coils and detectors it is possible to create
a point-to-point image of the sample. After the electron beam is produced by the electron gun, lenses and apertures, the beam is
interacting with the sample, which is inserted in the sample stage in the vacuum. In this
interaction, mainly two processes are involved: inelastic scattering and elastic scattering (Figure
8 a). In Figure 8 b) the different zones of signal emissions are shown. [24]
Figure 8: a) Elastic and inelastic scattering and [25] b) different zones of signal emissions [24]. In elastic scattering the beam electron hits a sample’s outer-shell electrons or atomic nucleus. In
this collision, the electron has negligible energy loss, but the directionality of the electron changes.
These electrons are called the backscattered electrons (BSE) if the directional change is more than
90 ° and they produce a useful imaging signal. Number of backscattered electrons are dependent
on atomic-number of sample atoms: if the atom is high atomic-number, the collision produces
more backscattered electrons and hence higher signal. That is why BSEs are used to detect
different chemical compositions.
21
In inelastic scattering the most of the energy is transferred to a sample electron. In this case, low
energy secondary electrons (SE) are ejected from the sample when the electron beam hit the
sample. The atom is ionized when the secondary electron is ejected from inner orbital. This results
in a vacancy, which is filled by the electron from outer-shell and after this X-ray photon or another
electron (so called Auger electron) is emitted. Auger electron and X-ray photon which are emitted
and then detected, can give chemical information about the sample. The number of emitted
secondary electrons are independent of the atomic-number. Even though SEM is the most useful characterization tool in nanotechnology it also has
limitations. The main limitations of SEM are lens aberrations, imaging of the insulating samples,
radiation damage and contamination. Lens aberrations might cause problems in focusing the beam and it might affect on the diameter
of the beam. This affects also directly to resolution. These aberrations can be so called spherical
and chromatic aberrations or astigmatism. The spherical aberration has occurred when the
electrons are focused differently depending on where they entered in the lens. This can be
prevented by using apertures. The chromatic aberration means an energy spread of the electrons
in the primary beam. This can be also prevented by a smaller aperture. Asymmetries in the
magnetic field and contamination on lenses or apertures might cause astigmatism, which effect
on the focal lengths and the beam diameter. This can be fixed by using the stigmators. When the sample is bombardment by high-energy electrons, insulating the sample comes quickly
negatively charged, which makes sample imaging difficult. This can be prevented by sputter-
coating with a conductive material on the sample, which provides a ground plane for the electrical
field. The coating materials are usually platinum, palladium or gold. The bombardment of high-energy electrons might also cause radiation damage (for example
burning) on the surface of the sample. The damage will be worse if the beam is scanned over the
sample. This usually creates problems in scanning very soft materials. This can be avoided by
adjusting the strength of the beam. Also, contaminations can affect on the imaging results. Main sources of contamination come for
example from atmospheric particles and finger marks of the user. This needs to be taken into
account while using SEM. [24]
Transmission Electron Microscopy (TEM) Transmission electron microscopy (TEM) is based on accelerated electrons which are interacting
with the sample under the examination, so it is a very similar technique as scanning electron
microscopy (SEM). The main difference between these microscopy technologies is that in TEM
imaging signals are obtained from electrons which are transmitted through the sample whereas in
SEM signals are obtained from scattered electrons. TEM is used excessively in nanotechnology,
because by TEM it is possible achieve 0.2 nm resolution and study chemical information of the
sample. TEM can be also used to study the composition, morphology and internal structure (for
example symmetry of crystals) of the sample. Similar to SEM, TEM also consists of almost the same components: the electron gun,
electromagnetic lenses, apertures sample stage and vacuum. Electrons which, are produced by the
electron gun, are accelerated in a vacuum. Used acceleration voltages are typically 80 - 300 kV.
After this electron beam is focused on the sample by apertures and electromagnetic lenses. The
22
most of the electrons don’t lose energy or change direction when they transmit through the
sample. The final image is usually detected by a sensor (for example charge-coupled device,
CCD) and displayed fluorescent viewing screen. Sample the need to insert into sample stage,
which is also sealed in the vacuum. There are few different type of TEM techniques. One of them is conventional TEM (CTEM),
which is an original form of TEM. It uses a stationary beam, which can be parallel or convergent.
