Phase Transitions in the Newly-Born Neutron Star and Neutrino Emissions from SN1987A : Astrophysics and Relativity
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概要
- 論文の詳細を見る
We investigated the possibility that the last three events detected by Kamiokande-II can be explained by the phase transitions occurred in the neutron stars just born. We found that, if the equation of state of neutron stars is stiff enough, the last three neutrino events can be explained by the enhanced neutrino emission from the neutron star reheated by phase transitions.
- 理論物理学刊行会の論文
- 1988-11-25
著者
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TAKAHARA Mariko
Department of Physics, Kyoto University
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Takahara M
Doshisha Women's Coll. Liberal Arts Kyoto
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Takahara Mariko
Department Of Astronomy University Of Tokyo
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Sato Katsuhiko
Department Of Cardiovascular Medicine Hokkaido University School Of Medicine
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