Gravitational Wave Physics and Astronomy in the nascent era

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抄録

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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詳細情報 詳細情報について

  • CRID
    1050299439981519104
  • ISSN
    20503911
  • HANDLE
    2433/287227
  • 本文言語コード
    en
  • 資料種別
    journal article
  • データソース種別
    • IRDB

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