Quasinormal modes for the charged Vaidya metric

preprint2010arXivOpen access

Abstract

The scalar wave equation is considered in the background of a charged Vaidya metric in double null coordinates (u,v)(u,v) describing a non-stationary charged black hole with varying mass m(v)m(v) and charge q(v)q(v). The resulting time-dependent quasinormal modes are presented and analyzed. We show, in particular, that it is possible to identify some signatures in the quasinormal frequencies from the creation of a naked singularity.

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