Properties of Planetary Fluids at High Shock Pressures and Temperatures-Reference-Cited by-同舟云学术

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Properties of Planetary Fluids at High Shock Pressures and Temperatures

Published:2013-03-18 Issue: Volume: Page:387-391
ISSN:2328-8779
Container-title:High-Pressure Research: Application to Earth and Planetary Sciences
language:
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Author:

Nellis W. J.,Mitchell A. C.,Holmes N. C.,Mccandless P. C.

Publisher

American Geophysical Union

Link

http://onlinelibrary.wiley.com/wol1/doi/10.1029/GM067p0387/fullpdf

Reference20 articles.

1. Metallization of solid hydrogen at megabar pressures: a first-principles quasiparticle study;Chacham;Phys. Rev. Lett.,1991

2. Band gap closure and metallization of molecular solid hydrogen;Garcia;Europhys. Lett.,1990

3. Models of Uranus and Neptune with partially mixed envelopes;Gudkova;Astron. Vestn.,1988

4. Electrical conductivity and equation of state of shock-compressed liquid oxygen;Hamilton;J. Chem. Phys.,1988

5. Structure and evolution of Uranus and Neptune;Hubbard;J. Geophys. Res.,1980

Cited by 1 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Static compression experiments on low-Z planetary materials;Geophysical Monograph Series;1998

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