Phys. Chem. Minerals., 25, 401-414, 1998

High-temperature X-ray diffraction and Raman spectroscopy of diopside and pseudowollastonite

Pascal Richet 1,
Bjorn O. Mysen
2 and Jannick Ingrin 3*


1 Laboratoire des Géomatériaux, URA 734 CNRS

Institut de Physique du Globe, 4 place Jussieu, 75252 Paris cedex 05, France

2 Geophysical Laboratory, Carnegie Institution of Washington, 5251 Broad Branch Rd, NW
Washington, DC, 20015-1305, USA

and NSF-sponsored Center for High-Pressure Research (CHiPR)

3 Laboratoire de Géophysique et Géodynamique Interne, URA CNRS 1369, Université Paris-Sud, 91405 Orsay, France

* Present address: Laboratoire des mécanismes de transfert en géologie, UMR CNRS 5563, 39 allée Jules Guesde, 31400 Toulouse, France

Abstract

Diopside (CaMgSi2O6) and pseudowollastonite (CaSiO3) have been studied by X-ray powder diffraction and Raman spectroscopy up to their respective melting points. In agreement with previous unit-cell parameters determinations below 1100 K, thermal expansion of diopside along the a and c axis is much smaller than along the b axis. For pseudowollastonite, the axis expansivity increases slightly in the order b > a > c. For both minerals, the change in unit-cell angles are very small. There are no anomalous variations of the other unit-cell parameters near the melting point. With increasing temperatures, the main changes observed in the Raman spectra are strong increases of the linewidths for those bands which involve Si-O-Si bending (near 600 cm-1) or represent mainly Ca-O or Mg-O stretching, in the range 270-500 cm-1 for diopside, and 240-450 cm-1 for pseudowollastonite. At temperatures near the onset of calorimetric premelting effects, this extensive band widening results in a broad Raman feature that can no longer be deconvoluted into its individual components. No significant changes affect the Si-O stretching modes. For both diopside and pseudowollastonite, premelting thus appears to be associated with enhanced dynamics of the alkaline-earth elements. This conclusion contrasts markedly with that drawn for sodium metasilicate in which weaker bonding of sodium allows the silicate framework to distort and deform in such a way as to prefigure the silicate entities present in the melt.

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[1], [2], [3], [4],
[5], [6], [7], [8], [9], [10], [11], [12], [13], [14], [15], [16], [17], [18],
[19], [20], [21], [22], [23], [24], [25]

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Copyright 2002, Geophysical Laboratory, Washington, DC.
http://gl.ciw.edu. June 2002.

Email: mysen@gl.ciw.edu