The Evolution of Silicon Wafer Cleaning Technology
Werner Kern*
Lam Research Corporation, Advanced Research Center, San Diego, California 92126
ABSTRACT
The purity of wafer surfaces is an essential requisite for the successful fabrication of VLSI and U L S I silicon circuits.
Wafer cleaning chemistry has remained essentially unchanged in the past 25 years and is based on hot alkaline and acidic
hydrogen peroxide solutions, a process k n o w n as "RCA Standard Clean." This is still the primary method used in the industry. What has changed is its implementation with optimized equipment: from simple immersion to centrifugal spraying, megasonic techniques, and enclosed system processing that allow simultaneous removal of both contaminant films
and particles. I m p r o v e m e n t s in wafer drying by use of isopropanol vapor or by "slow-pull" out of hot deionized water are
being investigated. Several alternative cleaning methods are also being tested, including choline solutions, chemical
vapor etching, and UV/ozone treatments. The evolution of silicon wafer cleaning processes and technology is traced and
reviewed from the 1950s to August 1989.
The importance of clean substrate surfaces in the fabrication of semiconductor microelectronic devices has been
recognized since the early days of the 1950s. As the requirements for increased device performance and reliability have become more stringent in the era of VLSI and
U L S I silicon circuit technology, techniques to avoid contamination and processes to generate very clean wafer surfaces have become critically important. Besides, over 50%
of yield losses in integrated circuit fabrication are generally accepted to be due to microcontamination. Trace ibmpurities, such as sodium ions, metals, and particles, are especially detrimental if present on semiconductor surfaces
during high-temperature processing (thermal oxidation,
diffusion, epitaxial growth) because they may spread and
diffuse into the semiconductor interior. Impurities must
also be removed from surfaces before and/or after lower
temperature steps, such as chemical vapor deposition,
dopant implanting, and plasma reactions. Postcleaning
after photoresist stripping is necessary for every mask
level throughout the production process.
Many wafer cleaning techniques have been tested and
several are being used. The generally most successful approach for silicon wafers without metallization uses wetchemical treatments based on hydrogen peroxide chemistry. This process has remained essentially unchanged
during the past 25 years, but important advances have
been made in its technical implementation. The evolution
of the cleaning technology for premetallized silicon wafers
from its beginning to the present time will be traced in this
paper.
Type, Origin, and Effects of Contaminants
Impurities on silicon wafer surfaces occur in essentially
three forms: (i) contaminant films, (ii) discrete particles,
and (iii) adsorbed gases that are of little practical consequence in wafer processing. Surface contaminant films
and particles can be classified as molecular compounds,
ionic materials, and atomic species. Molecular compounds
are mostly particles or films of condensed organic vapors
from lubricants, greases, photoresist, solvent residues,
components from plastic storage containers, and metal oxides or hydroxides. Ionic materials comprise cations and
anions, mostly from inorganic compounds that may be
physically adsorbed or chemically bonded (chemisorbed),
such as sodium ions, fluoride ions, and chlorine ions.
Atomic or elemental species comprise metals, such as gold
and copper, that may be electrochemically plated out on
the silicon surface from HF-containing solutions, or they
ma y consist of silicon particles or metal debris from
equipment.
The sources of impurities are manifold. In the case of
particles, which can be detected and measured m u c h more
easily than contaminant films, the major sources are equipment, chemicals, factory personnel, and production processes. For example, mechanical equipment, process operators, furnace tubes, film deposition systems, gas piping,
* Electrochemical Society Active Member.
and liquid containers are especially serious sources,
whereas materials, liquid and gaseous chemicals, and ambient air tend to cause less particle contamination; but all
contribute significantly to the generation of contaminant
films. Static charge built up on wafers and carriers is a
powerful mechanism of particle deposition, but is often
overlooked and not properly dealt with.
