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.
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2017–2026
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Quasinormal modes of black holes and black branes
Emanuele Berti, Vítor Cardoso, Andrei O. Starinets · Classical and Quantum Gravity · 2009 · 2.3K citations · Full text
Quasi-Normal Modes of Stars and Black Holes
Living Reviews in Relativity · 1999 · 2K citations · Full text
Natural Sciences, Astronomy, Physics +17
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Universidade de São Paulo
São Paulo, Brazil
37 h-index
97 publications
7.1K citations

Silesian University in Opava
Opava, Czechia
36 h-index
87 publications
7.3K citations
FZU ‒ Institute of Physics of the Academy of Sciences of the Czech Republic
Prague, Czechia
35 h-index
84 publications
7K citations

University of Tübingen
Tübingen, Germany
34 h-index
85 publications
9.5K citations

Universidade Federal do ABC
Santo André, Brazil
33 h-index
60 publications
5.7K citations
Max Planck Institute for Gravitational Physics
Potsdam, Germany
33 h-index
103 publications
8.2K citations
University of Lisbon
Lisbon, Portugal
31 h-index
70 publications
7K citations
Istituto Nazionale di Fisica Nucleare, Sezione di Roma I
Rome, Italy
30 h-index
104 publications
6.8K citations
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187 publications · 15.5K citations
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PRD · 280 publications · 14.5K citations
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JHEP · 125 publications · 5K citations
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