Perturbation theory of spherically symmetric self-similar black holes

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dc.creatorHamilton, A. J. S.
dc.date2007-06-22
dc.date2007-06-22
dc.date.accessioned2026-07-07T08:11:50Z
dc.date.available2026-07-07T08:11:50Z
dc.descriptionThe theory of perturbations of spherically symmetric self-similar black holes is presented, in the Newman-Penrose formalism. It is shown that the wave equations for gravitational, electromagnetic, and scalar waves are separable, though not decoupled. A generalization of the Teukolsky equation is given. Monopole and dipole modes are treated. The Newman-Penrose wave equations governing polar and axial spin-0 perturbations are explored.
dc.description63 pages, 1 eps figure
dc.identifierhttps://arxiv.org/abs/0706.3238
dc.identifierhttp://arxiv.org/abs/0706.3238
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/132250
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.titlePerturbation theory of spherically symmetric self-similar black holes
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