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

被引:76
作者
Lee, Kanani K. M. [1 ]
Benedetti, L. Robin
Jeanloz, Raymond
Celliers, Peter M.
Eggert, Jon H.
Hicks, Damien G.
Moon, Stephen J.
Mackinnon, Andrew
Da Silva, Luis B.
Bradley, David K.
Unites, Walter
Collins, Gilbert W.
Henry, Emeric
Koenig, Michel
Benuzzi-Mounaix, Alessandra
Pasley, John
Neely, David
机构
[1] Univ Calif Berkeley, Dept Earth & Planetary Sci, Berkeley, CA 94720 USA
[2] New Mexico State Univ, Dept Phys, Las Cruces, NM 88003 USA
[3] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA
[4] Lawrence Livermore Natl Lab, Livermore, CA 94550 USA
[5] Ecole Polytech, Lab LULI, F-91128 Palaiseau, France
[6] Univ Calif San Diego, Energy Res Ctr, La Jolla, CA 92093 USA
[7] Rutherford Appleton Lab, Cent Laser Facil, Didcot OX11 0QX, Oxon, England
基金
美国国家科学基金会;
关键词
EQUATION-OF-STATE; ELECTRICAL-CONDUCTIVITY; MELTING CURVE; PRESSURE; GPA; COMPRESSION; H2O; AMMONIA; TEMPERATURE; HYDROGEN;
D O I
10.1063/1.2207618
中图分类号
O64 [物理化学(理论化学)、化学物理学];
学科分类号
070304 ; 081704 ;
摘要
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 similar to 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.
引用
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页数:7
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