Molecular contaminant films on wafer surfaces can
mask effective cleaning or rinsing, cause poor adhesion of
deposited layers, and lead to harmful decomposition products. For example, organic films, if heated to high temperatures in a nonoxidizing atmosphere, can carbonize and
form silicon carbide that can nucleate polycrystalline regions in an epitaxial deposit. Ionic films and metals cause
a host of problems in semiconductor devices. During hightemperature processing or on application of an electric
field they may diffuse into the bulk of the semiconductor
structure or spread on the surface, leading to electrical defects, device degradation, and yield losses. For example,
highly mobile alkali ions may cause drift currents and unstable surface potential, shifts in threshold and flatband
voltages, surface current leakage, and may lower the oxide
breakdown field of thermally grown layers. In the growth
of epitaxial silicon layers, sufficiently high concentrations
of ions can give rise to twining dislocations, stacking
faults, and other crystal defects. Atomic metals, especially
the heavy metals, can affect minority-carrier lifetime, surface conduction, electrical device stability, and lead to
structural defects in epitaxial layers. Particles may cause
blocking in photolithography and etching or rinsing, and
lead to shorts if they are conductive and located adjacent
to conductor lines. They are considered potential killer defects if their size exceeds one tenth of the linewidth. Particles that are present during film growth or deposition may
lead to pinholes, material voids, cracks, and the generation
of defects noted above, depending on their chemical composition. Additional information on the nature, origin, detection, and effects of contaminants is available from selected papers and reviews (1-13).
Early Cleaning Procedures
During the early stages of silicon wafer processing until
about 1970, one used organic solvent extraction, boiling nitric acid, aqua regia, concentrated hydrofluoric acid, and
hot acid mixtures as cleaning chemicals. Mixtures of sulfuric acid-chromic acid led to chromium contamination
and caused ecological problems of disposal. Mixtures of
sulfuric acid and hydrogen peroxide caused sulfur contamination. Aqueous solutions containing hydrogen peroxide had long been used for cleaning electron tube components (14, 15) but not for semiconductors. In general,
impurity levels and particles in process chemicals were
high and in themselves tended to lead to surface contamination. Particulate impurities were removed by ultrasonic
treatment in detergent solutions or by brush scrubbing.
The first caused frequent wafer breakage and the second
often deposited more debris from the bristles than it rem o v ed from the wafer surfaces.
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Cleaning Processes Based on Hydrogen Peroxide
Solutions
Cleaning chemistry.--The first systematically developed
cleaning process for bare or oxidized silicon wafers was
based on a two-step oxidizing and complexing treatment
with hydrogen peroxide solutions: (i) an alkaline mixture
at high pH followed by (ii) an acidic mixture at low pH (1).
The choice of chemicals was based on reaction chemistry,
oxidation potentials, reagent purity, reagent volatility,
safety, and economy. The process was developed at RCA,
introduced to device production in 1965, and published in
1970 (1).
In the first treatment step the wafers are exposed to a hot
mixture of water-diluted hydrogen peroxide and ammonium hydroxide. This procedure was designed to remove
organic surface films by oxidative breakdown and dissolution to expose the silicon or oxide surface for concurrent
or subsequent decontamination reactions. Group IB and
IIB metals and several other metals, including gold, silver,
copper, nickel, cadmium, zinc, cobalt, and chromium, are
dissolved and removed by the complexing effectiveness of
a m m o n i u m hydroxide; copper, for example, forms the
Cu(NH3)4 § amino-complex.
The second treatment step exposes the rinsed wafer to a
hot mixture of water-diluted hydrogen peroxide and hydrochloric acid. This procedure was designed to remove
alkali ions, and cations such as A1§ Fe § and Mg § that
form NH4OH-insoluble hydroxides in basic solutions. This
second step also eliminates metallic contaminants
that were not entirely removed by the first treatment, such
as gold. Electrochemical displacement replating of heavy
metals from the solution is prevented by formation of soluble complexes with the dissolved metal ions.
Solution composition, process conditions, and effectiveness.--The solution compositions are based on ultrafiltered deionized water, electronic grade NH4OH (29 weight
percent (w/o) as NH3), electronic-grade HC1 (37 w/o), and
high-purity "unstabilized" H202 (30%). The hydrogen peroxide must be low in aluminum and stabilizer additives
(sodium phosphate, sodium stannate, or amino derivatives) to prevent wafer recontamination. The usual volume
ratios for the solution used in the first treatment step are 5
H20:l H~O2:l NH4OH; the mixture is known as "RCA
standard clean 1 or SC-I." The usual volume ratios for the
second solution are 6 H20:1 H2Q:I HC1, "RCA standard
clean 2, or SC-2." Treatments by the original immersion
technique are typically 10 min at 75~176 in each solution.
Higher temperatures must be avoided to minimize excessive thermal decomposition of the hydrogen peroxide. Intermediate and final rinses in ultrafiltered deionized water
are used.
The effectiveness of the process was demonstrated by
sensitive radioactive tracer measurements with several radionuclides (1, 16) and by capacitance-voltage bias temperature measurements of MOS capcitors (1). H202 solutions are unstable at elevated temperature, especially at
high pH, rapidly decomposing to H20 and 02. The processing temperature should therefore be kept at 75~176 to sufficiently activate the mixtures without causing excessively
fast decomposition.
