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Modeling giant planets and brown dwarfs

Published online by Cambridge University Press:  10 November 2011

Andreas Becker ,
Nadine Nettelmann ,
Ulrike Kramm ,
Winfried Lorenzen ,
Martin French  and
Ronald Redmer
Andreas Becker
Affiliation:
Institute of Physics, University of Rostock, Universitätsplatz 3, 18051, Rostock, Germany email: [email protected]
Nadine Nettelmann
Affiliation:
Dept. of Astronomy & Astrophysics, University of California, CA 95064 Santa Cruz, USA
Ulrike Kramm
Affiliation:
Institute of Physics, University of Rostock, Universitätsplatz 3, 18051, Rostock, Germany email: [email protected]
Winfried Lorenzen
Affiliation:
Institute of Physics, University of Rostock, Universitätsplatz 3, 18051, Rostock, Germany email: [email protected]
Martin French
Affiliation:
Institute of Physics, University of Rostock, Universitätsplatz 3, 18051, Rostock, Germany email: [email protected]
Ronald Redmer
Affiliation:
Institute of Physics, University of Rostock, Universitätsplatz 3, 18051, Rostock, Germany email: [email protected]
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Abstract

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We present new results in modeling the interiors of Giant Planets (GP) and Brown Dwarfs (BD). In general models of the interior rely on equation of state data for planetary materials which have considerable uncertainties in the high-pressure domain. Our calculations are based on ab initio equation of state (EOS) data for hydrogen, helium, hydrogen-helium mixtures and water as the representative of all heavier elements or ices using finite-temperature density functional theory molecular dynamics (FT-DFT-MD) simulations. We compare results for the BD Gliese 229B calculated with Saumon-Chabrier-Van Horn EOS (SCVH95) and our EOS data.

Keywords

equation of stateplanetary systemsbrown dwarfs
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 6 , Symposium S276: The Astrophysics of Planetary Systems: Formation, Structure, and Dynamical Evolution , October 2010 , pp. 473 - 474
Copyright
Copyright © International Astronomical Union 2011

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