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Perturbative Approach to the Quasinormal Modes of Dirty Black Holes

P. T. Leung·Y. T. Liu·W. -M. Suen·C. Y. Tam·K. Young
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Abstract

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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P. T. Leung, Y. T. Liu, W. -M. Suen, C. Y. Tam, K. Young. 1999-03-08. Perturbative Approach to the Quasinormal Modes of Dirty Black Holes. https://doi.org/10.1103/physrevd.59.044034

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