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• W2079000329 abstract "We have studied the evolution of the massless scalar field propagating in a time-dependent charged Vaidya black hole background. A generalized tortoise coordinate transformation was used to study the evolution of the massless scalar field. It is shown that, for the slowest damped quasinormal modes, the approximate formulas in the stationary Reissner-Nordstrom black hole turn out to be a reasonable prescription, showing that results from quasinormal mode analysis are rather robust." @default.
• W2079000329 created "2016-06-24" @default.
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• W2079000329 date "2005-02-02" @default.
• W2079000329 modified "2023-10-16" @default.
• W2079000329 title "Quasinormal modes in a time-dependent black hole background" @default.
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• W2079000329 doi "https://doi.org/10.1103/physrevd.71.044003" @default.
• W2079000329 hasPublicationYear "2005" @default.
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