Optional processing steps.--A preliminary clean-up
treatment with a hot H2SO4-H202 mixture (2:1 vol) can be
used advantageously for grossly contaminated wafers having visible residues, such as photoresist layers. Another
step, not noted in the original paper (1), concerns an etch in
H F solution for bare silicon wafers. Since the hydrous
oxide film from the SC-1 treatment may trap trace impurities, its removal before the SC-2 step should be beneficial.
A 15s immersion in 1% HF-H20 solution is sufficient to remove this film, as evidenced by the change from the hydrophilic oxidized surface to hydrophobic after stripping.
However, unless high-purity and point-of-use ultrafiltered
and particle-free HF solution is used under controlled conditions, more harm than good can result. A silicon surface
that was exposed to HF is highly reactive and immediately
attracts particles and organic contaminants from solutions, DI water, and the ambient air. Contrary to SC-1, the
subsequent SC-2 solution, which has no surfactant activity, will not eliminate these contaminants. It may therefore
be preferable to rely on the dissolution action of SC-1 that
dissolves and regrows the hydrated oxide layer at about
the same rate. If the preclean is used, then the 1% H F step
prior to SC-1 is acceptable since SC-1 will remove the contaminants. Exposure of bare silicon wafer to H F after SC-2
should not be done since it would destroy the passivated
surface resulting from SC-2 and cause recontamination.
Immersion technique.--The original RCA cleaning process was based on a simple immersion technique. Several
different and improved techniques have been introduced
over the years, as will be discussed. The immersion procedure is done in vessels of fused silica to prevent leaching of
aluminum, boron, and alkalis if Pyrex glass is used. A
batch of wafers is immersed in the SC-1 or SC-2 solution
under the prescribed conditions. The reaction is terminated by overflow quenching with cold DI water before
the wafers are transferred to a flow rinse system with ultrafiltered DI water, followed by spin drying in a wafer centrifuge. Several types of refined wet bench immersion systems for automated processing are now available for
large-scale production (17-19).
Centrifugal spray cleaning.--In 1975, F S I Corporation
introduced the first centrifugal spray cleaning machine
specifically designed for automatic operation with corrosive chemicals. The wafers rotate past a stationary spray
column. Filtered acids and reagent solutions, including
hot SC-1, SC-2, and DI water, are pressure-fed into a mixing manifold and then directed as a dispersed spray onto
the spinning wafers. The spin-rinsed wafers are dried by
high-speed spinning in heated nitrogen. A reduced volume
of freshly mixed reagents is used and the process is faster
than by immersion. The chemical cleaning efficiency, according to FSI, is comparable with that of immersion, but
particles are removed more efficiently. Improved versions
of this system (20) and other types of spray processing machines (17-19) are widely used but tend to require considerable maintenance.
Megasonic cleaning.--The original objective of the RCA
cleaning process was the removal of contaminant films
rather than particles. To c o m p l e m e n t this technique, the
megasonic particle removal system was developed at RCA
and first described in 1979 (21). A highly effective noncontact scrubbing action on both front and back side surfaces
of the wafers is achieved by ultrahigh-frequency sonic
energy while the wafers are submerged in the cleaning solution. The sonic waves of 850-900 kHz are generated by an
array of piezoelectric transducers. Particles ranging in size
from several micrometers down to about 0.3 ~m can be efficiently removed with input power densities of 2-5 W/cm 2.
For comparison, ultrasonic systems operate typically at
20-80 kHz and require power densities of up to 50 times
that of the megasonic system but are m u c h less effective
for removing very small particles. Megasonic cleaning
made it possible to remove simultaneously contaminant
films and particles in one operation by combining the peroxide treatments with megasonics. The system allows removal of particles, organic contaminant films, and lightly
adsorbed contaminants with diluted SC-1 solution at the
ambient bath temperature of only 35~176 Chemisorbed
inorganics generally require higher temperatures (about
70~ for complete desorption with SC-1 and SC-2, but no
quantitative data are available as yet. A detailed paper on
megasonic wafer cleaning was published in 1985 (22). Improved megasonic systems built under license from RCA
have become available in the past few years from Verteq,
Semiconductor Technology, and Estek.
