HR: 10:50h
AN: V21E-03 [PDF]
TI: A statistical approach to atomistic simulation of geophysical solid solutions
AU: Bukowinski, M S
EM: markb@socrates.berkeley.edu
AF: Earth & Planetary Science, UC Berkeley, Berkeley, CA 94720 United States
AU: * Akber-Knutson, S
EM: sofia@eps.berkeley.edu
AF: Earth & Planetary Science, UC Berkeley, Berkeley, CA 94720 United States
AB:
Many materials of geophysical importance are solid solutions rather
than pure minerals. Mascropic modeling of the thermodynamic properties
of these minerals often necessitates ideal mixing assumptions. While
atomistic models make it possible to model solid solutions without the
ideal mixing approximation, such calculations were not computationally
feasible until recently. Nevertheless, no convenient methodology for
studying the configurational aspects of geophysical solid solutions
currently exists, especially for the high temperatures of the earth.
We introduce a technique for studying solid solutions at high
temperature and apply it to the MgSiO$_3$-Al$_2$O$_3$-MgO system at
lower mantle conditions. We use a statistical mechanics based
approach that samples calculated Gibbs free energies of the solid
solutions corresponding to different, and often very numerous, mixing
configurations ({\em i.e.} ways to arrange atoms in mixing
sites). Vibrational contributions to the Gibbs free energies are
calculated from phonon spectra calculated under the quasiharmonic
approximation. We then use the sampled configurational free energies to
estimate configurational thermodynamic properties of the solid
solutions.
We first discuss the choice of an appropriate unit cell size that
properly samples a space of mixing configurations and avoids imposing
artificial ordering. We then compare Boltzmann-derived entropies of
mixing with those resulting from ideal mixing. We also discuss the
role of configurational heat capacity on the energetics of solid
solutions at high temperatures. Finally, we introduce a technique for
approximating configurational high temperature thermodynamic
properties of solid solutions from 0 Kelvin energy distributions (over
mixing configurations). Combining these results with only a few high
temperature configurations greatly reduces the number of computations
necessary to determine the full high temperature thermodynamic
properties of complex mineral assemblages.
DE: 3210 Modeling
SC: Volcanology, Geochemistry, Petrology [V]
MN: 2003 Fall Meeting