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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...
Autores principales: | , , , , , |
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Lenguaje: | eng |
Publicado: |
2019
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1103/PhysRevD.99.104077 http://cds.cern.ch/record/2683806 |