Black hole mass decreasing due to phantom energy accretion

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dc.creatorBabichev, E.
dc.creatorDokuchaev, V.
dc.creatorEroshenko, Y.
dc.date2005-07-28
dc.date.accessioned2026-07-07T03:29:51Z
dc.date.available2026-07-07T03:29:51Z
dc.descriptionSolution for a stationary spherically symmetric accretion of the relativistic perfect fluid with an equation of state p(rho) onto the Schwarzschild black hole is presented. This solution is a generalization of Michel solution and applicable to the problem of dark energy accretion. It is shown that accretion of phantom energy is accompanied with the gradual decrease of the black hole mass. Masses of all black holes tend to zero in the phantom energy universe approaching to the Big Rip.
dc.descriptionPlenary talk presented at Workshop on High Energy Physics&Field Theory (Protvino, Russia, 2004)
dc.identifierhttps://arxiv.org/abs/gr-qc/0507119
dc.identifierhttp://arxiv.org/abs/gr-qc/0507119
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/35340
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleBlack hole mass decreasing due to phantom energy accretion
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