The scanning transmission electron microscopy (STEM) differs from CTEM so that the electron
beam is used to scan over the sample. Scanning can be done for example by scanning coils as in
the case of SEM. Other modifications of TEM are for example low-voltage electron microscope
(LVEM) which uses lower acceleration voltages and cryo-microscopy where samples are imaged
in cryogenic temperatures. [24] Before using TEM, samples need to be prepared thin enough (about 20 - 100 nm), because sample
needs to be transparent for electrons. Depending on the sample, preparation can be made by
different ways as electropolishing (metals and alloys), mechanical polishing, ion beam thinning
or samples can be dispersed in a solution. Sample preparation can be destructive so it is need to
be done with care. The preparation can also take a lot of time, which is one disadvantage of using
TEM. [26] TEM has some limitations, which some of them are similar in case of SEM. The electron beam
can cause severe damage to the sample, which can make imaging difficult. Also, vacuum
environment differs from normal environment, which need to be taken into account in some
samples (mainly in biological samples). With TEM it is only possible to produce 2D-pictures (in
contrast to SEM, which can produce 3D-pictures) and the area which can be studied at once is
very small. This might cause problems and missed information from local points if it is assumed
that the small imaged part represents the whole sample. [24] In Table 14, the main differences of SEM and TEM are presented. Table 14: Differences of SEM and TEM. [24]
Scanning electron
microscopy (SEM)
Transmission electron
microscopy (TEM)
Detected electrons Scattered electrons Transmitted electrons
Imaged areas Surface of a sample Internal composition
Dimensions of picture 3D 2D
Number of samples which can be
analysed at once
Large Small
Resolution 4 nm 0.2 nm
23
Atomic Force Microscopy (AFM) Atomic force microscopy (AFM) is a very-high-resolution type of scanning probe microscope
that can reach a resolution of up to one tenth of nanometer. The operation principle is based on
scanning the surface of the sample with a flexible cantilever tip. While the tip moves across the
surface, the interatomic potentials force the cantilever to bounce up and down depending on the
surface. The motion of the cantilever is then measured. Figure 9 shows the basic setup of an AFM
system. [27]
Figure 9. AFM system. [27] AFM has three different scanning modes: contact mode, non-contact mode and the tapping mode.
In contact mode the probe is dragged across the surface and the up-down movement of the tip is
measured. This mode can damage the surface of the sample or even the tip itself but the resolution
is better than in non-contact mode. In non-contact mode the cantilever is vibrated close to its resonance frequency and the tip
oscillates just above the surface of the sample. Its resonance frequency and amplitude depend on
the distance between the tip and the surface. Either the resonance frequency or the amplitude is
kept constant via a feedback loop. The shape of the surface can then be measured by measuring
the change of the other non-constant parameter. This mode has a slow scan speed and the lateral
resolution is lower than in contact or the tapping mode but it does not damage the sample. In the tapping mode, the cantilever is also vibrated close to its resonance frequency but the
amplitude of the oscillation is 20-200 nm greater than in non-contact mode. However, in this
mode the tip makes contact with the surface in every oscillation cycle. The resolution is similar
to contact mode but does not damage the sample the same way contact mode does.
24
Sample preparation is rather easy in AFM when compared with SEM and TEM: scanning of non-
conductors (polymers) requires no special preparation. The possibility of radiation damage of the
sample is also non-existent because the scanning is based on molecular interactions. AFM produces direct 3D images of the surface of the sample with a lateral resolution of a few
nanometers and vertical resolution of less than 1 nm. AFM can also differentiate the type of
materials at the polymer surface. However, AFM is complex and susceptible to outside influences
like contamination of the surfaces and instrumentation control. [27]
2.1.2 Other characterization methods
Other characterization methods are listed below. These methods are not so practical in
this project and they might be more difficult to use.
