Structure, Bonding, and Geochemistry of Xenon at High Pressures

Author:

Caldwell Wendel A.123,Nguyen Jeffrey H.123,Pfrommer Bernd G.123,Mauri Francesco123,Louie Steven G.123,Jeanloz Raymond123

Affiliation:

1. W. A. Caldwell and R. Jeanloz, Department of Geology and Geophysics, University of California, Berkeley, CA 94720, USA.

2. J. H. Nguyen, Department of Physics, University of California, Berkeley, CA 94720, USA.

3. B. G. Pfrommer, F. Mauri, S. G. Louie, Department of Physics, University of California, Berkeley, CA 94720, USA, and Materials Sciences Division, Lawrence Berkeley National Laboratory, Berkeley, CA 94720, USA.

Abstract

Although xenon becomes metallic at pressures above about 100 gigapascals, a combination of quantum mechanical calculations and high pressure–temperature experiments reveals no tendency on the part of xenon to form a metal alloy with iron or platinum to at least 100 to 150 gigapascals. The transformation of xenon from face-centered cubic (fcc) to hexagonal close-packed (hcp) structures is kinetically hindered, the differences in volume and bulk modulus between the two phases being smaller than we can resolve (less than 0.3 percent and 0.6 gigapascals, respectively). The equilibrium fcc-hcp phase boundary is at 21 (±3) gigapascals, which is a lower pressure than was previously thought, and it is unlikely that Earth's core serves as a reservoir for primordial xenon.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

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