Binary Black Hole Simulations

Binary Black Hole Simulations is a computational framework in numerical relativity that models the dynamical evolution of two orbiting black holes and their gravitational wave emission under Einstein's field equations, distinguished by its treatment of strong-field gravity, spacetime singularities, and asymptotically flat boundary conditions.

439

Publications

40K

Citations

2.1K

Authors

441

Institutions

Publications per year

2017–2026

169

Authors

2.1K

  1. MS
    Mark Scheel

    California Institute of Technology, United States

    42 publications · 5.9K citations

    34

    h-index

  2. CO
    C. O. Loustó

    Rochester Institute of Technology, United States

    36 publications · 3.3K citations

    30

    h-index

  3. HP
    Harald Pfeiffer

    California Institute of Technology, United States

    37 publications · 5.1K citations

    29

    h-index

  4. MC
    Manuela Campanelli

    Rochester Institute of Technology, United States

    25 publications · 2.3K citations

    21

    h-index

  5. BS
    Béla Szilágyi

    California Institute of Technology, United States

    23 publications · 3.3K citations

    21

    h-index

1–5 of 2.1K

Venues

  1. 53

    h-index

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

    PRD · 82 publications · 5.5K citations

    41

    h-index

  3. The Astrophysical Journal

    ApJ · 34 publications · 4.8K citations

    31

    h-index

  4. Classical and Quantum Gravity

    50 publications · 3.5K citations

    30

    h-index

  5. Monthly Notices of the Royal Astronomical Society

    38 publications · 2.9K citations

    29

    h-index

1–5