Binary Black Hole Systems

Binary Black Hole Systems is a theoretical astrophysical construct denoting a gravitationally bound system consisting of two black holes in close orbit around their common center of mass, distinguished from single black hole systems by the dynamics of their mutual interaction and eventual merger through the emission of gravitational waves.

2.2K

Publications

207K

Citations

12.1K

Authors

1.3K

Institutions

Publications per year

2017–2026

998

Authors

12.1K

  1. SH
    S. Husa

    Max Planck Institute for Gravitational Physics, Germany

    63 publications · 31.3K citations

    50

    h-index

  2. HP
    Harald Pfeiffer

    California Institute of Technology, United States

    71 publications · 28.8K citations

    49

    h-index

  3. AV
    A. Vecchio

    University of Birmingham, United Kingdom

    51 publications · 29.3K citations

    45

    h-index

  4. MS
    Mark Scheel

    California Institute of Technology, United States

    56 publications · 7.7K citations

    44

    h-index

  5. CO
    C. O. Loustó

    Rochester Institute of Technology, United States

    59 publications · 23.9K citations

    43

    h-index

1–5 of 12.1K

Venues

  1. The Astrophysical Journal

    ApJ · 324 publications · 31.3K citations

    100

    h-index

  2. 91

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    303 publications · 23.9K citations

    85

    h-index

  4. Physical review. D/Physical review. D.

    PRD · 352 publications · 25.6K citations

    83

    h-index

  5. Physical Review Letters

    PRL · 99 publications · 35K citations

    64

    h-index

1–5