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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
  • Department of Earth and Planetary Science
  • University of California, Berkeley
  • New Mexico State University
  • Physics Department
  • Lawrence Livermore National Laboratory

Research output: Contribution to journal › Article › peer-review

83 Citations (Scopus)

Abstract

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.

Original languageEnglish
Article number014701
JournalJournal of Chemical Physics
Volume125
Issue number1
DOIs
Publication statusPublished - 14 Jul 2006

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