(Hee-Young Shin)
12
(Tae-Ho Kim)
1
(Jun-Woo Park)
3
(Hyun-Chul Sohn)
1*
Copyright © 2019 The Korean Institute of Metals and Materials
Key words(Korean)
DC magnetron sputtering, flux distribution, step coverage, long throw sputter, simulation
1. INTRODUCTION
In recent semiconductor devices, the through-silicon-via (TSV) technology is introduced
to overcome the restriction by wire connection and the signal delay as the number
of cells increases [1,2]. During the TSV processes, chips are connected by via hole of high aspect ratio.
Then, barrier layer and seed layer are formed using the physical vapor deposition
(PVD) method in via holes and then Cu films are deposited to fill via holes [3].
The conventional sputtering has a wider angular distribution of arrival atoms that
induces a pinch-off of the barrier and the seed layers at the top, producing a nonconformal
film profile with the poor coverage at the bottom and the side of vias [4,5]. To obtain a conformal film in the high aspect ratio via structure, the angular
flux of the sputtered Cu toward to the bottom of the deep via needs to be enhanced
to produce a relatively thick film at the contact bottom [6]. As the distance between target and substrate increases, the range of the angle
of the atomic flux that is reaching the substrate is decreased naturally such that
the deposition can be added to the bottom of the structure [7,8]. The angular distribution of atoms sputtered from the target is significant effect
on the step coverage and the deposition profile [9] and the understanding of effects of sputtering process parameters on the angular
distribution of sputtered atoms is important to control the deposition profile of
films on deep vias [10-12]. LTS method is applied to improve the step coverage at via bottoms by enhancing
the atomic flux toward a contact bottom. In the LTS method, atoms with large deviation
angles are separated from the wafer and only a narrow angle of flux reaches the substrate.
In this study, the angular distribution of sputtered Cu atoms for LTS are investigated
by the comparison of the deposition profile measured in overhang structures with the
simulated deposition profile from various angular fluxes with the shape of cosine
law. And effects of the sputtering parameters such as the substrate RF power, the
operation pressure, and the target DC power on the angular distribution of Cu are
investigated. Then, the deposition profile of sputtered Cu films on the deep via of
aspect ration 10 is simulated based on the optimized sputtering conditions and compared
with the measured Cu film profile to check the validity of the optimized atomic flux.
2. EXPERIMENTAL PROCEDURES
Bulb-shaped contact structures of low aspect ration of < 2 with overhang are fabricated
to extract angular distributions of sputtered Cu and to investigate the effect of
the sputtering process conditions on deposition profile of Cu films. To make contact
structure with overhang, SiO2 of 2 μm is deposited using low pressure chemical vapor deposition (LP-CVD) using
tetraethyl orthosilicate (TEOS) and then, the silicon nitride film of 0.4μm is deposited
using LP-CVD. After patterning the 2μm hole using photolithography, the silicon nitride
is dry etched with RIE to form holes, then SiO2 is etched by the wet etchant of 0.5% HF solution to form overhang structure. Cu films
are deposited on the overhang structure by the AP systems’ LTS sputter system with
the sample-target distance of 380 mm. Then the profile and step coverage are measured
using cross-sectional transmission electron microscopy (TEM) of JEOL JEM-2100. Simulation
of the deposition profiles is conducted using the Athena program, which can be applied
to PVD deposition. For simulation, the hemispherical model in the Athena program by
Silvaco is used to represent the successive deposition distributions for different
incident angles. The angular distribution of sputtered Cu atoms is extracted from
the simulated deposition profile that matches the measured profile. Then, the optimized
process condition is applied to the deep contact with aspect ratio of 10 and the measured
profile of Cu film is compared with the simulated deposition profile to validate the
extracted angular distribution of atomic flux.
3. RESULTS AND DISCUSSION
The main factor that determines the bottom step coverage and the deposition profile
is the angular distribution of the sputtered flux. In general, the angular distribution
of sputtered atoms can be expressed as the following formula [10-12]
where Ytotal is the total integrated yield, θ is the cone angle, ρ is the fitting (an empirical
parameter), and dΩ is the differential solid angle in the direction of emission. ρ
< 1 indicates the under-cosine distribution, ρ > 1 implies the over-cosine distribution.
Therefore, the large ρ value with the over-cosine distribution increases the directionality
of the sputtered atoms towards the substrate, thus improving the bottom coverage [13]. To empirically determine the value of ρ, we use both simulation and the empirical
measurement of film profiles on overhang structures. With the assumption that the
angular distribution has an elliptical shape (cosine law), the amount of flux for
each angle can be calculated as the length of the vector.
where xi is the scalar length of the vector, θ is the cone angle, a is the length of the short axis, b is the length of the long axis, and ρ is b/a. As shown Fig 1, each of the fluxes passing through the hole is deposited continuously on the bottom
surface. The amount of each flux depends on the value of ρ and can be calculated using
Equation (2). Integration of the magnitude of flux can produce the deposition profile of the bottom.
