TY - GEN
T1 - Electromagnetic emission from compact binary mergers
AU - Tanaka, Masaomi
N1 - Publisher Copyright:
© Proceedings of the 25th Workshop on General Relativity and Gravitation in Japan, JGRG 2015. All rights reserved.
PY - 2015
Y1 - 2015
N2 - 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).
AB - 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).
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M3 - Conference contribution
AN - SCOPUS:85092260020
T3 - Proceedings of the 25th Workshop on General Relativity and Gravitation in Japan, JGRG 2015
SP - 139
EP - 155
BT - Proceedings of the 25th Workshop on General Relativity and Gravitation in Japan, JGRG 2015
PB - Kyoto University, Yukawa Institute for Theoretical Physics
T2 - 25th Workshop on General Relativity and Gravitation in Japan, JGRG 2015
Y2 - 7 December 2015 through 11 December 2015
ER -