Closed system chemical cleaning.--A system termed
Full-Flow TM, developed in 1986 by CFM Technologies, Incorporated, is based on keeping the wafers stationary and
enclosed in the system during the entire cleaning, rinsing,
and drying process (23). The vessel containing the wafers
is hydraulically controlled to remain filled with hot or cold
process fluids, including SC-1 and SC-2, that flow sequentially and continuously over stationary wafers loaded in
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cassettes. The repeated crossing through the gas/liquid
phase boundaries in the immersion techniques is thereby
eliminated. The system thus avoids recontamination problems encountered when wafers are pulled out from a
liquid.
Chronological Literature Survey
Beginning in 1972, independent investigators examined
and verified by various analytical methods the effectiveness of the RCA cleaning method published in 1970 (1).
This section chronologically reviews references on silicon
wafer cleaning pertaining specifically to hydrogen peroxide solutions, up to mid-1989.
In 1972 Henderson published results on the evaluation
of SC-1/SC-2 cleaning, using high-energy electron diffraction and Auger electron spectroscopy as analytical methods (24). He concluded that the process is well-suited for
wafer cleaning prior to high-temperature treatments, as
long as quartz ware is used for processing, as specified by
us (1). A n additional final etch in HF solution after SC-1/
SC-2 caused carbon contamination and surface roughening during vacuum heating at ll00~ due to loss of the
protective 1.5 n m thick C-free oxide film remaining after
SC-2. Meek et al. (1973) investigated the removal of inorganic contaminants, including Cu and heavy metals, from
silica-sol polished wafers by several reagent solutions (25).
Using Rutherford backscattering, they qoncluded that SC1/SC-2 preoxidation cleaning removes all elements heavier
than CI. Sulfur and chlorine remained after either SC-1,
SC-2, or other cleaning procedures at 1013/cm2. SC-1/SC-2
cleaning eliminated Ca and Cu much more reliably than
did HF-HNO3. Amick (1976) reported the presence of C1 on
Si after SC-2 and S after H2SO4-H202; he used spark source
mass spectrometric analysis (26). In 1976 Kern and
Deckert published a brief review of surface contamination
and semiconductor cleaning as part of a book chapter on
etching (3). Murarka et al. (1977) studied methods for oxidizing Si without generating stacking faults and concluded that SC-1/SC-2 prior to oxidation is essential for
this purpose (27). Gluck (1978) discussed removal of gold
from Si by a variety of solutions. The desorption efficiency
of SC-1 was more effective than that for SC-2, but the reco m m e n d e d sequential treatment of SC-1 followed by SC-2
was found to be the most effective method at high gold
surface concentrations (10Wcm2 range) (28). Peters and
Deckert (1979) investigated photoresist stripping by solvents, chemical agents, and plasma ashing. The SC-1 procedure was the only acceptable technique by which the
residues could be removed completely (29). B u r k m a n
(1981) reported on desorption of gold with several reagent
solutions by centrifugal spraying. SC-1 type solution was
m u c h more effective than H2SO4-H202, while a SC-2 type
alone showed poor efficiency (20).
Phillips et al. (1983) applied SIMS (secondm~ ion mass
spectroscopy) to determine the relative quantities of contaminants on Si. Cleaned wafers were purposely contaminated with gross quantities of numerous inorganic materials and then cleaned by immersion or spray techniques
with various aggressive reagents including aqua regia, hot
fuming HNO~, and H2SO4-H202. The lowest residual concentrations for most impurity elements were obtained by
spray cleaning with H2SO4-H202 followed by the SC-1/HF/
SC-2 type cleaning sequence (30). Goodman et al. (1983)
demonstrated by minority-carrier diffusion-length measurements the effectiveness of SC-1/SC-2 for desorbing
trace metals on Si (31). The author (1983) published a review of the subject on the occasion of the Citation Classic
declaration of the original 1970-paper (32). In 1983 Watanabe et al. (33) reported dissolution rates of SiO2 and Si3N~
films in SC-1. The rate of thermally grown SiO2 in SC-1
during 20 m i n at 80~ was a constant 0.4 nm/min, a significant rate for structures with thin oxide layers. The etch
rate of CVD Si3N4 was 0.2 n m / m i n u n d e r the same conditions. Measurements by the author in 1981 (and published
in 1984), however, indicated much lower oxide dissolution
rates u n d e r nearly identical conditions (34). Film thicknesses were measured by ellipsometry after each of four
consecutive treatments in fresh 5:1:1 SC-1 at 85~ and totaled only 7.0 rim/80 min, or 0.09 nm/min. Under the same
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conditions, 6:1:1 SC-2 showed no loss. Similar results averaging 0.13 n m / m i n were obtained with thermal SiO2 films
grown on lightly or heavily doped Si. Wafers from the
same sets were used to determine the etch rates of exposed
Si in SC-1 solutions with decreasingly lower H2Oz content.
