Compact Binary Coalescence

Compact Binary Coalescence is a dynamical astrophysical process, within the framework of general relativity and the post-Newtonian approximation, in which two compact objects—such as neutron stars or black holes—lose orbital energy through gravitational wave emission, inspiral, and ultimately merge into a single compact object.

494

Publications

59.9K

Citations

10.9K

Authors

759

Institutions

Publications per year

2017–2026

267

Authors

10.9K

  1. JV
    J. Veitch

    University of Birmingham, United Kingdom

    73 publications · 21.7K citations

    45

    h-index

  2. NC
    N. Christensen

    Carleton College, United States

    52 publications · 15K citations

    41

    h-index

  3. AV
    A. Vecchio

    University of Birmingham, United Kingdom

    51 publications · 15.4K citations

    40

    h-index

  4. VR
    V. Raymond

    Max Planck Institute for Gravitational Physics, Germany

    47 publications · 15.3K citations

    39

    h-index

  5. SF
    S. Fairhurst

    Cardiff University, United Kingdom

    51 publications · 14.7K citations

    39

    h-index

1–5 of 10.9K

Venues

  1. Physical review. D/Physical review. D.

    PRD · 121 publications · 8.7K citations

    48

    h-index

  2. The Astrophysical Journal

    ApJ · 65 publications · 9K citations

    45

    h-index

  3. 40

    h-index

  4. Monthly Notices of the Royal Astronomical Society

    37 publications · 3.1K citations

    28

    h-index

  5. Classical and Quantum Gravity

    39 publications · 4.3K citations

    26

    h-index

1–5