Warm dense matter in giant planets and exoplanets

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.

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Bibliographische Detailangaben
Veröffentlicht in:	Physics of particles and nuclei 2008-12, Vol.39 (7), p.1122-1127
Hauptverfasser:	Nettelmann, N., Redmer, R., Blaschke, D.
Format:	Artikel
Sprache:	eng
Schlagworte:	ASTROPHYSICS, COSMOLOGY AND ASTRONOMY HYDROGEN JUPITER PLANET Part 3. Applications in Astrophysics Particle and Nuclear Physics Physics Physics and Astronomy SATURN PLANET SIMULATION WARM DENSE MATTER
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Beschreibung
Zusammenfassung:	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.
ISSN:	1063-7796 1531-8559
DOI:	10.1134/S1063779608070277