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Gravitational Wave Physics and Astronomy in the nascent era

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arxiv 2104.02445 v1 pith:4LU5QT6A submitted 2021-04-06 gr-qc astro-ph.HE

Makoto Arimoto , Hideki Asada , Michael L. Cherry , Michiko S. Fujii , Yasushi Fukazawa , Akira Harada , Kazuhiro Hayama , Takashi Hosokawa
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Kunihito Ioka Yoichi Itoh Nobuyuki Kanda Koji S. Kawabata Kyohei Kawaguchi Nobuyuki Kawai Tsutomu Kobayashi Kazunori Kohri Yusuke Koshio Kei Kotake Jun Kumamoto Masahiro N. Machida Hideo Matsufuru Tatehiro Mihara Masaki Mori Tomoki Morokuma Shinji Mukohyama Hiroyuki Nakano Tatsuya Narikawa Hitoshi Negoro Atsushi Nishizawa Takayuki Ohgami Kazuyuki Omukai Takanori Sakamoto Shigeyuki Sako Mahito Sasada Yuichiro Sekiguchi Motoko Serino Jiro Soda Satoshi Sugita Kohsuke Sumiyoshi Hajime Susa Teruaki Suyama Hirotaka Takahashi Kazuya Takahashi Tomoya Takiwaki Takahiro Tanaka Masaomi Tanaka Ataru Tanikawa Nozomu Tominaga Nami Uchikata Yousuke Utsumi Mark R. Vagins Kei Yamada Michitoshi Yoshida
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classification gr-qcastro-ph.HE
keywords gravitationalphysicsastronomywavebinarydetectorobservationswaves
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The detections of gravitational waves (GW) by LIGO/Virgo collaborations provide various possibilities to physics and astronomy. We are quite sure that GW observations will develop a lot both in precision and in number owing to the continuous works for the improvement of detectors, including the expectation to the newly joined detector, KAGRA, and the planned detector, LIGO-India. In 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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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap

    astro-ph.HE 2025-09 reject novelty 4.0 of 10

    Applying a phase-space overlap method to GWTC-4, the paper claims first-generation black holes are truncated near 45.5 solar masses, but the cutoff follows from the assumed exponential mass prior rather than from the data.

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