Gravity and the Thermodynamics of Horizons

dc.creatorPadmanabhan, T.
dc.date2003-11-11
dc.date2005-01-20
dc.date.accessioned2026-07-07T10:48:14Z
dc.date.available2026-07-07T10:48:14Z
dc.descriptionSpacetimes with horizons show a resemblance to thermodynamic systems and it is possible to associate the notions of temperature and entropy with them. Several aspects of this connection are reviewed in a manner appropriate for broad readership. The approach uses two essential principles: (a) the physical theories must be formulated for each observer entirely in terms of variables any given observer can access and (b) consistent formulation of quantum field theory requires analytic continuation to the complex plane. These two principles, when used together in spacetimes with horizons, are powerful enough to provide several results in a unified manner. Since spacetimes with horizons have a generic behaviour under analytic continuation, standard results of quantum field theory in curved spacetimes with horizons can be obtained directly (Sections III to VII). The requirements (a) and (b) also put strong constraints on the action principle describing the gravity and, in fact, one can obtain the Einstein-Hilbert action from the thermodynamic considerations. The latter part of the review (Sections VIII to X) investigates this deeper connection between gravity, spacetime microstructure and thermodynamics of horizons. This approach leads to several interesting results in the semiclassical limit of quantum gravity, which are described.
dc.descriptionpublished version; references updated
dc.identifierhttps://arxiv.org/abs/gr-qc/0311036
dc.identifierhttp://arxiv.org/abs/gr-qc/0311036
dc.identifierPhys.Rept.406:49-125,2005
dc.identifierdoi:10.1016/j.physrep.2004.10.003
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/183804
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Theory
dc.titleGravity and the Thermodynamics of Horizons
dc.typetext

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