Deformations of the Schwarzschild Black Hole

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dc.creatorGrumiller, D.
dc.date2003-11-04
dc.date2003-12-18
dc.date.accessioned2026-07-07T03:28:13Z
dc.date.available2026-07-07T03:28:13Z
dc.descriptionDue to its large number of symmetries the Schwarzschild Black Hole can be described by a specific two-dimensional dilaton gravity model. After reviewing classical, semi-classical and quantum properties and a brief discussion of virtual black holes deformations are studied: the first part is devoted to deformations of the Lorentz-symmetry, the second part to dynamical deformations and its role for the long time evaporation of the Schwarzschild Black Hole.
dc.description6 pages, 3 figures, invited contribution to the QG1 session at MGX, v2: updated affiliation
dc.identifierhttps://arxiv.org/abs/gr-qc/0311011
dc.identifierhttp://arxiv.org/abs/gr-qc/0311011
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/34746
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Theory
dc.titleDeformations of the Schwarzschild Black Hole
dc.typetext

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