Relativistic Hartree-Bogoliubov Calculation of the Specific Heat for the Inner Crust of Neutron Stars(Nuclear Physics)
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概要
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We calculate the specific heat of the inner crust of neutron stars, which determines the cooling time, using a local-density approximation of an improved relativistic Hartree-Bogoliubov model. The non-uniformity of the system enhances the specific heat, especially at low temperatures. We examine a schematic interpolation between the results of Broglia et al., adopting the Gogny force, and ours, based on the Lagrangian of the relativistic mean-field model.
- 理論物理学刊行会の論文
- 2004-10-25
著者
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Nakano T
Department Of Physics Kyushu University:(present Address)sasaguri Town Office
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NAKANO Takuya
Department of Physics, Kyushu University
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MATSUZAKI Masayuki
Department of Physics, Fukuoka University of Education
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Matsuzaki M
Department Of Physics Fukuoka University Of Education
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Matsuzaki Masayuki
Department Of Physics Fukuoha University Of Education
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NAKANO Takuya
Department of Physics, Kyushu University:(Present Address)Sasaguri Town Office
関連論文
- Relativistic Hartree-Bogoliubov Calculation of the Specific Heat for the Inner Crust of Neutron Stars(Nuclear Physics)
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