Semiclassical ultraextremal horizons

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dc.creatorMatyjasek, Jerzy
dc.creatorZaslavskii, O. B.
dc.date2005-02-26
dc.date2005-03-04
dc.date.accessioned2026-07-07T11:42:59Z
dc.date.available2026-07-07T11:42:59Z
dc.descriptionWe examine backreaction of quantum massive fields on multiply-degenerate (ultraextremal) horizons. It is shown that, under influence of the quantum backreaction, the horizon of such a kind moves to a new position, near which the metric does not change its asymptotics, so the ultraextremal black holes and cosmological spacetimes do exist as self-consistent solutions of the semiclassical field equations.
dc.descriptionReferences added
dc.identifierhttps://arxiv.org/abs/gr-qc/0502115
dc.identifierhttp://arxiv.org/abs/gr-qc/0502115
dc.identifierPhys.Rev.D71:087501,2005
dc.identifierdoi:10.1103/PhysRevD.71.087501
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/201079
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleSemiclassical ultraextremal horizons
dc.typetext

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