Compact Binary Inspirals

Compact Binary Inspirals is a dynamical astrophysical process in which two compact objects, such as neutron stars or black holes, gradually spiral toward each other due to the emission of gravitational radiation, ultimately leading to merger within the framework of post-Newtonian gravity.

225

Publications

28.3K

Citations

2.4K

Authors

371

Institutions

Publications per year

2017–2026

83

Authors

2.4K

  1. NC
    N. Christensen

    Carleton College, United States

    17 publications · 4.1K citations

    16

    h-index

  2. AB
    Alessandra Buonanno

    University of Maryland, College Park, United States

    13 publications · 3.5K citations

    13

    h-index

  3. NY
    Nicolás Yunes

    Montana State University, United States

    12 publications · 1.5K citations

    12

    h-index

  4. BR
    B. R. Iyer

    Centre National de la Recherche Scientifique, France

    12 publications · 5.6K citations

    11

    h-index

  5. BS
    B. S. Sathyaprakash

    Cardiff University, United Kingdom

    12 publications · 4.5K citations

    11

    h-index

1–5 of 2.4K

Venues

  1. 33

    h-index

  2. Physical review. D/Physical review. D.

    PRD · 40 publications · 3.2K citations

    28

    h-index

  3. Classical and Quantum Gravity

    34 publications · 1.9K citations

    22

    h-index

  4. 17

    h-index

  5. The Astrophysical Journal

    ApJ · 18 publications · 3.5K citations

    16

    h-index

1–5