Results of an ab initio investigation of the pressure dependence of the Raman-active phonon modes in the {β}-Sn phase of Si, Ge, and Sn and the hexagonal-close-packed phase of Si are presented. The calculations are in very good agreement with experimental measurements. Both measurements and calculations show that the {β}-Sn-structure LO mode has a different pressure dependence for Ge than for Si. This difference between Si and Ge is discussed, and an explanation in terms of d electrons is given.
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Lewis et al. (1993) studied this question.
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