On the quasinormal modes of the de Sitter spacetime

A. López-Ortega

doi:10.1007/s10714-012-1398-4

On the quasinormal modes of the de Sitter spacetime

A. López-Ortega

Producción científica: Contribución a una revista › Artículo › revisión exhaustiva

15 Citas (Scopus)

Resumen

Modifying a method by Horowitz and Hubeny for asymptotically anti-de Sitter black holes, we establish the classical stability of the quasinormal modes of the de Sitter spacetime. Furthermore using a straightforward method we calculate the de Sitter quasinormal frequencies of the gravitational perturbations and discuss some properties of the radial functions of these quasinormal modes.

Idioma original	Inglés
Páginas (desde-hasta)	2387-2400
Número de páginas	14
Publicación	General Relativity and Gravitation
Volumen	44
N.º	9
DOI	https://doi.org/10.1007/s10714-012-1398-4
Estado	Publicada - sep. 2012
Publicado de forma externa	Sí

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abstract = "Modifying a method by Horowitz and Hubeny for asymptotically anti-de Sitter black holes, we establish the classical stability of the quasinormal modes of the de Sitter spacetime. Furthermore using a straightforward method we calculate the de Sitter quasinormal frequencies of the gravitational perturbations and discuss some properties of the radial functions of these quasinormal modes.",

keywords = "Classical stability, Quasinormal modes, de Sitter spacetime",

author = "A. L{\'o}pez-Ortega",

note = "Funding Information: Acknowledgments This work was supported by CONACYT M{\'e}xico, SNI M{\'e}xico, EDI-IPN, COFAA-IPN, and Research Projects SIP-20120773 and SIP-20121648.",

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N2 - Modifying a method by Horowitz and Hubeny for asymptotically anti-de Sitter black holes, we establish the classical stability of the quasinormal modes of the de Sitter spacetime. Furthermore using a straightforward method we calculate the de Sitter quasinormal frequencies of the gravitational perturbations and discuss some properties of the radial functions of these quasinormal modes.

AB - Modifying a method by Horowitz and Hubeny for asymptotically anti-de Sitter black holes, we establish the classical stability of the quasinormal modes of the de Sitter spacetime. Furthermore using a straightforward method we calculate the de Sitter quasinormal frequencies of the gravitational perturbations and discuss some properties of the radial functions of these quasinormal modes.

KW - Classical stability

KW - Quasinormal modes

KW - de Sitter spacetime

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M3 - Artículo

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JO - General Relativity and Gravitation

JF - General Relativity and Gravitation

IS - 9

ER -

On the quasinormal modes of the de Sitter spacetime

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