Atomistic simulations of deep submicron interconnect metallization Y. G. Yang,a) X. W. Zhou, R. A. Johnson, and H. N. G. Wadley Department of Materials Science and Engineering, University of Virginia, Charlottesville, Virginia 22903 共Received 27 July 2001; accepted 14 January 2001兲 Damascene approaches are widely used for creating microelectronic interconnects. Successful implementation of the process is reliant upon the deposition of a refractory metal or metal nitride liner coating. It functions as a diffusion barrier layer to suppress transport of subsequently deposited interconnect metals into the surrounding dielectric. The development of vapor-phase processes for the deposition of uniform thickness liner layers has been problematic. Flux collimation and energetic deposition approaches have been attempted with mixed results as the feature size is decreased. Here, a modified kinetic Monte Carlo 共KMC兲 method has been used to explore the physical vapor deposition of liner coatings. To incorporate the many effects associated with energetic metal fluxes, the results of molecular dynamics calculations of incident atom reflection, resputtering, surface biased diffusion, and athermal relaxations have been introduced into the KMC algorithm. The method has been applied to investigate the effects of the incidence flux’s angular distribution and kinetic energy upon the liner coating coverage. It has been found that trench step coverage uniformity increases with increasing atom kinetic energy above a threshold energy value of 20 eV. Atom resputtering/reflection are found to be the most important mechanisms responsible for improvements in the step coverage. Sputtering of already deposited material is found to be the most important mechanism for transporting the flux to the most difficult to coat lower sidewall region of a trench. Energetic deposition processes that activate these mechanisms are therefore preferred. The simulations reveal the existence of an optimal incident angular distribution to maximize coverage uniformity. For a flux with a kinetic energy of 70 eV, a cosine angular distribution within the collimation angle of ⫾15°–25° provided the best balance of direct and resputtered/reflected fluxes to maximize coating uniformity. © 2002 American Vacuum Society. 关DOI: 10.1116/1.1458952兴 I. INTRODUCTION In a damascene interconnect manufacturing process,1–3 trenches or vias are etched in a flat dielectric and a conducting metal is then placed in the cavities. The process is followed by chemical mechanical polishing to planarize the embedded conductors. This approach is dramatically different from earlier approaches, which were based on the reactive ion etching of blanket metal films followed by dielectric deposition and planarization.3 The recent transition to copper as the interconnect metal also requires the use of a thin, conformal layer on the inner surface of the patterned dielectric to promote adhesion and facilitate nucleation and growth of the best interconnect microstructure in addition to functioning as a barrier layer that prevents copper diffusion through the dielectric.1,2 This layer also plays a role in inhibiting chemical reactions between the deposited metal conductor and the dielectric.2 Various barrier layer materials including titanium, titanium nitride, and various refractory metals and compounds are used for the diffusion barrier.2 These coatings are known generically as ‘‘liner’’ films, since their role is to conformally line the sidewalls and bottoms of the various trenches and vias used to create the interconnect structure. To achieve the functions above, it is critical that the liner layer is continuous and free of pinholes. Since it is also desirable to maximize the cross sectional area of the a兲 Electronic mail: [email protected] 622 J. Vac. Sci. Technol. B 20„2…, MarÕApr 2002 interconnect 共for current flow兲, the thinnest possible pinhole free coating is needed. Both are achieved by a coating of uniform thickness. Liner films are usually deposited by sputtering—a simple, relatively low cost physical vapor deposition 共PVD兲 process.1 At typical process pressures, PVD is a geometrical line-of-sight deposition process. A simple view factor model presented in the Appendix reveals that the direct flux incident upon the interior of a trench is nonuniform. Thus thickness nonuniformity within the trench is a significant problem.1–7 This has been particularly true for high aspect ratio structures and as result, the development and optimization of the PVD process is becoming correspondingly more difficult as feature widths 共but not depths兲 decrease. Additional complexity results from the high kinetic energy of the impacting metals in a low pressure sputtering2 or ionized