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arXiv · 0706.3238

Perturbation theory of spherically symmetric self-similar black holes

A. J. S. Hamilton
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Abstract

The 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.

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A. J. S. Hamilton. 2007-06-22. Perturbation theory of spherically symmetric self-similar black holes. https://arxiv.org/abs/0706.3238

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