Neutrino Energy Loss in Neutron Star Matter
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概要
- 論文の詳細を見る
The theory of the energy loss due to neutrino processes in neutron stars is formulated in such a form that one can include the effect of strong interaction systematically. As an application the rates of energy loss are calculated for the following cases of interest in the study of neutron stars; i) the neutron and the proton liquid are both normal, ii) the proton or iii) the neutron liquid is in the superfluid state. Our results largely confirm the earlier calculations by Bahcall and Wolf and by Wolf. The rate of energy loss in the state of nuclei coexisting with free neutrons is also discussed.
- 理論物理学刊行会の論文
- 1972-12-25
著者
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Itoh Naoki
Department Of Urology Sapporo Medical University
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Itoh Naoki
Department Of Biology Faculty Of Science Okayama University
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Itoh Naoki
Department Of Physics Kyoto University : Department Of Physics University Of Illinois
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TSUNETO Toshihiko
Department of Physics, Kyoto University
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Tsuneto Toshihiko
Department Of Physics Faculty Of Engineering Science Osaka University
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Itoh Naoki
Department of Physics, Kyoto University : Department of Physics, University of Illinois
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