PVD process.1 High energy impacts can result in atom reflection and resputtering 共to regions out of the line of sight of a target兲 and activate athermal modes of atom diffusion.8 –11 This has stimulated our interest in the use of simulation techniques that can predict thin film thickness given as an input, the angular distribution of the atomic flux, its kinetic energy, and the aspect ratio of a trench. Many simulation approaches have been explored for this class of problems.4 –7,12–17 They can be classified into two types: those based upon continuum methods4 –7,12 and those that utilize atomistic techniques.13–17 The continuum ap- 1071-1023Õ2002Õ20„2…Õ622Õ9Õ$19.00 ©2002 American Vacuum Society 622 623 Yang et al.: Atomistic simulations of deep submicron metallization proaches first calculate the speed with which the material is added to, or removed from a small region of the surface 共a node or cell兲. This depends on the net effect of deposition, etching 共resputtering兲, and diffusive flow on the films surface.5 A moving front algorithm such as the string,6 shock wave,7 or level set12 method is then used to incrementally advance the surface. To approximate the effects of the impacting atoms kinetic energy, a simple sticking coefficient approximation is often made. While continuum methods can reasonably predict the topography of the growth surface during a metallization process, the method is less suited to the analysis of individual device features that have entered the deep submicron region where atomic reflection/resputtering can redistribute the flux and athermal diffusion distances can approach the dimensions of the feature.5 Most atomistic approaches applied to metallization are based on either the SIMBAD method13 or a Monte Carlo technique.14,15 In the SIMBAD method, the effect of thermally activated surface diffusion is approximated by a ‘‘mobility’’ factor. The mobility factor allows a landed disk 共i.e., an atom cluster兲 to move a specified distance once before stopping for good. A higher deposition temperature is modeled by a longer distance. The technique does not address the change in mobility that accompanies changes to the atomic scale surface roughness. The effects of an adatom’s kinetic energy such as atom resputtering have been attempted to be incorporated by using data from experimental measurements. Often the experimental data for a specific metal under the required conditions is unavailable and approximations have to be made to fit the materials and conditions of the case of interest.13 This subclass of model has additional problems when used to link film morphology to process conditions. Since diffusion of any one of the atoms in the system is allowed only once, the constant rearrangement of the atomic ensemble configuration during deposition cannot be simulated, and since time is also not explicitly included, the role of the deposition rate cannot be quantitatively analyzed nor its tradeoff against deposition temperature. Kinetic Monte Carlo methods that more realistically treat thermally activated atom jumps have been developed and used to investigate deposition on flat and patterned surfaces.14,15 While these approaches do allow the role of temperature, flux incident angle distribution, and deposition rate to be reasonably well evaluated, the role of the incident atoms kinetic energy has until recently not been addressed. In one recent approach molecular dynamics 共MD兲 simulations of impacts have been followed by kinetic Monte Carlo 共KMC兲 relaxation.18 However, the great computational cost of such an approach precludes its use for the study of liner deposition where many thousands of impacting atoms must be examined. In an alternative to the direct MD/KMC method,18 a KMC approach has recently been extended to energetic atom deposition by incorporating the results of off-line MD simulations of energetic incident atom interactions with substrate atoms.19 Reflection, resputtering, biased, and athermal diffusion were examined and their dependence upon the impact energy and angle catalogued. A modified 共hyperthermal兲 JVST B - Microelectronics and Nanometer Structures 623 KMC algorithm was then developed and used to simulate the PVD of metals on a flat surface.19 The energy incorporated KMC method avoids the computational demanding direct combination of KMC and MD,18 while still addressing energy dependent phenomena such as reflection and resputtering,8 biased surface diffusion, and thermal spike induced atomic relaxation at the impact site.9 It is important to include surface biased diffusion and athermal relaxation since they can have significant effects upon film coverage, especially when atomic mobility is limited by a low substrate temperature and/or a high