Nucleon Superfluidity in Neutron Star Core with Direct URCA Cooling
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概要
- 論文の詳細を見る
Nucleon superfluidity in a neutron star core with abundant protons making possible the direct URCA cooling is investigated using a realistic approach. It is found that the existence of both n- and p-superfluids is unlikely when the realistic effective mass of nucleons is taken into account. This leads to the conclusion that the direct URCA cooling would be excluded from the candidates of rapid cooling scenario of neutron stars and thereby constrain their masses.
- 理論物理学刊行会の論文
- 1997-02-25
著者
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TAMAGAKI Ryozo
Kyoto University
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TAMAGAKI Ryozo
Department of Physics, Kyoto University
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玉垣 良三
Kyoto University
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Takatsuka Tatsuyuki
Faculty Of Humanities And Social Sciences Iwate University
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