Statistical model of sphalerite structured quaternary A1−xBxYyZ1−y systems

Abstract Tetrahedron coordinated sphalerite quaternary systems of type A 1− x B x Y y Z 1− y consist exclusively of binary and ternary elemental tetrahedra, 4 of the first and 4 of the latter, each 1 with 3 configurations, i.e., a total of 16 elemental tetrahedron configurations. These configurations cannot contain all four constituent atoms simultaneously in the same elemental tetrahedron; as a consequence we can consider each ternary tetrahedron composition as diluted in the quaternary compound. Thus, A 1− x B x Y y Z 1− y extended X-ray absorption fine structure (EXAFS) data can be treated by using the strained tetrahedron model which, originally developed to deal with ternary systems, has already exhibited excellent agreement with numerous experimental data. To determine ion site occupation preferences of quaternary systems, we applied this model to our EXAFS data for Cd 1− x Mn x Se y Te 1− y and to Ga x In 1− x As y Sb 1− y data available in the literature, and compared them to those derived from ternary data for Cd 1− x Mn x Te and Ga x In 1− x As. In both sets, as the ternary is diluted in the quaternary system, a drift of the preference values of the pure ternary is observed. The present analysis of experimental reflectivity far-infrared (FIR) phonon spectra of quaternary Cd 1− x Mn x Se y Te 1− y crystals confirms the model predictions and leads to an interpretation of the experimental data for A 1− x B x Y y Z 1− y quaternary systems.