deposition rate. For example, surface biased diffusion was reported to be the cause of a layer by layer 共step flow兲 growth mode at cryogenic temperature where island growth 共and pinhole formation兲 is more usually expected.20 Here, we briefly review the fundamentals of hyperthermal incident atom impacts and the design of a KMC technique for simulating atomic self assembly following a hot atoms impact with a surface. The technique is then applied to analyze the deposition of thin metal films on the interior surface of a trench. The technique can be used to investigate the effect upon coating thickness uniformity of the many adjustable PVD process parameters including the substrate temperature, the deposition rate, the atomic kinetic energy, truncation of the incident metal atom angle distribution, and the aspect ratio of the feature. II. METHODOLOGY To simulate the deposition of thin films from energetic metal fluxes both impact energy and thermally activated atomic diffusion must be addressed. When interconnect deposition takes place under conditions that result in zone I or zone II of the structure zone model,21 surface diffusion dominates the evolution of the film profile. The contribution of bulk diffusion in this regime is negligible. The first step is to identify an appropriate surface diffusion model to track the constant rearrangement of atoms in the simulated system. Kinetic Monte Carlo methods appear to be the best approach for simulating competing thermally activated processes.14,22–24 In this approach atomic configurations evolve by identifying and executing all available thermally activated jumps. The likelihood that an atom jumps from one lattice site to another depends upon its local configuration, which can be characterized by an activation energy and/or a jump attempt rate. The details of the simulation approach used here can be found in Ref. 14. Briefly, it first deduces the set of jump rates for every allowed jump path using precalculated activation energies and then executes jumps according to their relative probabilities. After a jump is executed, time is advanced by the residence time of the system, i.e., the reciprocal of the sum of the jump rates for all the allowed jump paths of the system. This process is then repeated until the time between atom arrivals is exhausted. A new atom is then added and the algorithm iterated. The second step is to incorporate interactions of energetic incident atoms with the growing film. This interaction includes incident atom reflection, resputtering, biased diffu- 624 Yang et al.: Atomistic simulations of deep submicron metallization sion, and athermal rearrangement induced by the thermal spike that arises from partitioning of the impacting atoms velocity and heat of condensation among the lattice vibrational modes near the impact site.8,10,11 The impact energy/ angle dependence of these processes has recently been investigated by MD10,11 and their effects incorporated in a hyperthermal KMC code. A detailed description of the impact atom energy dependent implementation can be found in Ref. 19. The essential concept is recognition that impact energy induced processes are completed in a few picoseconds, whereas thermally activated hopping occurs intermittently with quiescent times in the nano- to microsecond range. In a simulation, energy dependent mechanisms of transport can therefore be implemented instantaneously followed by thermally activated assembly. Briefly, the reflection and resputtering is incorporated by first identifying the incident atom’s impact angle and kinetic energy. The probability of either reflection, resputtering, or both is then deduced from the results of previous 共off-line兲 MD calculations.11 The relevant atoms’ next movement direction and residual energy are also determined from results of the same calculations. The reflected and/or resputtered atom is then ballistically translated until it either again impinges with the surface or is removed from the system 共if no surface is encountered兲. To incorporate biased diffusion, the diffusion distance is first deduced from a MD simulation.10 Steps and ledges can arrest the process and so the distance to the nearest ledge or step from the impact site is deduced. If this is greater than the MD computed bias diffusion distance, the MD precalculated distance is used. Otherwise, the atom is allowed to reach the ledge or step and then arrest. The remote atoms kinetic energy and its heat of condensation are both partitioned among the local modes of vibration near an atoms impact point. This rapidly heats the surface near the impact site, allowing thermally activated jumps to occur before cooling to the quiescent background. This jumping rate depends weakly on the