Thermal Evolution of Neutron Stars--Current Status (ハドロン物質の諸相と中性子星の熱的進化(研究会報告))

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概要

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• Our recent work on thermal evolution of neutron stars is introduced. We start by presenting the results of our pion cooling calculations. We carry out calculations for other various non-standard cooling scenarios and the results are compared. Next we summarize the results of our work on frictional heating. Our theoretical models are then compared with the currently up-dated observational data. Very recently we started our investigation of the effects of magnetic fields on thermal properties of neutron stars, mainly in the form of temperature modulation over the stellar surface due to the anisotropic electron and photon conductivities under strong, quantized magnetic fields. Our preliminary results are summarized.

• 素粒子論グループ 素粒子研究編集部の論文
• 1993-11-20

著者

• 鶴田 幸子

  Montana州立大

• 鶴田 幸子

  Montana State Univ. Dep. Of Physics

関連論文

• Thermal Evolution of Neutron Stars--Current Status (ハドロン物質の諸相と中性子星の熱的進化(研究会報告))
• 中性子星の冷却(高密度核物質と中性子星の現象,研究会報告)
• 極東における古代および中世天文学の現代天文学への影響

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