Stability under scalar perturbations and quasinormal modes of 4D Einstein–Born–Infeld dilaton spacetime: exact spectrum

Kyriakos Destounis, Grigoris Panotopoulos, Ángel Rincón

Resultado de la investigación: Contribución a una revistaArtículorevisión exhaustiva

25 Citas (Scopus)

Resumen

We study the stability under scalar perturbations, and we compute the quasinormal modes of the Einstein–Born–Infeld dilaton spacetime in 1 + 3 dimensions. Solving the full radial equation in terms of hypergeometric functions, we provide an exact analytical expression for the spectrum. We find that the frequencies are purely imaginary, and we confirm our results by computing them numerically. Although the scalar field that perturbs the black hole is electrically neutral, an instability similar to that seen in charged scalar perturbations of the Reissner–Nordström black hole is observed.

Idioma originalInglés
Número de artículo139
PublicaciónEuropean Physical Journal C
Volumen78
N.º2
DOI
EstadoPublicada - 1 feb. 2018
Publicado de forma externa

Huella

Profundice en los temas de investigación de 'Stability under scalar perturbations and quasinormal modes of 4D Einstein–Born–Infeld dilaton spacetime: exact spectrum'. En conjunto forman una huella única.

Citar esto