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Pressure-induced optical anisotropy of HfS2

  • Igor Antoniazzi*
  • , Tomasz Woźniak
  • , Amit Pawbake
  • , Natalia Zawadzka
  • , Magdalena Grzeszczyk
  • , Zahir Muhammad
  • , Weisheng Zhao
  • , Jordi Ibáñez
  • , Clement Faugeras
  • , Maciej R. Molas
  • , Adam Babiński
  • *此作品的通讯作者
  • University of Warsaw
  • CNRS
  • National University of Singapore
  • Institute of Earth Sciences Jaume Almera, CSIC

科研成果: 期刊稿件文章同行评审

摘要

The effect of pressure on Raman scattering (RS) in bulk H f S 2 is investigated under hydrostatic and non-hydrostatic pressure conditions. The RS line shape does not change significantly in the hydrostatic regime up to P = 9.6 GPa, showing a systematic blueshift of the spectral features. In a non-hydrostatic environment, seven peaks appear in the spectrum at P = 7 GPa, which dominate the RS line shape up to P = 10.5 GPa. The change in the RS line shape manifests a pressure-induced phase transition in H f S 2 . The simultaneous observation of both low-pressure (LP) and high-pressure (HP) related RS peaks suggests the coexistence of two different phases over a wide pressure range. It is found that the HP-related phase is metastable and persists during the decompression cycle down to P = 1.2 GPa, while the LP-related features eventually recover at even lower pressure. The angle-resolved polarized RS performed under P = 7.4 GPa revealed a strong in-plane anisotropy of both the LP-related A 1 g mode and the HP peaks. The anisotropy is related to the possible distortion of the structure induced by the non-hydrostatic component of the pressure. The results are explained in terms of a distorted P n m a phase as a possible pressure-induced phase of H f S 2 .

源语言英语
文章编号035901
期刊Journal of Applied Physics
136
3
DOI
出版状态已出版 - 21 7月 2024

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