Electromagnetic emission from compact binary mergers

研究成果: Conference contribution

抄録

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).

本文言語English
ホスト出版物のタイトルProceedings of the 25th Workshop on General Relativity and Gravitation in Japan, JGRG 2015
出版社Kyoto University, Yukawa Institute for Theoretical Physics
ページ139-155
ページ数17
ISBN(電子版)9780000000002
出版ステータスPublished - 2015
外部発表はい
イベント25th Workshop on General Relativity and Gravitation in Japan, JGRG 2015 - Kyoto, Japan
継続期間: 2015 12 72015 12 11

出版物シリーズ

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

Conference

Conference25th Workshop on General Relativity and Gravitation in Japan, JGRG 2015
国/地域Japan
CityKyoto
Period15/12/715/12/11

ASJC Scopus subject areas

  • 原子分子物理学および光学

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