No etching or attack of Si occurred until the H202 was reduced by more than 75% (34).
Bansal (1984, 1985) reported extensive results in particle
removal by spray cleaning from Si wafers with SC-1/SC-2,
H2SO4-H202, and HF solution of various purity grades. He
found the RCA cleaning solutions to be the most effective
(35, 36). Shwartzman et al. (1985) described simultaneous
removal of particles and contaminant films by megasonic
cleaning with SC-1 solutions (22). Ishizaka and Shiraki
(1986) showed that atomically clean Si surfaces for MBE
can be prepared below 800~ in UHV by thermal desorption of a thin (0.5-0.8 nm), passivating oxide layer that
protects from C contamination (37). It is formed in a series
of wet oxidation (HNO3, SC-1) and HF-stripping steps, terminating with an SC-2 type treatment. Wong and Klepner
(1986) used XPS analysis to examine Si after wet chemical
treatments. RCA cleaning without buffered HF stripping
resulted in about 30% of the Si atoms in the top 1.0 n m
being oxidized, whereas with a final BHF step less than
one monolayer of suboxide coverage resulted (38). Grundher and Jacob (1986) conducted extensive studies of Si surfaces after treatment with SC-1/SC-2 or 5% HF solutions,
using x-ray photoelectron and high-resolution electron
energy loss spectroscopy. Oxidizing solutions produced
hydrophilic surfaces, whereas HF solution led to hydrophobic surfaces consisting mainly of Si-H with some
Si-CH= and Si-F (39). I n 1986 Becker et al. (40) reported on
decontamination by different reagent sequences. SIMS
analysis was used to test for the removal of Na, K, Ca, Mg,
Cr, Cu, A1, and particle impurities. The best cleaning sequence for metallics was H2SO4-H202/SC-1/HF/SC-2. Reversing the order of SC-1 and HF was most effective for
particle removal and slightly less so for metal ions.
Kawado et al. (1986) found by SIMS that A1 on Si wafers
originated from impure H202 used in SC-2. Very high concentrations resulted if Pyrex vessels were used in the processing instead of fused quartz (41). I n 1986 McGillivray
et al. (42) investigated effects of reagent contaminants on
MOS capacitors. Low field breakdown was more prevalent
if preoxidation cleaning with SC-2 was terminated with
HF solution instead of omitting it. No other significant differences in electrical properties resulted from these two
treatments.
Lampert (1987) examined growth and properties of
oxide films on Si in various aqueous solutions, including
SC-1 and SC-2 (43). Gould and Irene (1987) studied the influence of preoxidation cleaning on Si oxidation kinetics
(44). They found significant rate variations depending on
treatment (SC-1/SC-2/HF, SC-1, SC-2, HF, no clean).
Ruzyllo (1987) reported on similar experiments and found
that various preoxidation cleans seem to affect structure
and/or composition of the subsequently grown oxide
rather than the reactivity of the Si surface (45). Slusser and
MacDowell (1987) found that sub-ppm levels of A1 in H202
used for SC-1/SC-2 causes a substantial shift (up to 0.2V) in
the flatband voltage of a dual dielectric. A l u m i n u m concentrates on the wafer surface, and basic media such as
SC-1, lead to 5 times higher levels than acid (SC-2) solutions (10). I n 1987 Kern and Schnable reviewed wafer
cleaning in a new chapter on wet etching (11). Probst et aI.
(1988) stated that for achieving predictable diffusion from
implanted doped poly-Si into single-crystal Si, an SC-1/
SC-2 treatment of the substrate prior to poly-Si deposition
is imperative (46). Khilnani (1988) discussed various
aspects of semiconductor cleaning, including the RCA
process (12). Peterson (1988) showed that the sequencing
of cleaning solutions (H2SO4-H202, SC-1, SC-2, HF) can
have dramatic effects on particles levels (47). In 1989
Morota et al. (48) reported on the contamination of SC-1/
SC-2 cleaned wafers by Na, K, A1, Cr, Fe, Ni, and Cu from
solutions, showing that the absence or presence of an SiO~
layer on the Si surface strongly affects adsorption. Desorption of A1 and Fe was most effective with ttF-HzO, and that
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of Cu and Cr with SC-2. The same authors (49) postulated
that metals of high enthalpy of oxide formation adsorb on
the oxidized Si surface by oxide formation, whereas metals of low ionization tendency deposit electrochemically
on the bare Si. Gould and Irene (1989) studied the etching
of native SiOx and Si in NH4OH-H20, BHF, and SC-1 by ellipsometry. Severe Si surface roughness resulted from
NH4OH, less with BHF, and none with SC-1 (50). Ohmi
et al. (1989) compared particle removal efficiency of several cleaning solutions. They found that 5:1:1 SC-1 efficiently removes particles larger than 0.5 ~tm, but increases
those smaller than 0.5 ~m ("haze") unless the NH4OH ratio
was decreased to one half or less, in which case both types
of particles were reduced efficiently. However, no processing conditions and effects of low-NH4OH SC-1 on removal
of chemical contaminant films were mentioned (51).
