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arxiv: gr-qc/9903032 · v1 · submitted 1999-03-08 · 🌀 gr-qc

Perturbative Approach to the Quasinormal Modes of Dirty Black Holes

classification 🌀 gr-qc
keywords blackholemodesperturbationapproachdevelopeddirtyequation
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Using a recently developed perturbation theory for uasinormal modes (QNM's), we evaluate the shifts in the real and imaginary parts of the QNM frequencies due to a quasi-static perturbation of the black hole spacetime. We show the perturbed QNM spectrum of a black hole can have interesting features using a simple model based on the scalar wave equation.

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