Attenuation of ^3P_2-Superfluidity in Neutron Star Matter Due to Charged-Pion Condensation
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概要
- 論文の詳細を見る
It is investigated how the ^3P_2-type superfluidity of the main baryonic component in neutron star interior is affected by the occurrence of charged-pion condensation. Notable attenuation effect is found in a simple model calculation.
- 理論物理学刊行会の論文
- 1980-12-25
著者
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TAMAGAKI Ryozo
Department of Physics, Kyoto University
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Tamagaki Ryozo
Department Of Physcis Kyoto University
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Takatsuka Tatsuyuki
College Of Humanities And Social Sciences Iwate University
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Takatsuka Tatsuyuki
College Of Humaniteis And Social Sciences Iwate University
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