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

Collaborators

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

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.

Original languageEnglish
Title of host publicationJGRG 2013 - Proceedings of the 23rd Workshop on General Relativity and Gravitation in Japan
PublisherHirosaki University
Pages388-409
Number of pages22
ISBN (Electronic)9780000000002
Publication statusPublished - 2013
Externally publishedYes
Event23rd Workshop on General Relativity and Gravitation in Japan, JGRG 2013 - Aomori, Japan
Duration: 2013 Nov 52013 Nov 8

Publication series

NameJGRG 2013 - Proceedings of the 23rd Workshop on General Relativity and Gravitation in Japan
Volume2

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

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