Gravitational Back Reaction of Hawking modes

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dc.creatorRing, D.
dc.date2005-03-14
dc.date2005-08-28
dc.date.accessioned2026-07-07T04:18:10Z
dc.date.available2026-07-07T04:18:10Z
dc.descriptionThe radiation rate of an evaporating black hole is calculated in a toy model in which the geometry outside the collapsing matter is described by a Vaidya metric. When back reaction consistency is imposed, the singularity in the blueshift factor near the horizon is softened, suppressing the evaporation rate in the Schwarzschild case by the fourth power of the external time, thus rendering the hole eternal.
dc.descriptionMisguided discussion of partner propagation removed. Ridiculous claims withdrawn. It's still pretty cool, but now it's just a toy model
dc.identifierhttps://arxiv.org/abs/hep-th/0503109
dc.identifierhttp://arxiv.org/abs/hep-th/0503109
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/53065
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleGravitational Back Reaction of Hawking modes
dc.typetext

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