Surface-enhanced Raman scattering (SERS)
● The sample is illuminated by laser beam and electromagnetic radiation is collected from
the spot with a lens and sent through a monochromator to CCD.
● Surface of the object is treated so that Raman scattering is enhanced.
● Allows the analyzation of the composition of a body
● Resolution: nanoscale, can even detect single molecules
● Non-destructive [28]
Ultraviolet-visible spectroscopy (UV-VIS)
● The sample is illuminated by UV-light which excites electrons into higher energy
levels. When electrons return back to lower energy states, light with different
wavelength is emitted and measured.
● Resolution: 1 nm
● Non-destructive [29]
X-ray diffraction (XRD)
● Based on illuminating the sample with X-rays and measuring the reflection.
● Suitable for crystal structures.
● Provides following information:
o Lattice parameters
o Misorientation of the lattice respect to the substrate
o Other lattice defects
o Lattice densities
o Strain, composition and thickness of the film
o Non-destructive
● Not so useful in this project. [30]
25
2.2 Comparison of characterization methods
From table 15 can be seen characterization method comparison where SEM, AFM and
TEM techniques are compared.
Table 15: Characterization methods comparison.
Technique Features Radiation
damage Best
resolution Sample preparation
SEM Surface topography Rarely
serious 4 nm Easy
AFM Surface topography None 0,3 nm Easiest
TEM Internal morphology, lamellar
and crystalline structures Severe 0,2 nm Difficult and time-
consuming
3 Detailed schedule of experimental part and test plan In Table 16, schedule of laboratory work for this autumn is shown. In September, our team is
focusing on theoretical part of experimental paper and selection of etching and characterization
methods. Also, the main parameters of etching and characterization are defined. At the beginning of the October, the training for the laboratory working starts. In this phase, we
will be trained to learn how to act in clean room and how we are using the machine which is used
in reactive ion etching. In our project, we are focusing on only in RI-etching due to lack of time.
The wet etching requires a large amount of chemicals and therefore it also requires more
experience of chemistry. For safety reasons, it is dropped out from our project. At the end of
experimental part, we get familiar with SEM which is selected as a characterization tool. TEM
and AFM are excluded from our project due to lack of time. At the end of October, we start
etching in clean room. This phase takes three weeks. After etching, characterization part starts on
November. This phase is planned to take four weeks. This phase includes sample preparations
and analysis of characterization results (for example SEM pictures). Table 16: Laboratory schedule in autumn 2016.
26
3.1 Selected etching parameters
In this project, five silicon wafers were etched. Wafers 1 - 4 had a silicon oxide layer on top of
the Si wafer as a mask. In Table 17 information is presented about wafers 1 - 4. Wafer 5 was a
dummy wafer, which didn’t have a SiO2 layer on top of the wafer. In table 18 below is shown
selected etching parameters, which are used in reactive ion etching. This table is based on study
example 3 which is presented in chapter 1.1.2.3 “Parameters in RIE and DRIE and how they affect
etching results”. In contrast to study example 3 some of the parameters were decided to keep
constant while SF6 flow rate and system pressure vary. Table 17: Properties of wafers 1 - 4, which will be RI-etched.
Properties of Wafers 1 - 4
Diameter 100 mm
Type n-doped
Orientation <100>
Resistivity 5 - 10 Ω-cm
Thickness of Si 525 μm
Thickness of SiO2 302 nm
Table 18: Selected parameters and their variations for reactive ion etching.
Run No. SF6 [sccm] O2 [sccm] CHF3 [sccm] Pressure p [mTorr] Power P [w]
1 20 14 17 60 140 W
2 20 14 17 140 140 W
3 40 14 17 60 140 W
4 40 14 17 140 140 W
4 Experiments, sample fabrication and characterization
4.1 Lithography
Wafer etching started first from lithography, which has several phases. First wafers were in
HMDS priming for 5 minutes at 145 °C temperature. Liquid Photoresist A2 5214E was used to
produce resist layers on top of the wafers. First wafer was inserted into the spinner (Spinner BLE
2F0817). A drop of photoresist was dropped on top of the wafer and spinning started (30 seconds
27
at 4 000 rpm). Nominal thickness of photoresist was 1.4 μm. After spinning there is also
possibility of unwanted air bubbles and particles, which might appear on the surface of the
photoresist. In this case, the resist needs to be taken care of by acetone and spinning needs to be
done once again. After spinning, residues of photoresist are cleaned from equipment with acetone.