background temperature and is termed athermal diffusion.10 The athermal relaxation rate depends upon both the atoms’ acquired energy 共or equivalently the temporary rise of temperature兲 for each atom in the neighborhood of the impact and the activation barriers for rearrangement near the impact site. The atom with the highest energy and the lowest energy activation barrier is taken to have the highest probability to jump to a lower surface energy site. We characterize it by a jump probability, P i ⫽(E/Q) n , where E is the energy of an atom in the thermal spike zone precalculated from MD simulations,10 Q is the activation energy for a jump pathway,14 and n is an adjustment parameter that is found by fitting hyperthermal KMC results to MD simulation. A jump is allowed when P i ⬎ P, a jump index number also deduced from MD simulations. If an atom has a pathway meeting the above condition, it is then said to have a finite probability of jumping to a new place through that path. When many atoms have a nonzero probability to jump along different paths, the jump simulation is conducted in such a way that the probability for the jump in the ith pathway scales with P i . Once the jump is made, P i is J. Vac. Sci. Technol. B, Vol. 20, No. 2, MarÕApr 2002 624 FIG. 1. Schematic geometry for deposition from an extended source over a featured substrate used in the simulations. The trench parameters and the placement of the flux monitors on it are also shown. Each monitor had a length of L/10. updated for all the paths. This procedure is then iterated until no atoms have a finite probability to move. Simulations have been carried out with a two-dimensional 共2D兲 lattice using periodic boundary condition applied in the horizontal direction. The substrate had a width of 200 atoms. The trench was set to be 100 atoms in width. The activation barriers for atomic jumps on this surface were taken to be those for nickel.14 The atoms were randomly introduced from a target surface above the substrate with a 共sometimes truncated兲 cosine distribution,1 Fig. 1. When the flux was highly collimated, the simulation was analogous to that encountered in ionized PVD.2 The kinetic energy was assumed to be uniform within a simulation run and was varied between runs to investigate the effect of the kinetic energy. The substrate temperature was fixed at a 2D homologous temperature of T/T m ⫽0.3, which corresponds to 350 K and the deposition rate R fixed at 1.0 m/min. A total of 15 000 atoms were deposited and generally took less than 1 h on RS/6000 machines to execute. 共The execution time expects to increase exponentially with increasing substrate temperature.兲 The step coverage was used to characterize each run. It was defined as the relative thickness at a point on the trench surface scaled by the thickness of the film on the top areas of the trench2 and was recorded at three monitor positions on the sidewall and at the center of the bottom surface, Fig. 1. It is worth pointing out that the energy dependent phe- 625 Yang et al.: Atomistic simulations of deep submicron metallization FIG. 2. Effect of incident energy E on step coverage. The substrate temperature was 350 K (T/T m ⫽0.3), the deposition rate R was 1.0 m/min, the incidence flux had a cosine angular distribution within the collimation angle of ⫾25°. The aspect ratio of the trench was 5. 15 000 atoms were used for the simulations. The black regions correspond to the deposited coating. nomena 共sputtering yields, etc.兲 were obtained from threedimensional MD simulations and hence should correctly reflect the incidence flux and deposition rate. Because metallization geometries are mostly symmetric, the growth is simulated using a 2D model, which constrains atomic relaxations on a plane and reduces the number of diffusional paths. However, the differences should only have minor effects on the model’s qualitative predictiveness on surface morphological evolution. III. SIMULATION RESULTS The effect of atom energy upon the coverage of a trench with an aspect ratio of 5 is shown in Fig. 2. When the energy was 20 eV 共or less兲 关Fig. 2共a兲兴 the liner deposited on the sidewalls had a rough columnar-like structure prone to the formation of pinholes. The upper sidewall part of the coating had a greater thickness than that of the lower part. The pinholes were most prevalent close to the trench bottom. Coverage on the sidewalls was improved when the energy was increased to 40 eV 关Fig. 2共b兲兴. The surface was also smoother on all inner surfaces and no pinholes were present. When the energy was increased to 70 eV 关Fig. 2共c兲兴, the coating thickness in the lower part of the trench increased to nearly that of the mid section. The coverage on the bottom was also thicker. This trend of