Abstract
In the classical relativistic regime, the accretion of phantom-like dark energy onto a stationary black hole reduces the mass of the black hole. We have investigated the accretion of phantom energy onto a stationary charged black hole and have determined the condition under which this accretion is possible. This condition restricts the mass-to-charge ratio in a narrow range. This condition also challenges the validity of the cosmic-censorship conjecture since a naked singularity is eventually produced due to accretion of phantom energy onto black hole.
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Jamil, M., Qadir, A. & Rashid, M.A. Charged black holes in phantom cosmology. Eur. Phys. J. C 58, 325–329 (2008). https://doi.org/10.1140/epjc/s10052-008-0761-9
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DOI: https://doi.org/10.1140/epjc/s10052-008-0761-9