Electromagnetic emission from compact binary mergers

Masaomi Tanaka

Electromagnetic emission from compact binary mergers

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

Abstract

Why EM emission from NS merger? • Crucial for idenfification of GW sources • LIGO O1 started in 2015 Sep • Radioactively-powered emission • Fainter and redder than expected, but detectable • GRB 130603B => possible constraints on EOS (NS radius) • More realistic simulations are critical (wind components, BHCNS mergers, and⋯) • Prospects for observations • JCGEM: Japanese EM followCup network • Subaru/HSC is important (transient search started).

Original language	English
Title of host publication	Proceedings of the 25th Workshop on General Relativity and Gravitation in Japan, JGRG 2015
Publisher	Kyoto University, Yukawa Institute for Theoretical Physics
Pages	139-155
Number of pages	17
ISBN (Electronic)	9780000000002
Publication status	Published - 2015
Externally published	Yes
Event	25th Workshop on General Relativity and Gravitation in Japan, JGRG 2015 - Kyoto, Japan Duration: 2015 Dec 7 → 2015 Dec 11

Publication series

Name	Proceedings of the 25th Workshop on General Relativity and Gravitation in Japan, JGRG 2015
Volume	1

Conference

Conference	25th Workshop on General Relativity and Gravitation in Japan, JGRG 2015
Country	Japan
City	Kyoto
Period	15/12/7 → 15/12/11

ASJC Scopus subject areas

Atomic and Molecular Physics, and Optics

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Cite this

Electromagnetic emission from compact binary mergers. / Tanaka, Masaomi.

Proceedings of the 25th Workshop on General Relativity and Gravitation in Japan, JGRG 2015. Kyoto University, Yukawa Institute for Theoretical Physics, 2015. p. 139-155 (Proceedings of the 25th Workshop on General Relativity and Gravitation in Japan, JGRG 2015; Vol. 1).

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

Tanaka, M 2015, Electromagnetic emission from compact binary mergers. in Proceedings of the 25th Workshop on General Relativity and Gravitation in Japan, JGRG 2015. Proceedings of the 25th Workshop on General Relativity and Gravitation in Japan, JGRG 2015, vol. 1, Kyoto University, Yukawa Institute for Theoretical Physics, pp. 139-155, 25th Workshop on General Relativity and Gravitation in Japan, JGRG 2015, Kyoto, Japan, 15/12/7.

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abstract = "Why EM emission from NS merger? • Crucial for idenfification of GW sources • LIGO O1 started in 2015 Sep • Radioactively-powered emission • Fainter and redder than expected, but detectable • GRB 130603B => possible constraints on EOS (NS radius) • More realistic simulations are critical (wind components, BHCNS mergers, and⋯) • Prospects for observations • JCGEM: Japanese EM followCup network • Subaru/HSC is important (transient search started).",

author = "Masaomi Tanaka",

note = "Publisher Copyright: {\textcopyright} Proceedings of the 25th Workshop on General Relativity and Gravitation in Japan, JGRG 2015. All rights reserved. Copyright: Copyright 2020 Elsevier B.V., All rights reserved.; 25th Workshop on General Relativity and Gravitation in Japan, JGRG 2015 ; Conference date: 07-12-2015 Through 11-12-2015",

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