Cleaning is the important phase, because dried photoresist flakes and particles can cause problems
to spinner users afterwards. After the photoresist was spread, the wafer was inserted into the hot plate (Unitemp GmbH HP-
220). Between the hot plate and wafer was set a dummy wafer to protect hot plate from chemicals.
The purpose of the hot plate was to make resist solid. The wafer was on the hot plate for 50
seconds. Soft baking can be also used to make resist to solid form, but it takes more time (about
one hour). After photoresist spinning, the wafer is ready for actual lithography. In our case wafers and mask
was inserted in Süss Microtec MA6/BA6 manual mask aligner. Used mask was made from plastic,
which has a lower resolution than the glass mask, but it is less expensive mask material. Vacuum
was used to hold the mask in its place. After the mask was set at its place, wafers were inserted
into the mask aligner. Microscope was used to check the right alignment of the wafer. Vacuum
was also used to hold the wafer in its place during the process.After alignment, the wafer was set
in contact with the mask. After this ultraviolet light (UV-light)) exposure started. The exposure
lasted a few seconds. After UV exposure, the wafers were transferred to the lithography development process which
finalizes the photoresist removal from UV-exposed areas. First wafers were set to Teflon coated
cassette and after this wafers were immersed in AZ 351B and DI-water dilution (1:5, 1400 ml of
AZ 351B and 7000 ml DI-water) for one minute. Afterwards wafers were rinsed in DI-water tank.
The rinse can be also done by DI-water gun. After rinse wafers was flushed by nitrogen gas.
Finally, wafers were set to rinse drier (Sitek) for a couple of minutes. Rinse drier also measures
the resistivity of water during the drying process. Resistivity of water tells amount of chemicals
which have left the wafer. After development process wafers were first set at their original cassette and then transferred to
hard baking, which was done in hot plate (Unitemp GmbH HP-220). Temperature of hot plate
was set to 120 °C and wafer was on the hot plate for 50 seconds. Hard baking was used in this
case, because in RIE there is a need for harder resist.
4.2 Etching
After lithography wafers were checked by profilometer (Dektak /XT Bruker) to check that
lithography was successful. Profilometers working principle is based on the tip, which scans the
surface of the wafer from selected areas. First the depth of UV-exposed areas was measured from
all wafers. In Table 19, below the measurement results are shown. The 5th wafer was measured
five times to be sure about the selectivity of resist.
28
Table 19: Measured depths of UV-exposed areas.
Wafer No. Measured depth [nm]
1 1265
1 1285
1 1262
2 1344
3 1273
4 1342
5 1342
5 1325
5 1317
5 1331
5 1339
After initial measurements, 5th wafer was etched by Oxford Instruments Plasmalab 80 RIE etcher.
In this etching case, the 5th wafer worked as a test wafer and etching parameters were selected
according to the worst selectivity case (test case no. 1 in page 24). Selected step time was 5 min,
temperature 15 °C, DC bias 304 V and valve position 33 °. After etching, 5th wafer was measured
again by profilometer. In table 20 below is shown measurement results. Table 20: Wafer no. 5, selectivity check. Process parameters according to the test case no. 1 in
page 24 (CHF3 = 17 sccm, SF6 = 20 sccm, O2 = 14 sccm, Power = 140 W, pressure = 60 mTorr).
Measurement No. Measured Depth [nm]
Silicon + photoresist
1 1945
2 1844
3 1832
4 1871
5 1990
From measurement results, can be seen that etch rate is smaller than expected, but it seems that
wafer was etched enough. Smaller etch rate might be also explained by the lower power level
(140 W), which was used during the etching.
