Insulator-to-Conducting Transition in Dense Fluid Helium

P. M. Celliers, P. Loubeyre, J. H. Eggert, S. Brygoo, R. S. McWilliams, D. G. Hicks, T. R. Boehly, R. Jeanloz, and G. W. Collins
Phys. Rev. Lett. 104, 184503 – Published 5 May 2010
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Abstract

By combining diamond-anvil-cell and laser-driven shock wave techniques, we produced dense He samples up to 1.5g/cm3 at temperatures reaching 60 kK. Optical measurements of reflectivity and temperature show that electronic conduction in He at these conditions is temperature-activated (semiconducting). A fit to the data suggests that the mobility gap closes with increasing density, and that hot dense He becomes metallic above 1.9g/cm3. These data provide a benchmark to test models that describe He ionization at conditions found in astrophysical objects, such as cold white dwarf atmospheres.

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  • Received 12 November 2009

DOI:https://doi.org/10.1103/PhysRevLett.104.184503

©2010 American Physical Society

Authors & Affiliations

P. M. Celliers1, P. Loubeyre2, J. H. Eggert1, S. Brygoo2, R. S. McWilliams3,5, D. G. Hicks1, T. R. Boehly4, R. Jeanloz5, and G. W. Collins1

  • 1Lawrence Livermore National Laboratory, Post Office Box 808, Livermore, California 94551, USA
  • 2CEA/DAM/DIF, 91297 Arpajon. France
  • 3Institute for Shock Physics, Washington State University, Pullman, Washington 99164, USA
  • 4Laboratory for Laser Energetics, University of Rochester, Rochester, New York 14623, USA
  • 5University of California, Berkeley, California 94720, USA

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Issue

Vol. 104, Iss. 18 — 7 May 2010

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