Quasinormal modes for massless topological black holes

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An exact expression for the quasinormal modes of scalar perturbations on a massless topological black hole in four and higher dimensions is presented. The massive scalar field is nonminimally coupled to the curvature, and the horizon geometry is assumed to have a negative constant curvature.
CECS style, 11 pages, no figures. References added

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High Energy Physics - Theory, General Relativity and Quantum Cosmology

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http://salesiana.dossiersoluciones.com/handle/123456789/184238

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/hep-th/0211024
 http://arxiv.org/abs/hep-th/0211024
 Phys.Rev.D67:044014,2003
 doi:10.1103/PhysRevD.67.044014

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arXiv