coverage change with increasing atom energy has found excellent agreement with the experiments.2 The step coverage dependence upon atom energy is summarized in Fig. 3 for each monitor position. As the energy was increased from zero, the upper trench wall and bottom coverage both initially decreased. Above 20 eV, step coverage at all monitor positions increased with increasing atom energy. The step coverage at the bottom was always greater than that on the sidewalls. The rate of increase in thickness JVST B - Microelectronics and Nanometer Structures 625 FIG. 3. Effect of incident energy on step coverage. for the bottom and the upper sidewall appear similar but are noticeably greater than that for the mid and the lower parts. The amount of material left at the trench top decreases sharply with increasing atom energy above 20 eV 共Fig. 2兲. The decrease in bottom and upper sidewall coverage as the energy increases from 0 to 20 eV is a result of biased diffusion of material above the trench. This process transports material into the trench throat resulting in strong shadowing. Increasing the energy further induces sputtering of this material, which then reopens the trench throat and reduces shadowing of the trench interior. It is interesting to note that the increase of step coverage at all inner surface locations arises from material that, at low energy, would otherwise have assembled at the trench top to create the 共flux shadowing兲 overhang at the trench throat. Figure 4 shows the effect of the truncating the flux incident angle distribution 共collimation兲 on the liner coating process at a fixed atom energy of 70 eV. At a 5° cutoff 关Fig. 4共a兲兴 the majority of the middle sidewalls are sparsely coated and pinholes were present. At the lower corners, however, an extraordinary thick coating can be seen. Since incident atoms rarely reach this location directly and surface diffusion is not sufficient at this deposition temperature, the extra deposit must originate from energy induced redistribution mechanisms discussed above. This, in particular, agrees well with the experimental observations1 and would not be possible without including the energy effects into the KMC model. As the width of the distribution was increased by increasing the truncation angle to 25° 关Fig. 4共b兲兴 considerably better sidewall coverage was seen, and the amount of material deposited at the bottom of the trench was significantly decreased. These deposition conditions are close to the best for achieving uniformity of deposition. As the distribution was allowed to broaden by increasing the truncation angle to 45° 关Fig. 4共c兲兴, the lower sidewall coating thickness decreased while 626 Yang et al.: Atomistic simulations of deep submicron metallization FIG. 4. Effect of collimation angle on step coverage. The substrate temperature was 350 K (T/T m ⫽0.3), the deposition rate R 1.0 m/min, the incident kinetic energy E was 70 eV, and the trench aspect ratio was 5.15 000 atoms were used for the simulations. The black regions correspond to the deposited coating. that at the upper sidewall increased. Atom accumulation on the upper sidewalls was consistent with the greater probability of direct atom impact near the trench top because of the inclusion of more of the obliquely incident flux. The results in Fig. 4 indicate the existence of an optimal incident collimation angle for the most uniform liner coating. To better explore this, additional results were obtained and are plotted in Fig. 5. It can be seen that the most uniform sidewall coverage occurs at a truncation angle between 15° and 25°. It is apparent that the coverage at the bottom of the trench decreases with broadening of the incident angle distribution but 626 FIG. 6. Effect of trench aspect ratio on step coverage. The substrate temperature was 350 K (T/T m ⫽0.3), the deposition rate R was 1.0 m/min, the incidence flux had a cosine angular distribution within the collimation angle of ⫾25°, and the incident kinetic energy E was 70 eV. 15 000 atoms were used for the simulations. The black regions correspond to the deposited coating. is always significantly greater than that of the sidewalls. However, this may not be a significant issue for the manufacture of interconnects since the resulting loss of conductor area could be compensated by a minor increase in the depth of the trench etch. The observations above are sensitive to the aspect ratio of the trench. Figure 6 shows the effect of the trench aspect ratio on coating thickness. It can be seen that at an aspect ratio of 3 关Fig. 6共a兲兴 the coating thickness along the sidewalls is very uniform. As the aspect ratio was increased to 5 关Fig. 6共b兲兴 and then 7 关Fig. 6共c兲兴, the coating at the lower half of the sidewalls and on