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Ion Implantation and Temperature HEROS Modeling
Qiyang Hu , Shahram Sharafat, Nasr Ghoniem Mechanical & Aerospace Engineering University of California, Los Angeles San Diego, Aug 8th, 2006
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Leads to confidence in predicting IFE conditions
Objectives Calibrate HEROS with a wide range of applications: Deep implantation in pulses by UNC Shallow implantation in steady states by IEC condition Shallow implantation in steady states by Nishijima’04 Leads to confidence in predicting IFE conditions
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HEROS Code Improvement
Simulation Discussion Conclusions and Future Plans
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Previous HEROS code has serious numerical instability problems:
In most cases: Time to be simulated < 10 sec Running Time > 6 hours Time step > 2000 steps Temperature range < 2000 K
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HEROS model is improved:
Still, reaction-diffusion rate equation: Simplify the equation Ignore some cluster effects: (e.g. vacancy clusters, interstitial clusters etc.) 18 variables/equations 13 Ignore bubble coalescence
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HEROS numerical scheme:
Temperature profile Within a bin, each C(i) is in an average sense Implantation profile … W back W front variable bin size
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Recent Progresses in Modeling Helium Behavior:
Can integrate equations for thousands of pulses. Can include rapid temperature transients. Aim to calibrate model with experimental data.
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HEROS Code Improvement
Simulation Discussions Conclusions and Future Plans
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First, we want to use our new HEROS code to model UNC(’05) & UWM(’04) conditions.
We re-simulated UNC & UWM’s implantation cases Helium Implantation Damage
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UNC’s Temperature Profile
( L. Sneed,2005 )
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After 1 cycle of 1019 He/m2: Temperature C Time (sec) 2000C 850C
3000 3060 Time (sec)
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After 10 cycle of 1018 He/m2/cycle:
Temperature C 2000C 850C 300 360 720 Time (sec)
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After 100 cycle of 1017 He/m2/cycle:
Temperature C 2000C 850C 30 90 180 Time (sec)
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After 1000 cycle of 1016 He/m2/cycle:
Temperature C 2000C 850C 3 63 126 Time (sec)
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Helium Retention: Diffuse too fast in HEROS Short pulse OK! Cycles:
1000 100 10 1
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Bin Number=20; Total width=10m
Bubble & Radius Movies: HEROS also gives the spatial distribution information Bin Number=20; Total width=10m
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For UWM’s IEC conditions: Some notes before comparisons:
Surface bubble Surface pore Surface bubble density (volume bubble density|surf)2/3 We focus on steady condition.
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New HEROS code is stable and gives the information about bubble (pore) sizes:
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So does the pore density …
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We also calibrate our model by Nishijima group’s experiments (ITER):
Temperature: = 1950 C Gh 1m x
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HEROS also gives the spatial distribution information (average sense):
Bin Number=20; Total width=10m
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HEROS for temperature modeling:
Surface Heating Emissive effect can be ignored B.C. Max
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HEROS Code Improvement
Simulation Discussion Conclusions and Future Plans
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Total time to be simulated
Conclusions: Capabilities of HEROs code are largely improved Our HEROS can integrate equations : with thousands of pulses. with rapid temperature transients. Need to improve: Helium: More trapping mechanism Heat: new mechanism HEROs Total time to be simulated Running time Required time steps Temperature range Previous <10 sec >6 hrs >2000 steps <2000 K Current >106 sec <5 mins < 100 steps <3500 K
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Planning on HEROS: Implement recent “pulsed” conditions:
UWM UNC Implement IFE conditions Add bubble coalescence Exceed the 0-order (average) description Temperature/carbon diffusion problem
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We wish to develop a unified temperature/diffusion/microstructure code
Containing: Temperature transients Helium distribution Carbon distribution Point defect/displacement damage
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Thanks!
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Backup Slides
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Helium retention for IEC condition:
Most of He are in grain boundary
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