Implications of the Discovery of a Millisecond Pulsar in SN 1987A
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概要
- 論文の詳細を見る
From the observation of a millisecond pulsar in SN 1987A, the following implications are obtained. 1)The pulsar spindown in SN 1987A is caused by radiating gravitational waves rather than by magnetic dipole radiation and/or relativistic pulsar winds. 2)A mildly deformed shock wave would be formed at the core-collapse and explosion in SN 1987A, which is consistent with the conclusion given in Nagataki (2000). 3)The gravitational waves from the pulsar should be detected in several years using a Fabry-Perot-Michelson interferometer as the gravitational detector, such as LIGO and TAMA. 4)The neutrino oscillation model is not a promising model for the explanation of the kick velocity of the pulsar in SN 1987A. The hydrodynamical instability model is more favored.
- 理論物理学刊行会の論文
- 2001-03-25
著者
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SATO Katsuhiko
Department of Physics, Kyoto University
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Nagataki Shigehiro
Department Of Physics School Of Science The University Of Tokyo
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Nagataki Shigehiro
Department Of Phisics University Of Tokyo
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Sato Katsuhiko
Department Of Cardiovascular Medicine Hokkaido University School Of Medicine
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Sato Katsuhiko
Department Of Physics School Of Science University Of Tokyo:research Center For The Early Universe School Of Science University Of Tokyo
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SATO Katsuhiko
Department of Physics, School of Science, University of Tokyo:Research Center for the Early Universe, School of Science, University of Tokyo
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NAGATAKI Shigehiro
Department of Physics, School of Science, University of Tokyo
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NAGATAKI Shigehiro
Department of Phisics, University of Tokyo
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