Compact Object Merger Simulations

Compact Object Merger Simulations is a computational framework that models the dynamical interactions and gravitational wave emissions of coalescing compact astrophysical bodies, such as neutron stars and black holes, through high-resolution numerical relativity and hydrodynamics to predict observable signatures and post-merger remnants.

119

Publications

12.9K

Citations

1.3K

Authors

356

Institutions

Publications per year

2017–2026

65

Authors

1.3K

  1. MM
    Michela Mapelli

    Osservatorio Astronomico di Padova, Italy

    7 publications · 910 citations

    7

    h-index

  2. KB
    Krzysztof Belczyński

    Nicolaus Copernicus Astronomical Center, Poland

    6 publications · 712 citations

    6

    h-index

  3. NG
    Nicola Giacobbo

    Osservatorio Astronomico di Padova, Italy

    5 publications · 822 citations

    5

    h-index

  4. EQ
    Eliot Quataert

    University of California, Berkeley, United States

    5 publications · 1.6K citations

    5

    h-index

  5. AB
    Alessandra Buonanno

    University of Maryland, College Park, United States

    5 publications · 482 citations

    5

    h-index

1–5 of 1.3K

Venues

  1. Monthly Notices of the Royal Astronomical Society

    29 publications · 3.9K citations

    26

    h-index

  2. The Astrophysical Journal

    ApJ · 25 publications · 4.1K citations

    22

    h-index

  3. Physical review. D/Physical review. D.

    PRD · 17 publications · 1.1K citations

    16

    h-index

  4. Astronomy and Astrophysics

    6 publications · 448 citations

    6

    h-index

  5. The Astrophysical Journal Letters

    5 publications · 632 citations

    5

    h-index

1–5