the trench bottom thinned. This thinning was sufficient to result in pinhole formation when the aspect ratio was increased to 7 关Fig. 6共c兲兴. The coating thickness trends with aspect ratio are shown in Fig. 7. It can be seen that coverage at all interior surface locations decrease monotonically with increasing aspect ratio. The most noticeable decrease appears at the bottom of the trench. Little change in thickness occurs at the upper sidewall, which remains in the direct line of sight of a majority of the flux. IV. DISCUSSION FIG. 5. Effect of collimation angle on step coverage. J. Vac. Sci. Technol. B, Vol. 20, No. 2, MarÕApr 2002 In a liner coating process the objective is to obtain a uniform, pinhole free layer across the full interior of the trench. Since the upper part of the trench is closer to the vapor source material, it is always well positioned to directly receive more of the incident atoms. Shadowing by the upper part of the trench reduces the flux directly incident upon the lower parts of the trench. This inevitable effect increases with trench depth and divergence in the angular flux distri- 627 Yang et al.: Atomistic simulations of deep submicron metallization FIG. 7. Effect of trench aspect ratio on step coverage. bution. The problem is dynamic in the sense that the buildup of material at the trench throat increases the extent of shadowing. Two approaches have been experimentally explored to improve coating uniformity. One utilizes surface diffusion by increasing the substrate temperature 共thermal reflow兲.2 The high temperature enables diffusion over distances comparable to the trench dimensions. Different curvature of the surface then drives mass transport. However, this strategy is difficult to implement for liner deposition because of the use of refractory materials which require the use of too high a temperature.2 The second approach is to use energetic deposition in combination with flux collimation. Ignoring the role of energetic working gas ion bombardment, we have seen that energetic incident atoms can undergo reflection and cause resputtering of previously deposited material at the impact site.8,11 The simulations above indicate that both help to redeposit material to regions that otherwise would be shadowed. This reduces accumulation 共and shadowing兲 at the upper areas of the trench 关Figs. 2共b兲 and 2共c兲兴. As seen in Fig. 2共a兲, when the energy is low, the atoms do not trigger these desired interactions. Instead only biased and athermal diffusion occurs and these are insufficient to avoid material accumulation at the trench throat. The simulations indicate that the local thickness of the liner layer is governed by the flux directly incident upon the surface and that which is retransported by energy dependent transport mechanisms. To more completely understand the role of each, we have developed a simple view factor model to predict the local flux incidence upon the interior surfaces of the trench, while ignoring reflection, resputtering, and the assembly mechanisms discussed above. This flux illumination model and its analysis can be found in the Appendix. JVST B - Microelectronics and Nanometer Structures 627 FIG. 8. Effect of incident cutoff angle on step coverage. The curve was predicted from the view factor analysis. The symbols represent simulated data at various positions inside the trench. The simulations were done with the substrate temperature of 350 K (T/T m ⫽0.3), deposition rate of 1.0 m/min, aspect ratio of 5, kinetic energy of 0 eV, and 15 000 atoms. Figures 8 and 9 show comparisons of the flux illumination model 共solid lines兲 and full Monte Carlo solutions for incident atom energies of 0 and 70 eV. For the low energy case 共Fig. 8兲, the retransport mechanisms discussed above are ab- FIG. 9. Effect of cutoff angle on step coverage. The curve was predicted from the view factor analysis. The symbols represent simulated data at various positions inside the trench. The simulations were done with the temperature of 350 K (T/T m ⫽0.3), deposition rate of 1.0 m/min, aspect ratio of 5, kinetic energy of 70 eV, and 15 000 atoms. 