Menon et al. (1989) evaluated effects of solution chemistry
(5:1:1, SC-1, DI water) and particle composition on megasonic cleaning efficiency at various power levels. They
concluded that cleaning efficiency depends on several factors and that magasonics can provide wafer cleanliness
levels not previously attainable (52).
Alternative Cleaning Techniques
GeneraL--Many techniques for cleaning silicon wafers
have been tried over the years with various degrees of success. Some techniques are useful only for specific applications or may introduce undesirable side effects. For example, glow discharge techniques (53) such as plasma
etching, effectively strip photoresist films but leave inorganic contaminants and metals behind. Various types of
sputter-etching (53) can cause surface damage. Some techniques remain restricted to certain applications, such as
plasma treatments for preparing small-geometry devices
for metallization (54), or wet-chemical etching of the silicon to remove entire surface layers by etch dissolution
(3, 11). The following few techniques have been found viable and, in some cases, can be a desirable addition or alternative to the processes based on hydrogen peroxide solutions.
Brush scrubbing, fluid jet, and ultrasonic techniques.The removal of large particles (e.g., after sawing and
lapping operations) has been accomplished since the early
days with wafer scrubbing machines that dislodge particles hydrodynamically with brushes made of a hydrophilic
material (such as nylon) while DI water or isopropyl alcohol is applied to the surface (55). A thin layer of fluid must
be retained between the brush and the wafers by careful
mechanical adjustment to prevent surface scratching (22).
While many contradictory claims have been made (56), if
properly maintained, brush scrubbing can be very effective for removing particles larger than 1 ~m from planar
and preferably hydrophilic wafer surfaces.
High-pressure fluid jet cleaning consists of a highvelocity jet of liquid sweeping over the surface at pressures of up to 4000 psi (55, 56). The liquid can be DI water
or organic solvents. The shear forces effectively dislodge
submicron particles and penetrate into dense topography,
but damage to the wafer can result with improperly adjusted pressure (18).
Ultrasonic techniques use sonic energy of 20 kHz and
above to dislodge particles. High-intensity sound waves
generate pressure fluctuations that result in cavitation
bubbles which upon collapsing, release enough energy to
dislodge and disperse particles but can also lead to wafer
damage (56). Menon et al. have recently investigated various cleaning liquids for removing particles from wafers by
ultrasonic and spray jet techniques (57). DI water was best
for removing polymeric particles, while ethanol-acetone
(1:1) was best (better than Freons) for inorganic particles.
Cleaning efficiency decreased with decreasing particle
size. A unique acoustical cleaning system utilizing 20 kHz
frequency and only DI water as m e d i u m was introduced
by Estek in 1986 (18) but has been abandoned.
Choline cleaning.--In contrast to the mechanical techniques for particle removal discussed in the previous section, choline cleaning is a chemical treatment that removes
particles and some contaminant films but at the same time
appears to add certain contaminants to the surface. Choline, which is trimethyl-2-hydroxyethyl a m m o n i u m hydroxide, was first proposed by Asano et al. in 1976 (58) as a
replacement for inorganic bases for etching and cleaning.
It is a strong and corrosive base without alkali elements
and etches silicon like other bases. A formulation of the
chemical is available from Mallinckrodt under the
tradename "Summa-Clean SC-15 M," which is a dilute
choline solution containing a surfactant and methanol.
Etching of Si can be prevented by adding H202 as an oxidant (59). There is very little published information on this
subject, most data being contained in proprietary technical reports with contradictory results. Poly-flow engineering manufactures an automatic dual-cassette spray
machine that uses a warm choline-H202-H20 mixture and a
DI water spray rinse (18). In some procedures the mixture
replaces only SC-1 in the RCA cleaning procedure. In 1989
Kaos discussed oxide defect densities as a function of various preoxidation cleans including choline-H202-H20,
HF-H20, RCA cleans, and UV-ozone (60).
