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Laser-driven shock experiments on precompressed water: Implications for "icy" giant planets

  • Kanani K.M. Lee
  • , L. Robin Benedetti
  • , Raymond Jeanloz
  • , Peter M. Celliers
  • , Jon H. Eggert
  • , Damien G. Hicks
  • , Stephen J. Moon
  • , Andrew Mackinnon
  • , Gilbert W. Collins
  • , Emeric Henry
  • , Michel Koenig
  • , Alessandra Benuzzi-Mounaix
  • University of California, Berkeley
  • New Mexico State University
  • Lawrence Livermore National Laboratory

Résultats de recherche: Contribution à un journalArticleRevue par des pairs

Résumé

Laser-driven shock compression of samples precompressed to 1 GPa produces high-pressure-temperature conditions inducing two significant changes in the optical properties of water: the onset of opacity followed by enhanced reflectivity in the initially transparent water. The onset of reflectivity at infrared wavelengths can be interpreted as a semiconductor ↔ electronic conductor transition in water, and is found at pressures above ∼ 130 GPa for single-shocked samples precompressed to 1 GPa. Our results indicate that conductivity in the deep interior of "icy" giant planets is greater than realized previously because of an additional contribution from electrons.

langue originaleAnglais
Numéro d'article014701
journalJournal of Chemical Physics
Volume125
Numéro de publication1
Les DOIs
étatPublié - 14 juil. 2006

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