“Numerical relativity: Application to gravitational-wave science and astrophysics”

Collaborators

研究成果: Conference contribution

抄録

Neutron Star equation of State can be measured through • tidal effects in the late inspiral stage and • fourier peak frequency of gws from HMNS. However, to succeed in measuring the EOS, higher order PN corrections and • longer and more accurate NR computation are needed. GRB130603B is a golden event • This could be direct evidence of compact binary merger hypothesis of short GRBs. • The time scale, brightness, and color of Kilonova are quite consistent with the NR prediction. For NS5NS merger models, soft EOSs are favored. For BH5NS merger models, stiff EOSs are favored.

本文言語English
ホスト出版物のタイトルJGRG 2013 - Proceedings of the 23rd Workshop on General Relativity and Gravitation in Japan
出版社Hirosaki University
ページ388-409
ページ数22
ISBN(電子版)9780000000002
出版ステータスPublished - 2013
外部発表はい
イベント23rd Workshop on General Relativity and Gravitation in Japan, JGRG 2013 - Aomori, Japan
継続期間: 2013 11 52013 11 8

出版物シリーズ

名前JGRG 2013 - Proceedings of the 23rd Workshop on General Relativity and Gravitation in Japan
2

Conference

Conference23rd Workshop on General Relativity and Gravitation in Japan, JGRG 2013
CountryJapan
CityAomori
Period13/11/513/11/8

ASJC Scopus subject areas

  • Atomic and Molecular Physics, and Optics

フィンガープリント 「“Numerical relativity: Application to gravitational-wave science and astrophysics”」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