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Crater formation by fast ions: comparison of experiment with Molecular Dynamics simulations

E. M. Bringa·R. E. Johnson·R. M. Papaleo
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Abstract

An incident fast ion in the electronic stopping regime produces a track of excitations which can lead to particle ejection and cratering. Molecular Dynamics simulations of the evolution of the deposited energy were used to study the resulting crater morphology as a function of the excitation density in a cylindrical track for large angle of incidence with respect to the surface normal. Surprisingly, the overall behavior is shown to be similar to that seen in the experimental data for crater formation in polymers. However, the simulations give greater insight into the cratering process. The threshold for crater formation occurs when the excitation density approaches the cohesive energy density, and a crater rim is formed at about six times that energy density. The crater length scales roughly as the square root of the electronic stopping power, and the crater width and depth seem to saturate for the largest energy densities considered here. The number of ejected particles, the sputtering yield, is shown to be much smaller than simple estimates based on crater size unless the full crater morphology is considered. Therefore, crater size can not easily be used to estimate the sputtering yield.

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E. M. Bringa, R. E. Johnson, R. M. Papaleo. 2001-05-16. Crater formation by fast ions: comparison of experiment with Molecular Dynamics simulations. https://doi.org/10.1103/physrevb.65.094113

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