Killing horizons kill horizon degrees

dc.creatorBergamin, L.
dc.creatorGrumiller, D.
dc.date2006-05-30
dc.date2006-11-21
dc.date.accessioned2026-07-07T10:40:54Z
dc.date.available2026-07-07T10:40:54Z
dc.descriptionFrequently it is argued that the microstates responsible for the Bekenstein-Hawking entropy should arise from some physical degrees of freedom located near or on the black hole horizon. In this Essay we elucidate that instead entropy may emerge from the conversion of physical degrees of freedom, attached to a generic boundary, into unobservable gauge degrees of freedom attached to the horizon. By constructing the reduced phase space it can be demonstrated that such a transmutation indeed takes place for a large class of black holes, including Schwarzschild.
dc.description5 pages, received honorable mention in the GRF Essay Contest 2006, v2: version to be published in IJMPD
dc.identifierhttps://arxiv.org/abs/gr-qc/0605148
dc.identifierhttp://arxiv.org/abs/gr-qc/0605148
dc.identifierInt.J.Mod.Phys.D15:2279-2284,2006
dc.identifierdoi:10.1142/S0218271806009571
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/181469
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleKilling horizons kill horizon degrees
dc.typetext

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