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Quasinormal modes of Reissner–Nördstrom black hole surrounded by quintessence

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Abstract

We evaluate the complex frequencies of the normal modes for the charged scalar field perturbations around a Reissner–Nördstrom black hole surrounded by a static and spherically symmetric quintessence using third order WKB approximation approach. Quintessence decreases the oscillation frequency and increases the damping time of quasinormal frequencies. We studied the variation of quasinormal frequencies with charge of the black bole, mass and charge of perturbing scalar field and the quintessential parameters.

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Authors and Affiliations

  1. Department of Physics, Cochin University of Science and Technology, Cochin, 682022, Kerala, India

    Nijo Varghese & V. C. Kuriakose

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  1. Nijo Varghese
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  2. V. C. Kuriakose
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Correspondence to Nijo Varghese.

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Varghese, N., Kuriakose, V.C. Quasinormal modes of Reissner–Nördstrom black hole surrounded by quintessence. Gen Relativ Gravit 41, 1249–1257 (2009). https://doi.org/10.1007/s10714-008-0702-9

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  • DOI: https://doi.org/10.1007/s10714-008-0702-9

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