Ab initio simulations of hot dense methane during shock experiments

Benjamin L. Sherman, Hugh F. Wilson, Dayanthie Weeraratne, and Burkhard Militzer
Phys. Rev. B 86, 224113 – Published 28 December 2012
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Abstract

Using density functional theory molecular dynamics simulations, we predict shock Hugoniot curves of precompressed methane up to 75000 K for initial densities ranging from 0.35 to 0.70 gcm3. At 4000 K, we observe the transformation into a metallic, polymeric state consisting of long hydrocarbon chains. These chains persist when the sample is quenched to 300K, leading to an increase in shock compression. At 6000K, the sample transforms into a plasma composed of many, short-lived chemical species. We conclude by discussing implications for the interiors of Uranus and Neptune and analyzing the possibility of creating a superionic state of methane in high pressure experiments.

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  • Received 12 July 2012

DOI:https://doi.org/10.1103/PhysRevB.86.224113

©2012 American Physical Society

Authors & Affiliations

Benjamin L. Sherman1, Hugh F. Wilson2, Dayanthie Weeraratne1, and Burkhard Militzer2,3

  • 1Department of Geological Sciences, California State University Northridge, Northridge, California 91330, USA
  • 2Department of Earth and Planetary Science, University of California, Berkeley, California 94720, USA
  • 3Department of Astronomy, University of California, Berkeley, California 94720, USA

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Issue

Vol. 86, Iss. 22 — 1 December 2012

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