Quasi-normal Modes

Quasi-Normal Modes is a mathematical construct in the study of black hole perturbations within numerical relativity that characterizes the damped oscillatory behavior of spacetime in response to disturbances, distinguished by complex-valued frequencies encoding both the oscillation rate and exponential decay of gravitational wave emissions.

1.4K

Publications

91.6K

Citations

1.7K

Authors

797

Institutions

Publications per year

2017–2026

675

Authors

1.7K

  1. RA
    R. A. Konoplya

    Silesian University in Opava, Czechia

    63 publications · 7.3K citations

    46

    h-index

  2. VC
    Vítor Cardoso

    University of Lisbon, Portugal

    50 publications · 10.1K citations

    38

    h-index

  3. EB
    Emanuele Berti

    University of Mississippi, United States

    40 publications · 7.9K citations

    33

    h-index

  4. AZ
    A. Zhidenko

    Universidade Federal do ABC, Brazil

    37 publications · 4.1K citations

    31

    h-index

  5. BW
    Bin Wang

    Shanghai Jiao Tong University, China

    26 publications · 1.5K citations

    22

    h-index

1–5 of 1.7K

Venues

  1. 69

    h-index

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

    PRD · 280 publications · 14.5K citations

    67

    h-index

  3. 52

    h-index

  4. Journal of High Energy Physics

    JHEP · 125 publications · 5K citations

    43

    h-index

  5. Classical and Quantum Gravity

    109 publications · 9.5K citations

    43

    h-index

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