628 Yang et al.: Atomistic simulations of deep submicron metallization sent. The model shows that the flux incident upon the bottom of the trench decreases rapidly as the flux cutoff angle is increased. The decrease is particularly rapid as the cutoff angle is increased from 10° to 30°. This is accompanied by an increase in the flux incident upon the upper sidewall, which increases linearly with increasing cutoff angle. The flux incident upon the mid and the lower sidewalls both initially increase and then decrease as the cutoff angle increases. Deviations between the flux illumination model and the Monte Carlo results are a manifestation of flux shadowing by previously deposited material. For highly divergent fluxes this effect is large. It also has important effects for highly collimated fluxes. The flux illumination model and Monte Carlo model indicate that a compromise cutoff angle of 12°–15° provides the best sidewall coverage. Figure 8 also shows the full KMC simulation results for an incident atom energy of 0 eV. In this, the biased diffusion distance as well as the reflection and resputtering probabilities are close to zero since thermal diffusion results in little transport. The results therefore show the effects of the dynamic nature of flux shadowing due to the buildup of material near the trench top. The evolving shadowing has the most significant effect at the upper sidewall and is most important for small cutoff angles. The results indicate the need for a flux cutoff angle of at least 12° to avoid shadowing at the top sidewall monitor position. Figure 9 shows a comparison between the view factor model and KMC simulation for atoms with an energy of 70 eV. Significant differences can be seen. The KMC predicted coverage at the bottom of the trench exceeded that of the incident flux model for the high cutoff angle. This is shown below to result from reflection and resputtering from the sidewalls. A similar increase was seen at the upper walls for small cutoff angles and also resulted from the sputtering and reflection. To investigate more quantitatively the role of the various assembly mechanisms we have performed simulations in which the mechanisms of material redistribution have been selectively turned off. Detailed simulation results are shown in Fig. 10 and a summary is presented in Fig. 11. Using an energy of 70 eV and flux cutoff angle of 25°, Fig. 10共a兲 shows the configuration when all energy induced assembly mechanisms and thermal diffusion were enabled. Adequate coverage at both the sidewalls and at the bottom can be seen. In Fig. 10共b兲, energy induced reflection was suppressed while all other mechanisms remained intact. It can be seen that the thickness at the lower part of the sidewalls and at the bottom are noticeably thinner. This is a clear indication that reflection helps redirect a significant fraction of the incident atoms to the lower part of the trench bottom. The narrowing of the trench opening 共a manifestation of material accumulation at the trench opening兲 when reflection was absent is a graphic indication of the importance of the reflection mechanism. In Fig. 10共c兲, the sputtering was suppressed while all other mechanisms remained intact. The lower parts of the sidewalls are now even thinner than that of Fig. 10共b兲, whereas the thickness at the bottom compares favorably to J. Vac. Sci. Technol. B, Vol. 20, No. 2, MarÕApr 2002 628 FIG. 10. Contributions of each impact energy induced mechanism to step coverage. For all four cases the substrate temperature was 350 K (T/T m ⫽0.3), the deposition rate R was 1.0 m/min, the incidence collimation angle was ⫾25°, the aspect ratio was 5.0, and the incident kinetic energy E was 70 eV: 共a兲 all energy induced mechanisms are present, 共b兲 reflection suppressed, 共c兲 self-resputtering suppressed, and 共d兲 both reflection and selfresputtering mechanisms suppressed. that of the full treatment 关Fig. 10共a兲兴. Self sputtering is therefore seen to have the most significant effect upon coverage of the lower sidewall area of the trench where undesirable pinhole formation is most likely. This discovery has been confirmed by experiments25 and illustrates the usefulness of modeling in explaining phenomena that are otherwise elusive. In Fig. 10共d兲, both the reflection and self-resputtering mechanisms have been turned off. The coating at the lower FIG. 11. Contributions of each impact energy induced mechanism to step coverage. Test mode: 共1兲 all energy induced mechanisms are present; 共2兲 reflection suppressed; 共3兲 self-resputtering suppressed; and 共4兲 both reflection and self-resputtering mechanisms suppressed. 629 Yang et al.: Atomistic simulations of deep submicron metallization sidewalls is much thinner, that at the bottom is reduced, and the trench throat is much narrower, which contributes to a more severe self-shadowing effect. The results shown above have been summarized in Fig. 11. The discrete numbers on the abscissa are the test modes in the same order presented in Fig. 10. The shaded areas in the histograms are scaled to represent the step coverages at the different locations. Obviously, the full treatment represented by test mode 1 is the best. Simulation approaches that do not include the reflection and resputtering effects 共test mode 4兲 are clearly unlikely to be adequate. Test modes 2 and 3 indicate that reflection transfers more atoms into