Abstract
α-Sb2O3 (senarmontite), β-Sb2O3 (valentinite), and α-TeO2 (paratellurite) are compounds with pronounced stereochemically active Sb and Te lone pairs. The vibrational and lattice properties of each have been previously studied but often lead to incomplete or unreliable results due to modes being inactive in infrared or Raman spectroscopy. Here, we present a study of the relationship between bonding and lattice dynamics of these compounds. Mössbauer spectroscopy is used to study the structure of Sb in α-Sb2O3 and β-Sb2O3, whereas the vibrational modes of Sb and Te for each oxide are investigated using nuclear inelastic scattering, and further information on O vibrational modes is obtained using inelastic neutron scattering. Additionally, vibrational frequencies obtained by density functional theory (DFT) calculations are compared with experimental results in order to assess the validity of the utilized functional. Good agreement was found between DFT-calculated and experimental density of phonon states with a 7% scaling factor. The Sb-O-Sb wagging mode of α-Sb2O3 whose frequency was not clear in most previous studies is experimentally observed for the first time at ∼340 cm-1. Softer lattice vibrational modes occur in orthorhombic β-Sb2O3 compared to cubic α-Sb2O3, indicating that the antimony bonds are weakened upon transforming from the molecular α phase to the layer-chained β structure. The resulting vibrational entropy increase of 0.45 ± 0.1 kB/Sb2O3 at 880 K accounts for about half of the α-β transition entropy. The comparison of experimental and theoretical approaches presented here provides a detailed picture of the lattice dynamics in these oxides beyond the zone center and shows that the accuracy of DFT is sufficient for future calculations of similar material structures.
Original language | English |
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Pages (from-to) | 7869-7880 |
Number of pages | 12 |
Journal | Journal of Physical Chemistry A |
Volume | 124 |
Issue number | 39 |
DOIs | |
State | Published - Oct 1 2020 |
Funding
We thank Drs. Lucas Lindsay, Valentino Cooper, and Thomas Watkins for reviewing the manuscript, Dr. Elizabeth Sobalvarro Converso and Prof. Peter Khalifah for the provision of SbO powder, and Dr. Ronnie Simon for help with valentinite synthesis. Material synthesis work by C.A.B. and INS work by R.P.H., M.E.M., and D.H.M., and Mössbauer spectral work by R.P.H. was supported by the US Department of Energy, Office of Science, Office of Basic Energy Sciences, Materials Sciences and Engineering Division. Work by L.L.D. (INS and synthesis), Y.C., and A.J.R.C. (INS) was supported by the United States Department of Energy, Office of Science, Office of Basic Energy Sciences, Scientific User Facilities Division, both under Contract Number DE-AC05-00OR22725. We are grateful to the Helmholtz Association of German Research Centres and the Russian Academy of Sciences for supporting the projects HRJRG-402 “Sapphire ultra-optics for synchrotron radiation” and DFG SFB-917 “Nanoswitches”. We thank Mr. Jean-Philippe Celse for technical assistance during data acquisition at ID18. We acknowledge the ESRF for the provision of synchrotron radiation beamtime at ID18 and DESY for the provision of synchrotron beamtime at P01. A portion of this research (INS at VISION) used resources at the Spallation Neutron Source, a DOE Office of Science User Facility operated by Oak Ridge National Laboratory. 2 5
Funders | Funder number |
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U.S. Department of Energy | DE-AC05-00OR22725 |
Office of Science | |
Basic Energy Sciences | |
Division of Materials Sciences and Engineering | |
Deutsche Forschungsgemeinschaft | SFB-917 |
Russian Academy of Sciences | HRJRG-402 |
Helmholtz Association |