Vibrations and Phase Stability in Mixed Valence Antimony Oxide

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Abstract

α-Sb2O4 (cervantite) and β-Sb2O4 (clinocervantite) are mixed valence compounds with equal proportions of SbIII and SbV as represented in the formula SbIIISbVO4. Their structure and properties can be difficult to calculate owing to the SbIII lone-pair electrons. Here, we present a study of the lattice dynamics and vibrational properties using a combination of inelastic neutron scattering, Mössbauer spectroscopy, nuclear inelastic scattering, and density functional theory (DFT) calculations. DFT calculations that account for lone-pair electrons match the experimental densities of phonon states. Mössbauer spectroscopy reveals the β phase to be significantly harder than the α phase. Calculations with O vacancies reveal the possibility for nonstoichiometric proportions of SbIII and SbV in both phases. An open question is what drives the stability of the α phase over the β phase, as the latter shows pronounced kinetic stability and lower symmetry despite being in the high-temperature phase. Since the vibrational entropy difference is small, it is unlikely to stabilize the α phase. Our results suggest that the α phase is more stable only because the material is not fully stoichiometric.

Original languageEnglish
Pages (from-to)16464-16474
Number of pages11
JournalInorganic Chemistry
Volume62
Issue number40
DOIs
StatePublished - Oct 9 2023

Funding

Neutron scattering work by D.H.M., M.E.M., and R.P.H. and calculations by R.J., V.R.C., and L.L. were supported by the U.S. Department of Energy (DOE), Office of Science, Office of Basic Energy Sciences (BES), Materials Sciences and Engineering Division. L.L.D. synthesized all samples and M.K.K. performed the TGA-MS analysis. TGA-MS analysis by M.K.K. was funded by the U.S. Department of Energy (DOE), Office of Science, Office of Basic Energy Sciences (BES), Chemical Sciences, Geosciences, & Biosciences (CSGB) Division. A portion of this research (INS at VISION, conducted with L.L.D. and Y.C.) used resources at the Spallation Neutron Source, supported by DOE, BES, Scientific User Facilities Division. We acknowledge DESY (Hamburg, Germany), a member of the Helmholtz Association (HGF), for the provision of experimental facilities. Parts of this research were carried out at PETRA-III at the P01 High Resolution Dynamics beamline (NIS, conducted with I.S., R.S., and O.L.). Beamtime was allocated for proposal I-20200912. The calculations used resources of the Compute and Data Environment for Science (CADES) at the Oak Ridge National Laboratory, which is supported by the DOE Office of Science under Contract no. DE-AC05-00OR22725, and resources of the National Energy Research Scientific Computing Center, which is supported by the DOE Office of Science under Contract no. DE-AC02-05CH11231. We acknowledge Dr. Ercan Cakmak for his assistance in collecting and analyzing powder X-ray diffraction data.

FundersFunder number
CADES
Chemical Sciences, Geosciences, & Biosciences
Data Environment for Science
U.S. Department of Energy
Office of ScienceDE-AC05-00OR22725
Basic Energy Sciences
Division of Materials Sciences and Engineering
Chemical Sciences, Geosciences, and Biosciences Division
National Energy Research Scientific Computing CenterDE-AC02-05CH11231
Helmholtz-Gemeinschaft
Helmholtz Association

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