Fermion perturbations in string theory black holes


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

UNIVERSIDADE DE SÃO PAULO

Data(s)

20/10/2012

20/10/2012

2011

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

http://dx.doi.org/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