29
When the 5th wafer was measured by profilometer, the wafer was transferred to the wet bench to
remove resist from the top of the wafer. First the wafer was inserted into UV-assisted tank with
100 % acetone. Ultrasound was used shake wafers in acetone. Usually, wafers are in this acetone
tank for ten minutes but in this case wafer was hold in a tank a little bit shorter time. After
ultrasound-assisted acetone tank wafer was transferred to another acetone (100%) bath and finally
to the final bath of 100 % isopropanol (IPA). After this wafer was also flushed with DI-water
gun and dried with nitrogen. After resist removal, the 5th wafer was measured with profilometer
to see how much the actual silicon was etched from the wafer. In Table 21 is shown the measured
depths of etched silicon. Table 21: Measured depths of etched silicon on wafer no. 5
Measurement No. Measured depth [nm] Silicon
1 945
2 953
3 1063
From table, can be seen that the silicon on the wafer were etched about 1 μm, which is below
from target etch depth (3 μm). Selected etching parameters was etching also a photoresist quite
much but overall the measurement results were quite good in this case. After the test wafer, no 5 was etched and measured, wafer no 1 was inserted into PlasmaLab 80
RIE etcher for a silicon dioxide etching, which is used as a mask on top of the silicon. Wafer no.1
was etched by following etching parameters:
● Step time: 9 minutes ● CHF3: 25 sccm ● Ar: 25 sccm ● Power: 200 W ● Pressure = 30 mTorr.
After wafer no. 1, the silicon oxide layers of wafers 2 - 4 were etched also with the same etching
parameters. After etching the wafers were transferred to profilometer. From the measurement
results, can be seen that silicon oxide layer was removed. In Table 22 and in Figure 10 below it
can be seen that the measured depths of wafers 2 - 4. The nominal thickness of SiO2 was 302 nm.
30
Table 22: Measured depths of wafer no. 1 - 4 after silicon oxide (SiO2) etching.
Measurement
No.
Measured Depth
[nm]
Wafer no. 1
Measured Depth
[nm]
Wafer no. 2
Measured Depth
[nm]
Wafer no. 3
Measured Depth
[nm]
Wafer no. 4
1 1566 1466 1489 844
2 1543 1568 1414 1329
3 1550 1561 1448 1536
4 x 1568 1430 1547
5 x 1568 1493 1152
Average 1553 1546,2 1454,8 1281,6
Stdev 11,79 44,94 35,20 293,98
Figure 10: A graphical illustration of measured etch depths after silicon oxide RIE etching. After silicon oxide etching and profilometer measurements the wafers no. 2 -4 were etched with
PlasmaLab 80 RIE etcher to etch silicon. Used etching parameters are listed in table 23 below.
Oxygen and CHF3 flow rates, system power and step time were kept constant in every etching
case. The step time was relatively high due to suspicion of low etch rate during the etching. The
SF6 flow rate and system pressure varied. After the etching wafers were clean with acetone and
isopropanol baths and measured with profilometer. Measured etch depths are shown in table 24
and in Figure 11 below. Figure 12 shows the profile of wafers in different profilometer
measurements.
31
Table 23: Etching parameters of wafers 1 - 4 used in Si etching.
Wafer
no.
O2
[sccm]
CHF3
[sccm]
SF6
[sccm]
Power
[W]
Pressure
[mTorr]
Step
time
[min]
Etch
rate
[μm/
min]
Selectivity
1 14 17 20 140 60 25 0.42 6.3
2 14 17 20 140 140 25 0.19 12
3 14 17 40 140 60 25 0.31 10
4 14 17 40 140 140 25 0.58 10
Table 24: Measured etch depths of wafers 1 - 4 after Si etching.
Measurement
No.
Measured Depth
[nm]
Wafer no. 1
Measured Depth
[nm]
Wafer no. 2
Measured Depth
[nm]
Wafer no. 3
Measured Depth
[nm]
Wafer no. 4
1 8576 12795 7221 19263
2 8847 12040 7546 18926
3 9140 12086 7368 19040
4 9003 12502 7401 20051
5 9052 13473 7398 19966
Average 8923,6 12579,2 7386,8 19449,2
Stdev 221,54 588,51 115,67 525,62
32
Figure 11: A graphical illustration of measured etch depths after silicon RIE etching.
