Evolutionary transition between rapidly rotating compact stars after supernova explosion

N. Yasutake, M. Hashimoto, Y. Eriguchi, K. Arai

研究成果: Contribution to journalArticle査読

抄録

We propose a formation scenario of strange stars from rapidly rotating neutron stars after supernova explosions due to the spin-down of the compact stars. By considering a process where the total baryon mass is conserved but the angular momentum is lost due to the emission of gravitational waves and/or magnetic dipole radiation, we find that the transition from a rapidly rotating neutron star to a slowly rotating strange star is possible. The large amount of energy of 5 × 1053 ergs can be released, which is large by some factors compared to the transition between spherical stars. The liberated energy might become a new energy source for a delayed explosion of supernova. Thus our scenario suggests that the supernova associated with gamma-ray bursts becomes promising targets of future observation of gravitational waves.

本文言語英語
ページ(範囲)43-46
ページ数4
ジャーナルNuclear Physics A
758
1-4 SPEC. ISS.
DOI
出版ステータス出版済み - 7 25 2005

All Science Journal Classification (ASJC) codes

  • 核物理学および高エネルギー物理学

フィンガープリント

「Evolutionary transition between rapidly rotating compact stars after supernova explosion」の研究トピックを掘り下げます。これらがまとまってユニークなフィンガープリントを構成します。

引用スタイル