Phonon density of states of Sn in textured SnO under high pressure: Comparison of nuclear inelastic x-ray scattering spectra to a shell model
- Department Physik, Universitaet Paderborn, D-33095 Paderborn (Germany)
- Instituto de Fisica Rosario, Universidad Nacional de Rosario, 27 de Febrero 210 Bis, 2000 Rosario (Argentina)
- APS, Argonne National Laboratory, Argonne, Illinois 60439 (United States)
- HP-CAT, Carnegie Institute of Washington, APS, Argonne, Illinois 60439 (United States)
The local phonon density of states (DOS) at the Sn site in tin monoxide (SnO) is studied at pressures up to 8 GPa with {sup 119}Sn nuclear resonant inelastic x-ray scattering (NRIXS) of synchrotron radiation at 23.88 keV. The preferred orientation (texture) of the SnO crystallites in the investigated samples is used to measure NRIXS spectra preferentially parallel and almost perpendicular to the c axis of tetragonal SnO. A subtraction method is applied to these NRIXS spectra to produce projected local Sn DOS spectra as seen parallel and perpendicular to the c axis of SnO. These experimentally obtained local Sn DOS spectra, both in the polycrystalline case as well as projected parallel and perpendicular to the c axis, are compared with corresponding theoretical phonon DOS spectra, derived from dispersion relations calculated with a recently developed shell model. Comparison between the experimental projected Sn DOS spectra and the corresponding theoretical DOS spectra enables us to follow the pressure-induced shifts of several acoustic and optic phonon modes. While the principal spectral features of the experimental and theoretical phonon DOS agree well at energies above 10 meV, the pressure behavior of the low-energy part of the DOS is not well reproduced by the theoretical calculations. In fact, they exhibit, in contrast to the experimental data, a dramatic softening of two low-energy modes, their energies approaching zero around 2.5 GPa, clearly indicating the limitations of the applied shell model. These difficulties are obviously connected with the complex Sn-O and Sn-Sn bindings within and between the Sn-O-Sn layers in the litharge structure of SnO. We derived from the experimental and theoretical DOS spectra a variety of elastic and thermodynamic parameters of the Sn sublattice, such as the Lamb-Moessbauer factor, the mean force constant, and Debye temperatures, as well as the vibrational contributions to the Helmholtz free energy, specific heat, entropy, and internal energy. We found, in part, good agreement between these values, for instance, for the Grueneisen parameters for some selected phonon modes, especially for some optical modes studied recently by Raman spectroscopy. We discuss in detail a possible anisotropy in the elastic parameters resulting from the litharge-type structure of SnO, for instance for the Lamb-Moessbauer factor, where we can compare with existing data from {sup 119}Sn-Moessbauer spectroscopy.
- OSTI ID:
- 20853635
- Journal Information:
- Physical Review. B, Condensed Matter and Materials Physics, Vol. 74, Issue 9; Other Information: DOI: 10.1103/PhysRevB.74.094303; (c) 2006 The American Physical Society; Country of input: International Atomic Energy Agency (IAEA); ISSN 1098-0121
- Country of Publication:
- United States
- Language:
- English
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Related Subjects
SUPERCONDUCTIVITY AND SUPERFLUIDITY
36 MATERIALS SCIENCE
ANISOTROPY
COMPARATIVE EVALUATIONS
DEBYE TEMPERATURE
DISPERSION RELATIONS
ELASTICITY
ENTROPY
FREE ENERGY
GRAIN ORIENTATION
KEV RANGE
LAYERS
MOESSBAUER EFFECT
OPTICAL MODES
PHONONS
POLYCRYSTALS
PRESSURE DEPENDENCE
PRESSURE RANGE GIGA PA
RAMAN SPECTRA
RAMAN SPECTROSCOPY
SHELL MODELS
SPECIFIC HEAT
SYNCHROTRON RADIATION
TEXTURE
TIN
TIN 119
TIN OXIDES
X-RAY DIFFRACTION