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arXiv:astro-ph/0011363 (astro-ph)
[Submitted on 20 Nov 2000 (v1), last revised 14 Feb 2001 (this version, v3)]

Title:Implications of the Discovery of Millisecond Pulsar in SN 1987A

Authors:S. Nagataki, K. Sato
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Abstract: 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.
Comments: 8 pages. Accepted by Progress of Theoretical Physics after minor revisions
Subjects: Astrophysics (astro-ph)
Report number: UTAP-378/00, RESCEU-35/00
Cite as: arXiv:astro-ph/0011363
  (or arXiv:astro-ph/0011363v3 for this version)
  https://doi.org/10.48550/arXiv.astro-ph/0011363
Journal reference: Prog.Theor.Phys. 105 (2001) 429-436
Related DOI: https://doi.org/10.1143/PTP.105.429

Submission history

From: Nagataki Shigehiro [view email]
[v1] Mon, 20 Nov 2000 16:51:23 UTC (10 KB)
[v2] Sat, 2 Dec 2000 05:36:20 UTC (10 KB)
[v3] Wed, 14 Feb 2001 19:56:24 UTC (10 KB)
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