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Warm dense matter in giant planets and exoplanets

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.

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Nettelmann, N., Redmer, R. & Blaschke, D. Warm dense matter in giant planets and exoplanets. Phys. Part. Nuclei 39, 1122–1127 (2008). https://doi.org/10.1134/S1063779608070277

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  • DOI: https://doi.org/10.1134/S1063779608070277

PACS numbers

  • 96.15.De