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Parametrized black hole quasinormal ringdown: Decoupled equations for nonrotating black holes

Black hole solutions in general relativity are simple. The frequency spectrum of linear perturbations around these solutions (i.e., the quasinormal modes) is also simple, and therefore it is a prime target for fundamental tests of black hole spacetimes and of the underlying theory of gravity. The fo...

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Detalles Bibliográficos
Autores principales: Cardoso, Vitor, Kimura, Masashi, Maselli, Andrea, Berti, Emanuele, Macedo, Caio F.B., McManus, Ryan
Lenguaje:eng
Publicado: 2019
Materias:
Acceso en línea:https://dx.doi.org/10.1103/PhysRevD.99.104077
http://cds.cern.ch/record/2683806