Superradiant instability of near extremal and extremal four-dimensional charged hairy black holes in anti-de Sitter spacetime

P. A. González, Eleftherios Papantonopoulos, JOEL FRANCISCO SAAVEDRA ALVEAR, Yerko Vásquez

Resultado de la investigación: Contribución a una revistaArtículorevisión exhaustiva

25 Citas (Scopus)

Resumen

We study the instability of near extremal and extremal four-dimensional anti-de Sitter charged hairy black holes to radial neutral massive and charged massless scalar field perturbations. We solve the scalar field equation by using the improved asymptotic iteration method and the time domain analysis, and we find the quasinormal frequencies. For the charged scalar perturbations, we find the superradiance condition by computing the reflection coefficient in the low-frequency limit, and we show that in the superradiance regime, which depends on the scalar hair charge, all modes of radial charged massless perturbations are unstable, indicating that the charged hairy black hole is superradiantly unstable. On the other hand, calculating the quasinormal frequencies of radial neutral scalar perturbations in this background, we find stability of the charged hairy black hole.

Idioma originalInglés
Número de artículo064046
PublicaciónPhysical Review D
Volumen95
N.º6
DOI
EstadoPublicada - 27 mar 2017

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