Then, the value of ρ is determined from the best match between the simulated profile
of the films and the empirical film profile.
Figure 2 shows empirical profiles of films and simulations at two different working pressure
for Cu sputtering where the DC power, the substrate RF power, and deposition time
were set at 40 kW, 0 W, and 60 s respectively. The decrease in the working pressure
produces the increase in the top-to-bottom step coverage from 0.4 at 10 mTorr in Fig 2(b) to 0.7 at 0.5 mTorr in Fig 2(a), where the bottom step coverage is defined as the ratio of the film thickness at
the bottom to the film thickness at the top of contact. As the working pressure decreases,
the mean free path (MFP) of the Cu atoms is increased, resulting less collisions of
the sputtered Cu [14]. The MFP of Cu atoms is estimated to be 380 mm at 298 K and at 0.9 mTorr [15,16]. In this work, the MFP of Cu is comparable to the target-substrate distance of 380
mm. It is expected that directionality is improved without scattering of Cu atoms,
resulting in better step coverage at the bottom. However, if the working pressure
is too low, the maintaining plasma would be reduced, with the reduced deposition rate.
Long throw sputtering is technique used to control the angular distribution [17]. In standard sputtering configurations, there are two primary reasons for a wide
angular distribution of incident flux: first, the distance of a small target to substrate,
and secondly, the scattering of the flux by the neutral working gas as the flux travels
from the target to the substrate. A method to achieve narrow angular distribution
is to use the long throw sputtering systems in which the target can be sputtered at
very low pressures [18].
Figure 2(c)-2(d) show simulated profile of the deposited films carried out at working pressures of
0.5 mTorr and 10 mTorr, respectively. The angle of the flux deposited on the bottom
through the hole was set to be 0 - 53 degrees in the simulation. As the pressure decreases,
the bottom coverage was increased with the increased magnitude of flux toward the
substrate. The best fit ρ values are extracted for the working pressure of 0.5, 1,
5 and 10 mTorr by considering the deposition rate and distribution using equations
(1) and (2). The fit ρ value was estimated to be 2.43, 1.93, 1.45, and 1.01 for the pressure
of 0.5, 1, 5 and 10 mTorr, respectively, as shown in Fig 5 (a). Even though the pressure of 0.5 mTorr shows the highest ρ value with the increased
flux toward the substrate, the working pressure of 1 mTorr was used for the subsequent
experiment since the plasma formation appears to be more stable than the working pressure
of 0.5 mTorr.
Figure 3 shows a series of experiments and simulations in which the substrate RF power was
set to 0 W, 200 W, and 600 W with the DC power of 40 kW, the working pressure of 1
mTorr, and the deposition time of 60 s. As shown in Fig 3(a) and 3(b), the step coverage at the bottom is improved to 0.71 for the RF power of 200 W from
0.6 for the no substrate RF power. It is considered that the increase of bottom step
coverage is attributed to the increased Cu flux towards the contact bottom with increasing
substrate RF power, resulting in the over-cosine shape of flux distribution [19,20]. When the substrate RF power was increased further to 600 W, the bottom coverage
was significantly decreased to 0.57, as shown in Fig 3(c). Such a reduction of film thickness is considered to be due to re-sputtering of Cu
[21]. It was reported that the re-sputtered Cu from the bottom was redeposited on the
sidewall and thus the sidewall thickness could be increased [22,23].
For the substrate RF power of 0 W, 200 W, 400 W and 600 W, the best ρ values are estimated
to be 1.93, 2.60, 2.17, and 1.70, respectively, as shown in Fig 5(b).
Figure 4 shows cross-sectional TEM images of films and simulation images for the DC sputtering
power of 10 kW and 40 kW. For the film deposition, the substrate RF power, the pressure,
and the deposition time was set to 0 W, 1 mTorr, 60 s, respectively. As the DC sputtering
power increases from 10 kW to 40 kW, the film thickness is increased but no change
in the bottom coverage was observed, indicating that ρ is not affected by DC sputtering
power, as shown in Fig 5 (c). It is expected that the increase on the DC puttering power causes the sputtering
yield of Cu atoms to be increased but does not change the angular distribution of
sputtered Cu atoms, resulting in the thicker films with similar deposition profile
[24].
From the experiment, it is shown that the angular distribution of sputtered Cu atoms
is strongly dependent on the base pressure and the substrate RF power, affecting the
bottom step coverage after film deposition. The ρ value that determines the angular
distribution can be expressed as a quadratic function for substrate RF power that
is inversely proportional to pressure. The formula, obtained from the trend line,
is expressed as the following.
where a is (-1)(1.8×10-6/(P+0.0129) + 5.3×10-6), b is (0.032/(P+0.59)) +0.00167, c is (1.717/(P+0.57)) +0.88, RF is the substrate RF power (W), and P is the pressure (mTorr).
