Gravitational Wave Physics and Astronomy in the nascent era
Arimoto, Makoto
Asada, Hideki
Cherry, Michael L
Fujii, Michiko S
Fukazawa, Yasushi
Harada, Akira
Hayama, Kazuhiro
Hosokawa, Takashi
Ioka, Kunihito
Itoh, Yoichi
Kanda, Nobuyuki
Kawabata, Koji S
Kawaguchi, Kyohei
Kawai, Nobuyuki
Kobayashi, Tsutomu
Kohri, Kazunori
Koshio, Yusuke
Kotake, Kei
Kumamoto, Jun
Machida, Masahiro N
Matsufuru, Hideo
Mihara, Tatehiro
Mori, Masaki
Morokuma, Tomoki
Mukohyama, Shinji
Nakano, Hiroyuki
Narikawa, Tatsuya
Negoro, Hitoshi
Nishizawa, Atsushi
Ohgami, Takayuki
Omukai, Kazuyuki
Sakamoto, Takanori
Sako, Shigeyuki
Sasada, Mahito
Sekiguchi, Yuichiro
Serino, Motoko
Soda, Jiro
Sugita, Satoshi
Sumiyoshi, Kohsuke
Susa, Hajime
Suyama, Teruaki
Takahashi, Hirotaka
Takahashi, Kazuya
Takiwaki, Tomoya
Tanaka, Takahiro
Tanaka, Masaomi
Tanikawa, Ataru
Tominaga, Nozomu
Uchikata, Nami
Utsumi, Yousuke
Vagins, Mark R
Yamada, Kei
Yoshida, Michitoshi
京都大学
DOI:10.1093/ptep/ptab042
概要
The detections of gravitational waves (GW) by the LIGO/Virgo collaborations provide various possibilities for both physics and astronomy. We are quite sure that GW observations will develop a lot, both in precision and in number, thanks to the continuous work on the improvement of detectors, including the expected new detector, KAGRA, and the planned detector, LIGO-India. On this occasion, we review the fundamental outcomes and prospects of gravitational wave physics and astronomy. We survey the development, focusing on representative sources of gravitational waves: binary black holes, binary neutron stars, and supernovae. We also summarize the role of gravitational wave observations as a probe of new physics.
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