Theoretical study of phase transitions in Sb2S3, Bi2S3 and Sb2Se3 under compression.

We report a theoretical study of Sb2S3, Sb2Se3 and Bi2S3 sesquichalcogenides at hydrostatic pressures up to 60 GPa. We explore the possibility that the R-3m, C2/m, C2/c and Im-3m phases observed in sesquichalcogenides with heavier cations, viz. Bi2Se3, Bi2Te3 and Sb2Te3, could also be formed in the former compounds as suggested by recent experiments. Our calculations show that the C2/m and C2/c phases are energetically unstable in any of the three compounds and over the entire range of pressures examined. In contrast, the disordered bcc-like Im-3m phase is energetically stable at high pressures, but only the Sb2Se3 phase does not show dynamical instabilities below 60 GPa. Our calculations show that the Pnma structure is the most energetically stable Sb2S3 and Bi2S3 phase at ambient pressure whereas, surprisingly, the R-3m phase of Sb2Se3 is predicted to have the lowest enthalpy energy at 0 GPa, in contradiction to experimental evidence. Our calculations show that both Pnma and R-3m phases are dynamical and mechanically stable at room pressure. These results suggest that the formation of the R-3m phase in Sb2Se3 could be feasible at close to ambient conditions. To aid its identification, we provide a theoretical crystal structure (lattice and atomic parameters) and complete infrared and Raman spectra for this phase.