VACUUM POLARIZATION EFFECTS ON QUASINORMAL MODES IN ELECTRICALLY CHARGED BLACK HOLE SPACE-TIMES
Contribuinte(s) |
UNIVERSIDADE DE SÃO PAULO |
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Data(s) |
20/10/2012
20/10/2012
2010
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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 |
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 |