Crystal structure solution of a high-pressure polymorph of scintillating MgMoO4 and its electronic structure
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Identificadores
URI: https://hdl.handle.net/10902/27721ISSN: 1098-0121
ISSN: 1550-235X
ISSN: 2469-9950
ISSN: 2469-9969
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Ruiz Fuertes, Javier
; Friedrich, A.; Garg, N.; Monteseguro Padrón, Virginia
; Radacki, K.; Errandonea, D.; Cavalli, E.; Rodríguez-Hernández, P.; Muñoz, A.
Fecha
2022Derechos
© American Physical Society
Publicado en
Physical Review B, 2022, 106, 064101
Editorial
American Physical Society
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Resumen/Abstract
The structure of the potentially scintillating high-pressure phase of  [Beta] - MgMoO 4  ( γ - MgMoO 4 ) has been solved by means of high-pressure single-crystal x-ray diffraction. The phase transition occurs above 1.5 GPa and involves an increase of the Mo coordination from fourfold to sixfold accommodated by a rotation of the polyhedra and a concommitant bond stretching resulting in an enlargement of the  c  axis. A previous high-pressure Raman study had proposed such changes with a symmetry change to space group  P 2 / c . Here it has been found that the phase transition is isosymmetrical ( C 2 / m -> C 2 / m ). The bulk moduli and the compressibilities of the crystal axes of both the low- and the high-pressure phase, have been obtained from equation of state fits to the pressure evolution of the unit-cell parameters which were obtained from powder x-ray diffraction up to 12 GPa. The compaction of the crystal structure at the phase transition involves a doubling of the bulk modulus  B 0  changing from 60.3(1) to 123.7(8) GPa and a change of the most compressible crystal axis from the (0,  b , 0) direction in  [Beta] - MgMoO 4  to the ( 0.9 a , 0,  0.5 a ) direction in  γ - MgMoO 4 . The lattice dynamical calculations performed here on  γ - MgMoO 4  served to explain the Raman spectra observed for the high-pressure phase of  [Beta] - MgMoO 4  in a previous work demonstrating that the use of internal modes arguments in which the  MoO n  polyhedra are considered as separate vibrational units fails at least in this molybdate. The electronic structure of  γ - MgMoO 4  was also calculated and compared with the electronic structures of  [Beta] - MgMoO 4  and  MgWO 4  shedding some light on why  MgWO 4  is a much better scintillator than any of the phases of  MgMoO 4 . These calculations yielded for  γ - MgMoO 4  a  Y 2 Γ -> Γ  indirect band gap of 3.01 eV in contrast to the direct bandgaps of  [Beta] - MgMoO 4  (3.58 eV at  Γ ) and  MgWO 4  (3.32 eV at  Z ).
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