Charged Black Holes in Phantom Cosmology

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dc.creatorJamil, Mubasher
dc.creatorRashid, Muneer Ahmad
dc.creatorQadir, Asghar
dc.date2008-08-08
dc.date2008-12-12
dc.date.accessioned2026-07-07T12:15:11Z
dc.date.available2026-07-07T12:15:11Z
dc.descriptionIn the classical relativistic regime, the accretion of phantom-like dark energy onto a stationary black hole reduces the mass of black hole. Here 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 limit. This condition also challenges the validity of the cosmic censorship conjecture since a naked singularity is eventually produced as magnitude of charge increases compared to mass of black hole.
dc.description10 pages, to appear in Eur. Phys. J C
dc.identifierhttps://arxiv.org/abs/0808.1152
dc.identifierhttp://arxiv.org/abs/0808.1152
dc.identifierEur.Phys.J.C58:325-329,2008
dc.identifierdoi:10.1140/epjc/s10052-008-0761-9
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/211432
dc.subjectAstrophysics
dc.titleCharged Black Holes in Phantom Cosmology
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