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    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/10902/27721
    DOI: 10.1103/PhysRevB.106.064101
    ISSN: 1098-0121
    ISSN: 1550-235X
    ISSN: 2469-9950
    ISSN: 2469-9969
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    Autoría
    Ruiz Fuertes, JavierAutoridad Unican; Friedrich, A.; Garg, N.; Monteseguro Padrón, VirginiaAutoridad Unican; Radacki, K.; Errandonea, D.; Cavalli, E.; Rodríguez-Hernández, P.; Muñoz, A.
    Fecha
    2022
    Derechos
    © American Physical Society
    Publicado en
    Physical Review B, 2022, 106, 064101
    Editorial
    American Physical Society
    Enlace a la publicación
    https://doi.org/10.1103/PhysRevB.106.064101
    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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    UNIVERSIDAD DE CANTABRIA

    Repositorio realizado por la Biblioteca Universitaria utilizando DSpace software
    Contacto | Sugerencias
    Metadatos sujetos a:licencia de Creative Commons Reconocimiento 4.0 España