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

Collaborators

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

Collaborators

SCI - Astronomy

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review

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 language	English
Title of host publication	JGRG 2013 - Proceedings of the 23rd Workshop on General Relativity and Gravitation in Japan
Publisher	Hirosaki University
Pages	388-409
Number of pages	22
ISBN (Electronic)	9780000000002
Publication status	Published - 2013
Event	23rd Workshop on General Relativity and Gravitation in Japan, JGRG 2013 - Aomori, Japan Duration: 2013 Nov 5 → 2013 Nov 8

Publication series

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

Conference

Conference	23rd Workshop on General Relativity and Gravitation in Japan, JGRG 2013
Country/Territory	Japan
City	Aomori
Period	13/11/5 → 13/11/8

Cite this

@inproceedings{5987cbb7a85e4872affb25610b50f7c0,

title = "“Numerical relativity: Application to gravitational-wave science and astrophysics”",

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.",

author = "Collaborators and Kenta Hotokezaka and K. Kiuchi and T. Muransushi and H. Nagakura and Y. Sekiguchi and M. Shibata and K. Kyutoku and H. Okawa and K. Taniguchi and M. Tanaka and S. Wanajo and K. Ioka",

note = "Publisher Copyright: {\textcopyright} JGRG 2013.; 23rd Workshop on General Relativity and Gravitation in Japan, JGRG 2013 ; Conference date: 05-11-2013 Through 08-11-2013",

year = "2013",

language = "English",

series = "JGRG 2013 - Proceedings of the 23rd Workshop on General Relativity and Gravitation in Japan",

publisher = "Hirosaki University",

pages = "388--409",

booktitle = "JGRG 2013 - Proceedings of the 23rd Workshop on General Relativity and Gravitation in Japan",

}

Collaborators 2013, “Numerical relativity: Application to gravitational-wave science and astrophysics”. in JGRG 2013 - Proceedings of the 23rd Workshop on General Relativity and Gravitation in Japan. JGRG 2013 - Proceedings of the 23rd Workshop on General Relativity and Gravitation in Japan, vol. 2, Hirosaki University, pp. 388-409, 23rd Workshop on General Relativity and Gravitation in Japan, JGRG 2013, Aomori, Japan, 13/11/5.

“Numerical relativity: Application to gravitational-wave science and astrophysics”. / Collaborators.
JGRG 2013 - Proceedings of the 23rd Workshop on General Relativity and Gravitation in Japan. Hirosaki University, 2013. p. 388-409 (JGRG 2013 - Proceedings of the 23rd Workshop on General Relativity and Gravitation in Japan; Vol. 2).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review

TY - GEN

T1 - “Numerical relativity

T2 - 23rd Workshop on General Relativity and Gravitation in Japan, JGRG 2013

AU - Collaborators

AU - Hotokezaka, Kenta

AU - Kiuchi, K.

AU - Muransushi, T.

AU - Nagakura, H.

AU - Sekiguchi, Y.

AU - Shibata, M.

AU - Kyutoku, K.

AU - Okawa, H.

AU - Taniguchi, K.

AU - Tanaka, M.

AU - Wanajo, S.

AU - Ioka, K.

PY - 2013

Y1 - 2013

N2 - 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.

AB - 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.

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UR - http://www.scopus.com/inward/citedby.url?scp=85092190102&partnerID=8YFLogxK

M3 - Conference contribution

AN - SCOPUS:85092190102

T3 - JGRG 2013 - Proceedings of the 23rd Workshop on General Relativity and Gravitation in Japan

SP - 388

EP - 409

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

PB - Hirosaki University

Y2 - 5 November 2013 through 8 November 2013

ER -

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

Abstract

Publication series

Conference

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