UV-ozone and other dry-cleaning techniques.--Irradiating a surface with short-wavelength UV from a mercury
quartz lamp in the presence of oxygen is a powerful technique for removing many contaminants. Oxygen absorbs
185 nm radiation forming very active ozone and atomic oxygen (61). The technique is most suitable for oxidative removal of adsorbed organics, but is generally not effective
for most inorganics or metals. Therefore, its use in the past
has been limited, in general, to special applications, such
as GaAs wafer cleaning. Improvements in oxide qualities
have been attained by applying the technique after SC-1/
SC-2/HF-H20, immediately before oxidation (62). Ruzyllo
et al. (1989) have shown that UV-O2 cleaning can replace
SC-1 for removing organics (63), and Kaos reported improvements in properties of thermal oxide films (60).
Hoenig (1988) investigated the use of dry ice snow for removing particles from wafers (64). Clean, liquid CO2 from a
tank is allowed to expand to form dry ice snow, which is
blown across the surface. The sliding snow is quite effective for mechanically removing particles. Particle detachment by electrostatic techniques has been investigated but
found to be impractical (12). In 1987 F S I Corporation introduced a processing system for anhydrous HF gas phase
etching of oxide and silicate films at room temperature
(65). Applications to device processing were published in
1988 (66, 67). The contamination problems inherent with
HF-H20 solutions were avoided and in combination with
the UV-ozone technique constitutes part of an ultrapure,
integrated dry cleaning process that can be carried out entirely in the gas phase and may replace conventional wet
techniques. Removal of metallic impurities could be accomplished by use of a remote microwave plasma (68), by
chlorine radical techniques (67) or by photoinduced desorption in reactant gases (69). These new processes being
developed are all designed to remove contaminants at low
temperatures as volatile compounds without damaging
the surface.
Wafer Rinsingand Drying
The last steps in wafer cleaning are rinsing and drying;
both are extremely critical because clean wafers become
recontaminated very easily if not processed properly.
Rinsing after wet cleaning is done with flowing highpurity and ultrafiltered high-resistivity DI water, usually at
room temperature (34). Megasonic rinsing is advantageous
(52). Centrifugal spray rinsing (20) and rinsing in a closed
system (23) have the advantage that the wafers are not rem o v ed between cleaning, rinsing, and drying. Wafer drying after rinsing must be done by physical removal of the
water rather than by allowing it to evaporate. Spin drying
accomplishes this and has been the most widely used technique. Hot forced-air drying is a preferred technique with
less chance for particle recontamination (21, 22). Capillary
drying is based on capillary action and surface tension to
remove the water. Individual wafers are pulled out of DI
water at 80~176 less than 1% of the water remains and
evaporates, leaving a particle-free surface (70). In solvent
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vapor drying wet wafers are moved into the hot vapor of a
high-purity solvent, usually IPA (isopropyl alcohol), which
displaces the water. The wafers dry quickly and are particle-free when the cassette is withdrawn above the hot
vapor zone. Commercial drying systems for IPA and for
nonflammable solvent mixtures are available (23, 70). The
purity of the solvent is extremely important, and the water
content during processing must be closely controlled,
preferably by continuous recycling (51, 70).
Conclusion
Processes and techniques for cleaning, rinsing, and drying bare and oxide-coated silicon wafers have been reviewed from the 1950s to the present. Wet chemical
cleaning based on hydrogen peroxide solutions and implemented by several techniques is still the main process
used in industry. However, new wafer surface preparation
technologies based on dry processing in the gas or vapor
phase are being developed that promise superior results.
A great deal of research activity is taking place in this
important area of technology, as evidenced by the scheduled presentation of over 40 papers (not referenced herein)
at the First International Symposium on Wafer Cleaning
Technology in Semiconductor Device Manufacturing, October 16-18, 1989, at the Electrochemical Society Fall
Meeting.
Manuscript submitted Sept. 5, 1989; revised manuscript
received Dec. 21, 1989. This was Paper 381 presented at fhe
Hollywood, FL, Meeting of the Society, Oct. 16-18, 1989.
Lain Research Corporation assisted in meeting the publication costs of this article.
