On The Black Hole Interior Spacetime

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dc.creatorCuletu, Hristu
dc.date2007-01-27
dc.date2007-03-07
dc.date.accessioned2026-07-07T13:08:06Z
dc.date.available2026-07-07T13:08:06Z
dc.descriptionA new version of the geometry inside a black hole is proposed, on the grounds of an idea given by Doran et al. The spacetime is still time dependent and is a solution of Einstein's equations with a stress tensor corresponding to an anisotropic fluid. The energy density of the fluid is proportional to $1/t^{2}$ as in many dark energy models and the Brown-York quasilocal energy of the black hole interior equals its mass $m$.
dc.description6 pages,one reference added, minor changes, no figures
dc.identifierhttps://arxiv.org/abs/hep-th/0701255
dc.identifierhttp://arxiv.org/abs/hep-th/0701255
dc.identifierInt.J.Mod.Phys.A24:1593-1597,2009
dc.identifierdoi:10.1142/S0217751X09045066
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/228309
dc.subjectHigh Energy Physics - Theory
dc.subjectAstrophysics
dc.titleOn The Black Hole Interior Spacetime
dc.typetext

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