The mechanism for the pressure-induced transformation of cristobalite to stishovite and post-stishovite phases has been obtained from constant pressure ab initio molecular dynamics simulations. The cristobalite to stishovite transformation is found to be a two step process where SiO4 tetrahedra first rotate followed by a lattice distortion to yield the six-coordinated stishovite structure. Further compression of stishovite yields the CaCl2 structure and is followed by another six-coordinated structure with symmetry P21/n (at 11 Mbars) which remains stable to a pressure of about 14 Mbars and then transforms into a nine-coordinated P21/m structure.

Klug, D., Rousseau, R., Uehara, K., Bernasconi, M., Le Page, Y., Tse, J. (2001). Ab initio molecular dynamics study of the pressure-induced phase transformations in cristobalite. PHYSICAL REVIEW. B, CONDENSED MATTER, 63(10), 1041061-1041065 [10.1103/PhysRevB.63.104106].

Ab initio molecular dynamics study of the pressure-induced phase transformations in cristobalite

BERNASCONI, MARCO;
2001

Abstract

The mechanism for the pressure-induced transformation of cristobalite to stishovite and post-stishovite phases has been obtained from constant pressure ab initio molecular dynamics simulations. The cristobalite to stishovite transformation is found to be a two step process where SiO4 tetrahedra first rotate followed by a lattice distortion to yield the six-coordinated stishovite structure. Further compression of stishovite yields the CaCl2 structure and is followed by another six-coordinated structure with symmetry P21/n (at 11 Mbars) which remains stable to a pressure of about 14 Mbars and then transforms into a nine-coordinated P21/m structure.
Articolo in rivista - Articolo scientifico
ab-iinitio simulations, silica, high pressure
English
2001
63
10
1041061
1041065
104106
none
Klug, D., Rousseau, R., Uehara, K., Bernasconi, M., Le Page, Y., Tse, J. (2001). Ab initio molecular dynamics study of the pressure-induced phase transformations in cristobalite. PHYSICAL REVIEW. B, CONDENSED MATTER, 63(10), 1041061-1041065 [10.1103/PhysRevB.63.104106].
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/10281/24564
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