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Growth and Properties of LPCVD Titanium Nitride as a
Diffusion Barrier for Silicon Device Technology
A. Sherman*
Varian Associates, Incorporated, Varian Research Center, Palo Alto, California 94303
ABSTRACT
Chemical vapor deposition has been used to deposit titanium nitride (TIN) on silicon wafers at low pressures in a coldwall single-wafer reactor. Experiments are reported for pressures in the range of 100-300 mtorr and temperatures between
450~176
with titanium tetrachloride and a m m o n ia as reactants. Both hydrogen and nitrogen are evaluated as diluents.
Deposition rates as high as 1000/~/min have been achieved. The chemical nature of the films are evaluated by Auger and
RBS techniques, while the morphology is depicted by SEM. For the most part, the films are stoichiometric and contain
small quantities of oxygen, chlorine, and hydrogen. Film resistivities as low as 50 ~ll-cm are reported. Behavior of the TiN
film as a diffusion barrier between silicon (boron doped) and aluminum, at annealing temperatures up to 550~ is evaluated by measurements of contact resistance and diode leakage.
Coating of various metals with titanium nitride has been
possible since the discovery in the 1920s of a chemical
vapor deposition technique using electrically heated wires
exposed to TIC14 + N2 + H2 gas mixtures (1, 2). In spite of
the high temperatures required (> 1000~ commercial applications for jewelry coating (3) (gold color) and tool
coating (4) (wear resistance) have seen considerable success. With the advent of reactive physical vapor deposition
techniques (5-8), where a discharge in nitrogen is created
with titanium atoms either evaporated or sputtered from
one electrode, low temperature depositions (<500~
became possible and applications of TiN coatings have become even more widespread. Other applications have
been as a transparent heat mirror for architectural windows (9, 10), and as a high temperature diffusion barrier
for silicon solar cells (11, 12).
Of particular interest, in the present paper, is the application of thin TiN films to silicon device technology. Because of the concern about exposure of circuits to high
temperature processes, barrier films deposited by physical
vapor techniques such as low temperature reactive sputtering (13-22) have been employed. However, as integrated
circuit feature sizes shrink to submieron dimensions, the
ability of physical techniques to uniformly coat high
aspect ratio vias has become a concern. Accordingly, there
has been an interest in developing a low temperature CVD
process for deposition of thin films of TiN. One approach
has been to explore plasma-enhanced CVD (PECVD)
using TIC14 plus either nitrogen (23-26) or ammonia (27, 28).
Another has been to investigate the low temperature thermal CVD process possible using TIC14 + NH3, where depositions are possible at temperatures as low as 450~ One
recent investigation has focused on a low pressure CVD
process (LPCVD) where many wafers are coated at one
time in a hot wall tube reactor (29). Two others describe a
LPCVD process in a cold-wall single-wafer reactor (30, 31).
In this paper we elaborate on the latter approach.
Experimental
The titanium nitride depositions were carried out in a
single-wafer cold-wall experimental reactor shown schematically in Fig. 1 (30). The chamber was stainless steel
and enclosed a water and air-cooled lamp assembly used
to heat the wafer. A single 10 kW tungsten halogen lamp
* Electrochemical Society Active Member.
was employed that can heat a 4 in. wafer to 700~ rapidly.
A load lock was used to maintain an oxygen and water vapor-free deposition environment.
Reactive gases were introduced through a showerhead
gas distributor several inches above the wafer. The TiCl4
and NH3 were introduced through two separate lines and
m i x e d for the first time in the shower head. As long as
these two gases are m i x ed close to the hot wafer on which
the deposit is to be made, the formation of NH4C1 can be
avoided as has been demonstrated in another experiment
similar to this one (31).
Before beginning TIC14 or NH3 flows, a nitrogen flow was
established in the TIC14 line downstream of the TIC14 bottle. Next the TIC14 flow was initiated, and after it was
stabilized then the NH3 flow was introduced. This procedure kept TIC14 and NH3 from mixing in the TIC14 line and
causing solid deposits there.
All of the gases were introduced through mass flow controllers (MFCs), including the TIC14 vapor which was obtained by heating TIC14 liquid to 40~ The TiCl4 line was
heated to 50~ to prevent any condensation of this vapor.
Since the pressure of the TIC14 vapor at 40~ was only 50
torr, we calibrated our Unit MFC (UFC 1100) by measuring
the time it took for a specified nitrogen mass flow (supplied at 40 torr) to increase the pressure in our chamber
from 100 to 200 mtorr. We then repeated this m easu r em e nt
w h e n the nitrogen was supplied at 10 psi. By this method
GAS BOX
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ARM
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Fig. 1. Schematic of CVD reactor system
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