Based on the above equation, the optimum process condition with the highest bottom
step coverage is expected to be the pressure of 0.5 mTorr, the substrate RF power
of 200 W, and for DC power of 40 kW with ρ value of ~3.1. To validate the optimization
for the improved bottom step coverage, Cu films are deposited on the deep contact
with diameter of 5 μm, aspect ratio of 10 and the profile of the deposited Cu films
is compared with the simulation of the Cu film with the of 3.1.
Figure 6(a)-6(d) show the measured profile of Cu films by TEM and simulation images for a DC power
of 40 kW, a pressure of 0.5 mTorr, and a substrate RF power of 200 W. Experimental
measurement of Cu profile shows the film profile at the side and the bottom of the
contact, where the film thickness is reduced as the distance from the contact opening
is increased, which is similar to the simulation of deposited film in deep contact.
The extraction of ρ values from comparison of experimental film profile with simulation
profile using the overhang structure is useful tool to extract angular distribution
of the sputtered atom at various sputtering conditions.
4. CONCLUSIONS
In this study, the angular distribution of sputtered Cu atoms in long-through sputtering
system is investigated by the comparison of the deposition profile measured in overhang
structures with the simulated deposition profile from the cosine law. Also effect
of the sputtering process parameters such as the operating pressure, the substrate
RF power, and the DC target power are investigated. Reducing operating pressure enhances
the over-cosine distribution with increased bottom step coverage in the contact. Increasing
the substrate RF power also enhances the over-cosine distribution but reduces the
bottom step coverage with too high RF power. DC target power, however, does not affect
the angular distribution of sputtered Cu atoms even though the sputtering yield is
increased with increasing DC power. Also it is demonstrated that the optimum sputtering
condition for high bottom step coverage for deep contact is deduced from effects of
process parameters and is validated with the deposition profile of Cu films in the
deep contact of aspect ratio of 10.
Acknowledgements
This work was supported by the Ministry of Trade, Industry & Energy (MoTIE, Korea)
under Industrial Strategic Technology Development Program (Grant no. 10067481) the
R&D Program of the industry-university cooperation project of SK hynix Inc., and the
Brain Korea 21 plus projects (BK21 plus).
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Figures
Fig. 1.
Schematic diagram of the angular distribution of sputtered atomic flux and the thickness
profile of a film deposited at the bottom of jar-shaped contact pattern.
Fig. 2.
Cross-sectional TEM images of deposited Cu films and simulated Cu profiles at the
bottoms of jar-shape-patterns with varying Ar pressure. For the deposition of Cu film,
DC power, substrate RF power, and deposition time were set to 40 kW, 0 W, and 60 s,
respectively. Ar pressure during Cu sputtering was set to be (a) 0.5 mTorr and (b)
10 mTorr. Simulated Cu profiles (c) with r value of 2.43 for Ar pressure of 0.5 mTorr,
and (d) with r value of 1.01 for Ar pressure of 10 mTorr.
Fig. 3.
Cross-sectional TEM images of the deposited Cu films and simulated Cu profiles at
the bottoms of jar-shape-patterns with varying substrate RF Power. For the deposition
of Cu film, DC power, Ar pressure, and deposition time were set to 40 kW, 1 mTorr,
and 60 s, respectively. The RF power was set to be (a) 0 W, (b) 200 W, and (c) 600
W. Simulated Cu profiles (d) with r value of 1.93 for the RF power of 0 W, (e) with
r value of 2.60 for the RF power of 200 W, (f) with r value of 1.70 for the RF power
of 600 W.
Fig. 4.
Cross-sectional TEM images of the deposited Cu films and the simulated Cu profiles
at bottoms of jar-shape-patterns with varying DC Power. For the deposition of Cu film,
RF power, Ar pressure, and deposition time were set to 0 kW, 1 mTorr, and 60 s, respectively.
The DC power was set to be (a) 10 kW, (b) 40 kW The simulated profiles of Cu films
(c) with r value of 1.93 for the DC power of 10 kW and (d) with r value of 1.93 for
the DC power of 40 kW.
Fig. 5.
ρ values that were estimated for various sputtering parameters (a) of operation pressure,
(b) of substrate RF power, and (c) of DC power for target.
Fig. 6.
The simulated thickness profile of Cu film and the crosssectional SEM images of Cu
films deposited on a deep contact of aspect ratio 10 (a diameter of 5 μm) (a) at the
top of contact, (b) 10 μm from the top, (c) 20 μm from the bottom, and (d) at the
bottom of a deep contact hole, respectively. For Cu sputtering, DC power, pressure,
substrate RF power, and deposition time were set to 40 kW, 0.5 mTorr, 200 W, and 60
s, respectively.