Fermion perturbations in string theory black holes
Contribuinte(s) |
UNIVERSIDADE DE SÃO PAULO |
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Data(s) |
20/10/2012
20/10/2012
2011
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Resumo |
In this paper we study fermion perturbations in four-dimensional black holes of string theory, obtained either from a non-extreme configuration of three intersecting five-branes with a boost along the common string or from a non-extreme intersecting system of two two-branes and two five-branes. The Dirac equation for the massless neutrino field, after conformal re-scaling of the metric, is written as a wave equation suitable to study the time evolution of the perturbation. We perform a numerical integration of the evolution equation, and with the aid of Prony fitting of the time-domain profile, we calculate the complex frequencies that dominate the quasinormal ringing stage, and also determine these quantities by the semi-analytical sixth-order WKB method. We also find numerically the decay factor of fermion fields at very late times, and show that the falloff is identical to those showing for massless fields in other four-dimensional black hole spacetimes. FAPESP (Fundacao de Amparo a Pesquisa do Estado de Sao Paulo) Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP) CNPQ (Conselho Nacional de Desenvolvimento Cientifico e Tecnologico), Brazil Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq) |
Identificador |
CLASSICAL AND QUANTUM GRAVITY, v.28, n.8, 2011 0264-9381 http://producao.usp.br/handle/BDPI/29540 10.1088/0264-9381/28/8/085023 |
Idioma(s) |
eng |
Publicador |
IOP PUBLISHING LTD |
Relação |
Classical and Quantum Gravity |
Direitos |
restrictedAccess Copyright IOP PUBLISHING LTD |
Palavras-Chave | #QUASI-NORMAL MODES #GRAVITATIONAL COLLAPSE #SCALAR #DUALITY #6-TORUS #FIELD |
Tipo |
article original article publishedVersion |