HIGH-PRESSURE RAMAN SPECTROSCOPIC STUDY OF CO- AND NI-OLIVINES

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dc.contributor.author Lin C.C.
dc.date.accessioned 2021-03-03T07:11:21Z
dc.date.available 2021-03-03T07:11:21Z
dc.date.issued 2001
dc.identifier https://elibrary.ru/item.asp?id=13712074
dc.identifier.citation Physics and Chemistry of Minerals, 2001, 28, 4, 249-257
dc.identifier.issn 0342-1791
dc.identifier.uri https://repository.geologyscience.ru/handle/123456789/26203
dc.description.abstract The Raman spectra of synthetic α-Co2SiO4 and α-Ni2SiO4 olivines have been studied at room temperature and various pressures. All the Raman frequencies of the two olivines increase with increasing pressure, and most of the frequency–pressure plots obtained under both quasi- and nonhydrostatic conditions are nonlinear. It has been found that the average pressure derivative of Raman frequencies of the lattice modes in both Co- and Ni-olivines is smaller than that of the internal modes of SiO4, indicating that the distortion of SiO4 tetrahedra under static compression may be more severe than that of MO6 octahedra. In addition, four new Raman bands were observed in Ni-olivine under nonhydrostatic compression and above 30 GPa. This result suggests that a new phase of Ni-olivine should be formed at 30 GPa or amorphization may occur at still higher pressure.
dc.title HIGH-PRESSURE RAMAN SPECTROSCOPIC STUDY OF CO- AND NI-OLIVINES
dc.type Статья


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