Figure 12: Wafer profiles in different profilometry measurement phases after UV-exposure, SiO2
RIE and Si RIE and measured depths with profilometer (averages). From the measurement results, it can be seen that system pressure has the highest impact on the
etch rate. This can be seen from wafers 2 and 4 which has deeper etch depth and system pressure
140 mTorr than in wafers 1 and 3 and system pressure 60 mTorr. The flow rate of SF6 didn’t have
so high impact than pressure on measured etch depths after silicon RIE etching. The anisotropy,
selectivity and surface smoothness of etched wafers can be determined after characterization
which is done with SEM.
33
4.3 Wafer preparations before characterization
4.3.1 Dicing
In order to prepare the wafer for characterization, the first step was to dice the wafer. The dicing
was done by using the dicing saw machine Micro Ace 3, Series 2. Vertical and horizontal dicing
was done on all the 5 wafer samples. After taking out the wafers from the dicing machine they
were put into the oven for the duration of 5 -10 minutes in order to vacuum so that if there were
any particles present that would get removed.
4.3.2 Molding
After dicing the wafers, they were molded so that they can be used for grinding afterwards. For
the molding process, silicon spray with Epofix was used. The chips cut out from the wafer were
placed in holders and a concentration made by mixing (2x) Epofix resin with (15x) Epofix
hardener along with the silicon spray was poured into the holders. Then the holders were put for
vacuuming purposes in order to remove any remaining bubbles from it. It took around a day for
the chips to hardened into the holder after which they became ready for grinding.
4.3.3 Grinding
For grinding the chips, Struers LaboPol-21 grinding machine was used. LaboPol-21 can be used
for both manual grinding or automatic grinding. We did the manual grinding of the chips, at the
beginning grinding paper of 300 grits was placed on the roller of the machine and water was
sprayed on it to make it a little moist. Afterwards the chips were grinded slowly from the sides
initially and then from the center. The 300-grit paper was a rough one for grinding purposes but
it made the initial grinding process somewhat quicker. In order to get a smooth surface for the
chips the grinding paper was varied several times during the whole process. Different grinding
papers with various grits like 400, 600, 1000, 1200 and 1400 were used respectively to remove
the roughness from the grinded part of the chips.
4.3.4 Polishing
After the grinding of the wafer polishing was done. Struers Rotopol 22 was used for
polishing purposes, diamond particles of various sizes along with a lubricant were utilized during
the process. For the first run, the force was set at 30 N, lubricant and 9μm diamond particles (the
roughest polisher) were sprayed on the machine and the chips were placed on the machine for 5
minutes. Then for the second run, the force remained at 30 N while 6μm diamond particles
alongside the lubricant were sprayed on the machine and the chips were placed on the machine
for 5 minutes. For the third run, 3μm diamond particles with the lubricant were used while the
force and time were maintained constant at 30 N and 5 minutes respectively. For the final run,
1μm diamond particles (the smoothest polisher) were used for 5 minutes with 5N force to polish the chips.
34
4.4 Characterization results
4.4.1 Selected method and equipment
Characterization was done using a field emission scanning electron microscope JEOL JSM
6330F. Energy-dispersive X-ray spectroscopy (EDX) was also tried out but the results were not
good so they are not discussed here. Each wafer had five samples of cross section profile and four samples of sidewall profile. The
samples had a thin chromium layer on top of them and copper tape was used to earth them. The
voltage for SEM was 15 kV and the current was about 12 µA. Pictures of the setup and samples
below.
Figure 13. JEOL JSM 6330F scanning electron microscope.
35
Figure 14. Cross section samples (left) and sidewall samples (right).
4.4.2 Measurements
Cross section samples were analyzed by measuring top width, bottom width and depth of the
etching. These values were used to calculate lateral extension and anisotropy. Figure 15 shows an
example of a SEM image and explains said terms.
