Abstract
The backscattering from and the implantation of 0.5–10-keV hydrogen and helium in Au is investigated with the MARLOWE and TRIM computer codes. The following are found in this paper: (1) The results of the MARLOWE and the much faster TRIM codes are in satisfactory agreement. (2) The influence of potential parameters and energy loss models (LSS and Oen-Robinson) is mainly on the heights and to less extent on the shapes of the energy distributions of backscattered particles. (3) The experimental data from the preceding paper favor the use of a potential for the calculation, which is weaker than the Molière potential. This can be simulated by using a screening length smaller than the Firsov value.
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Dates
Type | When |
---|---|
Created | 22 years, 6 months ago (Feb. 14, 2003, 5:37 p.m.) |
Deposited | 1 year, 7 months ago (Feb. 4, 2024, 5:38 p.m.) |
Indexed | 2 months, 3 weeks ago (June 15, 2025, 7:21 a.m.) |
Issued | 45 years, 7 months ago (Feb. 1, 1980) |
Published | 45 years, 7 months ago (Feb. 1, 1980) |
Published Print | 45 years, 7 months ago (Feb. 1, 1980) |
@article{Eckstein_1980, title={Computer simulation of the backscattering and implantation of hydrogen and helium}, volume={51}, ISSN={1089-7550}, url={http://dx.doi.org/10.1063/1.327687}, DOI={10.1063/1.327687}, number={2}, journal={Journal of Applied Physics}, publisher={AIP Publishing}, author={Eckstein, W. and Verbeek, H. and Biersack, J. P.}, year={1980}, month=feb, pages={1194–1200} }