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Electronic conduction in shock-compressed water

  • P. M. Celliers
  • , G. W. Collins
  • , D. G. Hicks
  • , M. Koenig
  • , E. Henry
  • , A. Benuzzi-Mounaix
  • , D. Batani
  • , D. K. Bradley
  • , L. B. Da Silva
  • , R. J. Wallace
  • , S. J. Moon
  • , J. H. Eggert
  • , K. K.M. Lee
  • , L. R. Benedetti
  • , R. Jeanloz
  • , I. Masclet
  • , N. Dague
  • , B. Marchet
  • , M. Rabec
  • , Le Gloahec
  • Ch Reverdin, J. Pasley, O. Willi, D. Neely, C. Danson
  • Lawrence Livermore National Laboratory
  • LULI
  • Università di Milano-Bicocca
  • University of California, Berkeley
  • CEA/DAM
  • Imperial College London
  • Central Laser Facility

Résultats de recherche: Contribution à un journalArticleRevue par des pairs

Résumé

The optical reflectance of a strong shock front in water, which increases with pressure above 100 GPa, was discussed. The water Hugoniot equation of state up to 790 GPa was also determined. The shock velocity measurements, made by detecting the Doppler shift of reflected light, were used for the purpose. It was found from a fit to the reflectance data, that an electronic mobility gap ∼2.5 eV controls thermal activation of electronic carriers at pressures in the range of 100-150 GPa. The results show that above 150 GPa, electronic conduction contributes significantly to the total conductivity along the Neptune isentrope.

langue originaleAnglais
Pages (de - à)L41-L44
journalPhysics of Plasmas
Volume11
Numéro de publication8
Les DOIs
étatPublié - 1 août 2004

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