QFT holography near the horizon of Schwarzschild-like spacetimes

dc.creatorMoretti, V.
dc.creatorPinamonti, N.
dc.date2003-04-10
dc.date2003-04-15
dc.date.accessioned2026-07-07T04:15:08Z
dc.date.available2026-07-07T04:15:08Z
dc.descriptionIt is argued that free QFT can be defined on the event horizon of a Schwarzschild-like spacetime and that this theory is unitarily and algebraically equivalent to QFT in the bulk (near the horizon). Under that unitary equivalence the bulk hidden SL(2,R) symmetry found in a previous work becomes manifest on the event horizon, it being induced by a group of horizon diffeomorphisms. The class of generators of that group can be enlarged to include a full Virasoro algebra of fields which are defined on the event horizon. These generators have a quantum representation in QFT on the event horizon and thus in the bulk.
dc.description8 pages, 1 figure, latex 2e, Relevant references added
dc.identifierhttps://arxiv.org/abs/hep-th/0304102
dc.identifierhttp://arxiv.org/abs/hep-th/0304102
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/51890
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleQFT holography near the horizon of Schwarzschild-like spacetimes
dc.typetext

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