Implications of the Discovery of Sub-Millisecond Pulsar in SN1987A : Astrophysics and Relativity
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概要
- 論文の詳細を見る
From the observation of the sub-millisecond pulsar in SN1987A the following implications are obtained. 1) The stiff equation of state of neutron star matter, such as Mean Field, Tensor Interaction, Bethe and Johnson I are ruled out. 2) The pulsar has a possibility to collapse into a black-hole by spin-down. 3) Although the sinusoidal modulation is explained by the existence of a 10^-3M_⦿ companion object, it seems hard to account for such an object in the scenario of the supernova explosion. We estimate the magnetic field, ellipticity and the mass of the neutron star and also the period of glitches.
- 理論物理学刊行会の論文
- 1989-05-25
著者
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鈴木 久男
北大理
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Sato Katsuhiko
Department Of Cardiovascular Medicine Hokkaido University School Of Medicine
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Suzuki Hideyuki
Department Of Biological Science And Technology Science University Of Tokyo
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Suzuki Hideyuki
Department Of Physics University Of Tokyo
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Suzuki Hideyuki
Department Of Bio-medical Engineering School Of High-technology For Human Welfare Tokai University
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SUZUKI Hisao
Institute of Physics, College of General Education Osaka University
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