VACUUM POLARIZATION EFFECTS ON QUASINORMAL MODES IN ELECTRICALLY CHARGED BLACK HOLE SPACE-TIMES


Autoria(s): PIEDRA, Owen Pavel Fernandez; OLIVEIRA, Jeferson de
Contribuinte(s)

UNIVERSIDADE DE SÃO PAULO

Data(s)

20/10/2012

20/10/2012

2010

Resumo

We investigate the influence of vacuum polarization of quantum massive fields on the scalar sector of quasinormal modes in spherically symmetric black holes. We consider the evolution of a massless scalar field on the space-time corresponding to a charged semiclassical black hole, consisting of the quantum-corrected geometry of a Reissner-Nordstrom black hole dressed by a quantum massive scalar field in the large mass limit. Using a sixth order WKB approach we find a shift in the quasinormal mode frequencies due to vacuum polarization.

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

FAPESP (Fundacao de Amparo a Pesquisa do Estado de Sao Paulo)

Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)

CNPQ (Conselho Nacional de Desenvolvimento Cientifico e Tecnologico), Brazil

ICTP, Trieste

ICTP, Trieste

Identificador

INTERNATIONAL JOURNAL OF MODERN PHYSICS D, v.19, n.1, p.63-78, 2010

0218-2718

http://producao.usp.br/handle/BDPI/29575

10.1142/S0218271810016257

http://dx.doi.org/10.1142/S0218271810016257

Idioma(s)

eng

Publicador

WORLD SCIENTIFIC PUBL CO PTE LTD

Relação

International Journal of Modern Physics D

Direitos

restrictedAccess

Copyright WORLD SCIENTIFIC PUBL CO PTE LTD

Palavras-Chave #Black holes #quasinormal modes #semiclassical gravity #STRESS-ENERGY TENSOR #MASSIVE SCALAR FIELDS #BACK-REACTION #WKB APPROACH #PERTURBATIONS #EVOLUTION #RADIATION #BEHAVIOR #GRAVITY #Astronomy & Astrophysics
Tipo

article

original article

publishedVersion