First-principles equation of state calculations of warm dense nitrogen

K. P. Driver and B. Militzer
Phys. Rev. B 93, 064101 – Published 1 February 2016
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Abstract

Using path integral Monte Carlo (PIMC) and density functional molecular dynamics (DFT-MD) simulation methods, we compute a coherent equation of state (EOS) of nitrogen that spans the liquid, warm dense matter (WDM), and plasma regimes. Simulations cover a wide range of density-temperature space, 1.513.9gcm3 and 103109 K. In the molecular dissociation regime, we extend the pressure-temperature phase diagram beyond previous studies, providing dissociation and Hugoniot curves in good agreement with experiments and previous DFT-MD work. Analysis of pair-correlation functions and the electronic density of states in the WDM regime reveals an evolving plasma structure and ionization process that is driven by temperature and pressure. Our Hugoniot curves display a sharp change in slope in the dissociation regime and feature two compression maxima as the K and L shells are ionized in the WDM regime, which have some significant differences from the predictions of plasma models.

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  • Received 17 August 2015
  • Revised 8 December 2015

DOI:https://doi.org/10.1103/PhysRevB.93.064101

©2016 American Physical Society

Physics Subject Headings (PhySH)

Condensed Matter, Materials & Applied Physics

Authors & Affiliations

K. P. Driver1,* and B. Militzer1,2

  • 1Department of Earth and Planetary Science, University of California, Berkeley, California 94720, USA
  • 2Department of Astronomy, University of California, Berkeley, California 94720, USA

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Issue

Vol. 93, Iss. 6 — 1 February 2016

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