Phase Transition of Color Superconductivity and Cooling Behavior of Quark Stars
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概要
- 論文の詳細を見る
We discuss color superconductivity and its effect on the cooling behavior of strange quark stars. The neutrino emissivity and specific heat of quark matter are calculated within the BCS theory. In the superconducting phase, the emissivity decreases and causes suppression of the cooling rate. It is shown that the phase transition leads to a sudden discontinuous suppression of the cooling rate in cooperation with the specific heat.
- 理論物理学刊行会の論文
- 2002-01-25
著者
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IWASAKI Masaharu
Department of Physics, Kochi University
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YAMAGUCHI Keiji
Department of Emergency and Critical Care Medicine, School of Medicine Keio University
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Yamaguchi Keiji
Department Of Chemical Engineering Faculty Of Engineering University Of Tokyo
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Yamaguchi Keiji
Department Of Physics Hiroshima University
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Miyamura O
Hiroshima Univ. Higashi‐hiroshima Jpn
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Miyamura Osamu
Department Of Applied Mathematics Faculty Of Engineering Science Osaka University
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Miyamura Osamu
Department Of Physics Hiroshima University
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Iwasaki Masaharu
Department Of Material Science Kochi University
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Iwasaki Masaharu
Department Of Applied Mathematics Faculty Of Engineering Science Osaka University
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MIYAMURA Osamu
Physics Department, Hiroshima University
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MIYAMURA Osamu
Department of Physics, Hiroshima University
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YAMAGUCHI Keiji
Department of Physics, Hiroshima University
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