1993
DOI: 10.1063/1.464361
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Pressure-induced amorphization of wollastonite (CaSiO3) at room temperature

Abstract: Energy dispersive x-ray diffraction and Raman measurements show that the mineral wollastonite (CaSiO3) becomes amorphous at a pressure of 25.6 GPa at 300 K. A consideration of the high pressure/high temperature behavior of CaSiO3 shows that the amorphization occurs because the phase transition wollastonite→perovskite CaSiO3 is kinetically impeded. We suggest that the amorphous phase may be viewed as a defective long-period modulated wollastonite phase.

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Cited by 36 publications
(14 citation statements)
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“…These hydrous minerals have thus similar pressure ranges of amorphization. Serghiou & Hammack (1993) observed near 26 GPa amorphization of wollastonite, CaSiO 3 , a pyroxenoid mineral which displays extensive polytypism. Without elaborating further, they suggested from X-ray diffraction experiments that amorphous CaSiO 3 can be considered as a defective long-period modulated wollastonite phase.…”
Section: Miscellaneous Mineralsmentioning
confidence: 95%
“…These hydrous minerals have thus similar pressure ranges of amorphization. Serghiou & Hammack (1993) observed near 26 GPa amorphization of wollastonite, CaSiO 3 , a pyroxenoid mineral which displays extensive polytypism. Without elaborating further, they suggested from X-ray diffraction experiments that amorphous CaSiO 3 can be considered as a defective long-period modulated wollastonite phase.…”
Section: Miscellaneous Mineralsmentioning
confidence: 95%
“…1a) except for diffraction lines of platinum and thus can be explained by pressure-induced * E-mail:yusa.hitoshi@nims.go.jp amorphization, as has been reported for silica (Hemley et al 1988) and silicates (Serghiou and Hammack 1993;Hemmati et al 1995). The diffraction pattern was an amorphous halo ( Fig.…”
Section: Resultsmentioning
confidence: 52%
“…At the same time, a close inspection of the Raman spectra for the second group of samples (see Fig. 4 ) detects an appearance of Ca–O local vibrational mode at about 336 and 412 cm −1 , and Raman features at 642 and 971 cm −1 corresponded the stretching vibration of the monomer SiO 4 and the stretching vibration of the chain SiO 4 tetrahedron, respectively [ 19 ]. These modes, as it is known [ 19 ], characterize the wollastonite form of CaSiO 3 .…”
Section: Resultsmentioning
confidence: 99%