Gravitational Wave Physics and Astronomy in the nascent era
Gravitational Wave Physics and Astronomy in the nascent era
复制标题
新生时代的引力波物理和天文学
DOI：
10.1093/ptep/ptab042
复制
发表时间：
2021
影响因子：
3.5
通讯作者：
他
中科院分区：
文献类型：
--
作者：
Arimoto Makoto;Asada Hideki;Cherry Michael L;Tsutomu Kobayashi;他
LIGO/Virgo合作探测到的引力波（GW）为物理学和天文学提供了多种可能性。我们非常确信，由于不断改进探测器的工作，包括预期的新探测器KAGRA和计划中的探测器LIGO-India， GW观测将在精度和数量上有很大的发展。在此，我们回顾引力波物理学和天文学的基本成果和前景。我们回顾了引力波的发展，重点介绍了引力波的代表性来源：双黑洞、双中子星和超新星。我们还总结了引力波观测作为新物理学探测的作用。
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.