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Mode Stability For Massless Scalars In Five-Dimensional Black Hole Backgrounds

The mode stability of the Kerr black hole in four dimensions was demonstrated by Whiting in 1989, by separating the Teukolsky equation that describes gravitational perturbations and then transforming the radial and angular equations in such a way that the problem can be reformulated as a wave equati...

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Detalles Bibliográficos
Autores principales:	Cvetic, M., Pope, C.N., Whiting, B.F., Zhang, Haoyu
Lenguaje:	eng
Publicado:	2022
Materias:	hep-th Particle Physics - Theory gr-qc General Relativity and Cosmology
Acceso en línea:	https://dx.doi.org/10.1103/PhysRevD.106.104026 http://cds.cern.ch/record/2815107

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