Figure 15. Example of a SEM image.
However, there is a problem with the depth measurements: it is practically impossible to
distinguish Si from SiO2 in SEM images. As explained in Chapter 4.1, SiO2 was also etched even
36
though the selectivity Si:SiO2 was quite high in silicon etching. This means that the depths
measured with SEM do not take into account on how much of the SiO2 was etched and what the
real etching depth is. Thus, depth results gained by profilometry in Chapter 4.1 will be used in
this analysis even though SEM results are quite close to profilometry values. The full SEM
measurements are located in Appendix I. Table 25 shows the average measurements for each
wafer (depths come from profilometry). Table 25. Measurements of the samples (average).
Pressure
(mTorr) SF6
flow
(sccm)
Width
top,
SEM
(µm)
Width
bottom
, SEM
(µm)
Depth
H,
profilo
metry
(µm)
Lateral
extension
V, SEM
(µm)
Anisotropy
1-V/H (µm) Etch rate,
profilome
try
(µm/min)
Wafer 1 60 20 149,86 141,10 8,641 4,378 0,493 0,346
Wafer 2 140 20 148,98 135,52 12,377 6,732 0,456 0,495
Wafer 3 60 40 146,16 138,98 7,205 3,592 0,501 0,288
Wafer 4 140 40 157,61 134,56 19,510 11,526 0,409 0,780
Etch rate behaves strangely. Higher pressure increases etch rate in both cases. However, with
lower pressure (60 mTorr), increasing SF6 flow decreases etch rate but with higher pressure (140
mTorr), increasing SF6 flow increases etch rate. Anisotropy seems to be slightly better with higher etch speeds. However, the calculated
anisotropy does not really tell much about the real anisotropy because the etch depth was quite
low and the bottom corners seemed to round similarly in every wafer. So basically, the deeper the
etching, the more anisotropic it would be with this formula. RIE is usually quite anisotropic so it
is fair to assume that with deeper etching this method should be quite anisotropic. There could be
a slope, meaning that the sidewall wouldn’t be exactly 90° but it is not possible to analyze this
better with our results. Figure 16 shows some SEM images of cross section samples.
37
Figure 16: Cross section samples.
4.4.3 Smoothness analysis
Smoothness can be analyzed from both cross section and sidewall profile samples. Close-up
images of cross section and sidewall samples are shown in Figures 16 and 17, respectively. Both
cross section and sidewall profile images show that the wafer 4 (combination of high SF6 flow
rate and high pressure) has really rough sidewalls. Wafer 3 seems to have the smoothest sidewalls. This wafer was etched with high SF6 flow rate
and low pressure. Also, the etch rate was slowest in this wafer. Wafer 1 seems to be the second
smoothest wafer according to sidewall profile images, and wafer 2 is the third smoothest wafer.
Sidewall profiles of wafer 2 and 4 have some bubbles which could’ve been caused by higher
pressure or higher etch rate.
38
Figure 16: Close-up of cross section samples.
Figure 17: Close-up of sidewall samples.
39
It looks like the etch rate correlates with the smoothness of the sidewall. The lower the etch rate,
the smoother the sidewall. Pressure correlates with both the etch rate and the smoothness so it is
difficult to say if pressure affects the smoothness directly or indirectly. More parameters would’ve
been needed to obtain better information on this issue. Table 26 summarizes the smoothness
analysis. Table 26. Summary of the smoothness analysis.
