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Physics of Particles and Nuclei

, Volume 39, Issue 7, pp 1122–1127 | Cite as

Warm dense matter in giant planets and exoplanets

  • N. Nettelmann
  • R. Redmer
  • D. Blaschke
Part 3. Applications in Astrophysics

Abstract

Interior models of giant planets are strongly connected with properties of hydrogen under extreme conditions. We present a detailed description of the modeling procedure and discuss results for Jupiter and Saturn.

PACS numbers

96.15.De 

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Copyright information

© Pleiades Publishing, Ltd. 2008

Authors and Affiliations

  • N. Nettelmann
    • 1
  • R. Redmer
    • 1
  • D. Blaschke
    • 2
    • 3
  1. 1.Institute of PhysicsUniversity of RostockRostockGermany
  2. 2.Joint Institute for Nuclear ResearchDubnaRussia
  3. 3.Theory Division, GSI DarmstadtDarmstadtGermany

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