Characterizing the Structure of Giant Planets
Author:
Publisher
Wiley
Subject
Condensed Matter Physics
Link
http://onlinelibrary.wiley.com/wol1/doi/10.1002/ctpp.201300001/fullpdf
Reference42 articles.
1. Formation of the Giant Planets by Concurrent Accretion of Solids and Gas
2. Shock Compression of Deuterium and the Interiors of Jupiter and Saturn
3. The properties of hydrogen and helium under extreme conditions
4. Ab Initio Equation of State Data for Hydrogen, Helium, and Water and the Internal Structure of Jupiter
5. A Massive Core in Jupiter Predicted from First-Principles Simulations
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