the trench than resputtering. However, at the lower sidewall monitor position 共the site most vulnerable to pinhole formation兲, resputtering is the most important mechanism for improving uniformity. The results of the KMC simulation indicate that a complex interplay occurs between the energy and incidence angle distribution of an atomic flux and the geometry of a trench whose interior is being coated. Uniformity in thickness at all locations within the trench appears an elusive goal. But uniformity of the sidewalls and a thicker trench bottom coating appears viable in the deep submicron regime. The best results are found when the incident energy is high 共within the limit of 70 eV used in this work兲 and a flux cutoff angle of between 15° and 25° is used. ACKNOWLEDGMENTS The authors are grateful to Dr. Steve Rossnagel 共IBM兲 for helpful discussions concerning interconnect manufacturing. The Defense Advanced Research Projects Agency 共A. Tsao and S. Wolf, Program Managers兲, and the National Aeronautics and Space Administration supported this work through NASA Grant Nos. NAGW1692 and NAG-1-1964. APPENDIX: FLUX ARRIVAL DISTRIBUTION AT TRENCH To obtain arrival distributions of incident flux on all surfaces inside a trench, we assume no kinetic energy induced reflection and resputtering and every atom sticks to its initial impinging position. We further assume the incident flux to be a cosine distribution 共it can be any other type of distribution function兲 which may be truncated using a collimator. Figure 1 shows a sketch of a trench with an incidence distribution truncated by . Arbitrary feature width and unit are used in the view factor analysis. Flux illumination at the top is normalized to be 1.0 and would thus be correspondingly smaller on all other surfaces. For flat surface like the trench top having open space above, the net flux illumination at an arbitrary position can be expressed as f 共 x 兲⫽ V. CONCLUSIONS A comprehensive energy dependent kinetic Monte Carlo method has been developed to simulate the PVD application of a refractory metal trench liner. Important impact energy dependent atom–substrate interaction events, including reflection, resputtering, surface biased diffusion, and athermal relaxation, are precalculated using a MD method and the results formulated as analytical expressions. A modified form of kinetic Monte Carlo modeling is then used to incorporate these hot atom effects into an atomistic treatment of thermally activated atomic assembly. It has been found that interior trench coverage uniformity increases with increasing atom kinetic energy when the energy is greater than a threshold value of 20 eV. Energy induced atom resputtering is most responsible for improving step coverage at the lower sidewall region. Reflection is responsible for a significant transport from the trench mouth region to the interior of the feature. The simulations indicate the existence of an optimal incident atom angle distribution at which the incident flux onto the sidewalls and the bottom can be balanced against that due to resputtering and reflection. For 70 eV fluxes used to coat the interior of trenches with aspect ratios in the 5:1 range, a cosine flux truncated between 15° and 25° results in relatively uniform sidewall coverage. This condition leads to thicker trench bottom coverage, but this may be less of an issue since it can be easily compensated for by increasing the depth of the trench. JVST B - Microelectronics and Nanometer Structures 629 冕 ⫺ cos ␣ d ␣ , 共A1兲 where cos(␣) is the distribution function and 关⫺, ⫹兴 the incident flux range. For all trench horizontal surfaces including the trench bottom, the general expression becomes f 共 x 兲⫽ 冕 u l cos ␣ d ␣ , 共A2兲 where l ⫽⫺⍀ 1 ⫺⍀ 2 •arc tan(x/H) and u ⫽⍀ 3 ⫹⍀ 4 •arc tan(L⫺x)/H; H is the height, L the width of the trench, and x the position away from the left sidewall at the bottom 共Fig. 1兲. The range of expressions of 关 l , u 兴 are due to the geometrical shadowing effect of the sidewalls. The coefficients ⍀ i (i⫽1 – 4) taking values of either 1 or 0 are used to indicate if a position x is under the effect of the sidewalls or not and have the following forms: ⍀ 1 ⫽int ⍀ 2 ⫽int ⍀ 3 ⫽int and ⍀ 4 ⫽int 冉 冉 冉 冉 L⫺x H•tan 冊冒再 冉 冊冒再 冉 冊冒再 冉 H•tan L⫺x 冊冒再 冉 x H•tan H•tan x 冊 冎 冊 冎 冊 冎 int x ⫺␦ , H•tan int H•tan ⫺␦ , x int L⫺x ⫺␦ , H•tan int 冊 冎 H•tan ⫺␦ , L⫺x 630 Yang et al.: Atomistic simulations of deep submicron metallization where int is an integer function and ␦ a small fraction number. The position-dependent incidence illumination at the top and the bottom of the trench upon integration of Eq. 共A2兲 becomes 冉 f 共 x 兲 ⫽sin ⍀ 1 ⫹⍀ 2 •arc tan 冉 x H ⫹sin ⍀ 3 ⫹⍀ 4 •arc tan 冊 冊 L⫺x . 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