Pressure
(mTorr) SF6 flow
(sccm) Etch rate,
profilometry
(µm/min)
Smoothness (1 = smoothest, 4 = roughest)
Wafer 1 60 20 0,346 2
Wafer 2 140 20 0,495 3
Wafer 3 60 40 0,288 1
Wafer 4 140 40 0,780 4
5 Discussion and conclusions In this project, RIE was done on five wafers in order to see its impact on the roughness of the
material sidewalls. Parameters of different kind such as the gas flow rate, temperature, pressure
and power were used to characterize the etching results. In our wafer samples, among these
parameters, we kept the power and flow of oxygen constant while the flow rate of SF6 and pressure
were varied. The scanning electron microscope was used for characterization purposes, by
looking at the results it can be concluded that wafer 3 which had the highest SF6 flow rate with
low etch rate and low pressure had the smoothest surface at the sidewalls. On the contrary, wafer
4 which had high SF6 flow rate and high pressure had the roughest sidewalls. In short, it can be said that the increase in pressure generally increases the etch rate unless the rate
of flow of SF6 is taken into account as with high SF6 and high pressure, the etch rate increases
while for high SF6 and low pressure, the etch rate decreases. Overall, the project went pretty well according to the original project plan. In spring, we slightly
underestimated the amount of work in the theoretical part: it took more time to find out different
studies and publications which were suitable for our project. But with hard work and committed
project members we were able to manage to cope with this issue. During the project, two people
left from our group one of them being the project manager in the spring part of the project, which
resulted in increased workload and caused some changes in our project plan as well as project
roles. This issue was also listed as a project risk and fortunately for us it did not have a huge
impact in our project. Regular meetings played a key part in our project. We had meetings at least once a week with the
core team. We also communicated with instant messaging tools, email and cloud services. Thus,
40
communication was fast and it worked well. We also had meetings with our instructor
approximately 2-3 times a month. Clear agendas for the meetings helped us to remained motivated
also each member had their own tasks before each meeting. With regular meetings, the project
members were able to see the progress of the project. Meetings were also documented and project
memos were sent to cloud service so that every member was able to remember what we had done
in previous meetings. Some of our group members had no prior studies or experience related to this specific project. So,
at the beginning, it felt nearly impossible to finish this project but with the passage of time and
our willingness to learn new things, good attitude and hard work we achieved the project goals.
41
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Appendix
Appendix I. SEM measurements and calculations of cross section samples.
Wafer 1 Sample Width
top
(µm)
Width
bottom
(µm)
Depth
(µm) Lateral
extension
V (µm)
Anisotropy
1-V/H (µm)
O2: 14 sccm 1 150,8 144,38 9,240 3,210 0,650
CHF3: 17 sccm 2 148 140,7 9,600 3,650 0,620
SF6: 20 sccm 3 151,82 142,36 8,240 4,730 0,430
140 W 4 148,8 136,97 8,180 5,920 0,280
60 mTorr average 149,86 141,10 8,815 4,378 0,495
stdev 1,76 3,14 0,714 1,210 0,173
Wafer 2 1 146,5 133 11,870 6,750 0,430
O2: 14 sccm 2 150,79 139,38 11,630 5,710 0,510
CHF3: 17 sccm 3 150,14 135,86 11,800 7,140 0,390
SF6: 20 sccm 4 147,68 134,66 12,440 6,510 0,480
45
140 W 5 149,79 134,7 13,070 7,550 0,420
140 mTorr average 148,98 135,52 12,162 6,732 0,446
stdev 1,81 2,39 0,592 0,695 0,048
Wafer 3 1 148 141,17 7,290 3,420 0,530
O2: 14 sccm 2 145,69 138,98 7,160 3,360 0,530
CHF3: 17 sccm 3 144,54 136,38 6,980 4,080 0,420
SF6: 40 sccm 4 148,45 142,84 6,070 2,800 0,540
140 W 5 144,14 135,54 6,440 4,300 0,330
60 mTorr average 146,16 138,98 6,788 3,592 0,470
stdev 1,97 3,09 0,516 0,602 0,092
Wafer 4 1 159,63 134,64 20,070 12,500 0,380
O2: 14 2 158,9 135,11 18,870 11,900 0,370
46
CHF3: 17 3 156,63 133,91 18,530 11,360 0,390
SF6: 40 4 158,52 136,09 18,370 11,220 0,390
140 W 5 154,36 133,07 18,030 10,650 0,410
140 mTorr average 157,61 134,56 18,774 11,526 0,388
stdev 2,13 1,15 0,785 0,703 0,015