Reynard, B;
Price, GD;
(1990)
Thermal expansion of mantle minerals at high pressures - A theoretical study.
Geophysical Research Letters
, 17
(6)
689 - 692.
10.1029/GL017i006p00689.
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Abstract
Recent experimental work has shown that the pressure dependence of the thermal expansion coefficient can be expressed as: ( α / α 0 ) = ( ρ / ρ 0 ( - δ T ( 1 ) where δ_{T}, the Anderson‐Gruneisen parameter, is assumed to be independent of pressure, and for the materials studied has a value that lies between 4 and 6. Calculation of δ_{T} from seismic data, however, appears to suggest a contradictory value of between 2 and 3 for mantle‐forming phases. Using an atomistic model based on our previously successful many‐body interatomic potential set (THBl), we have performed calculations to obtain values of δ_{T} for four major mantle‐forming minerals. Our model results are in excellent agreement with experimental data, yielding values of between 4 and 6 for forsterite and MgO, and values in the same range for MgSiO_{3-}perovskite and γ‐Mg_{2}SiO_{4}. Moreover, the calculations confirm that δ_{T} is indeed constant with pressure up to the core‐mantle boundary. The apparent conflict between the values of δ_{T} predicted from seismic data and those obtained from experiment, and now from theory, is discussed.
Type: | Article |
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Title: | Thermal expansion of mantle minerals at high pressures - A theoretical study |
Open access status: | An open access version is available from UCL Discovery |
DOI: | 10.1029/GL017i006p00689 |
Publisher version: | http://dx.doi.org/10.1029/GL017i006p00689 |
Language: | English |
Additional information: | Copyright 1990 by the American Geophysical Union |
UCL classification: | UCL |
URI: | https://discovery.ucl.ac.uk/id/eprint/99140 |
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