Semiclassical corrections to the Einstein equation and Induced Matter Theory

dc.creatorMoyassari, P.
dc.creatorJalalzadeh, S.
dc.date2007-05-16
dc.date.accessioned2026-07-07T10:55:36Z
dc.date.available2026-07-07T10:55:36Z
dc.descriptionThe induced Einstein equation on a perturbed brane in the Induced Matter Theory is re-analyzed. We indicate that in a conformally flat background, the local quantum corrections to the Einstein equation can be obtained via the IMT. Using the FRW metric as the 4D gravitational model, we show that the classical fluctuations of the brane may be related to the quantum corrections to the classical Einstein equation. In other words, the induced Einstein equation on the perturbed brane correspond with the semiclassical Einstein equation.
dc.description9 pages, to appear in GRG
dc.identifierhttps://arxiv.org/abs/0705.2289
dc.identifierhttp://arxiv.org/abs/0705.2289
dc.identifierGen.Rel.Grav.39:1467-1476,2007
dc.identifierdoi:10.1007/s10714-007-0466-7
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/186130
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleSemiclassical corrections to the Einstein equation and Induced Matter Theory
dc.typetext

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