Ba. Helmer et Db. Graves, MOLECULAR-DYNAMICS SIMULATIONS OF AR- DISTRIBUTIONS OF REFLECTED ENERGIES AND ANGLES( AND CL+ IMPACTS ONTO SILICON SURFACES ), Journal of vacuum science & technology. A. Vacuum, surfaces, and films, 16(6), 1998, pp. 3502-3514
Citations number
73
Categorie Soggetti
Physics, Applied","Materials Science, Coatings & Films
Previous profile evolution studies of plasma-assisted etch processes h
ave shown that ions scattered from sidewalls can lead to microtrench f
ormation on the bottom of an etched feature [see, for example, Dalton
ct al., J. Electrochem. Sec. 140, 2395 (1993)]. In these studies, the
ions impacting feature surfaces with incident angles above a critical
value were assumed to reflect specularly from the surfaces. In the pre
sent article, we describe the energy and angle distributions of reflec
ted atoms obtained from molecular dynamics (MD) simulations. We simula
ted Ar+ and Cl+ ions impacting model silicon surfaces. The ion inciden
t energies Ei were 20, 50, and 100 eV. We varied the ion incident angl
es theta(i) from 0 degrees to 85 degrees from the;surface normal. The
model silicon surfaces had chlorine coverages of 0 monolayers (ML) of
Cl, 1 ML Cl, and 2.3 ML Cl. We determined the Ar and Cl reflection pro
babilities, i.e., the fraction of Ar and Cl atoms scattered from the s
urfaces during the 1-2 ps MD trajectories. For theta(i) greater than o
r equal to 75 degrees, we found that the reflection probabilities were
greater than 90% in most cases. For these large incident angles, we d
escribe the distributions of energies E-r and angles (polar theta(r) a
nd azimuthal phi(r)) for the Ar and Cl atoms reflected from the surfac
es. The results of the MD simulations are compared with the assumption
of specular scattering. In addition, we compare the average energies
of the reflected atoms with the predictions of two simple models based
on the binary collision approximation. We discuss the effects of inci
dent ion species, E-i, theta(i), chlorine surface coverage, and surfac
e roughness on these results. (C) 1998 American Vacuum Society. [S0734
-2101(98)04506-0].