Counter example to a quantum inequality

dc.creatorKrasnikov, S.
dc.date2004-09-01
dc.date2005-05-25
dc.date.accessioned2026-07-07T07:35:54Z
dc.date.available2026-07-07T07:35:54Z
dc.descriptionA `quantum inequality' (a conjectured relation between the energy density of a free quantum field and the time during which this density is observed) has recently been used to rule out some of the macroscopic wormholes and warp drives. I discuss the possibility of generalizing that result to other similar spacetimes and first show that the problem amounts to verification of a slightly different inequality. This new inequality \emph{can} replace the original one, if an additional assumption (concerning homogeneity of the `exotic matter' distribution) is made, and \emph{must} replace it if the assumption is relaxed. Then by an explicit example I show that the `new' inequality breaks down even in a simplest case (a free field in a simply connected two dimensional space). Which suggests that there is no grounds today to consider such spacetimes `unphysical'.
dc.descriptionSec. II is completely rewritten: the gulf is discussed between the proven QIs and those used in ruling out exotic spacetimes
dc.identifierhttps://arxiv.org/abs/gr-qc/0409007
dc.identifierhttp://arxiv.org/abs/gr-qc/0409007
dc.identifierGrav.Cosmol. 46 (2006) 195
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/120253
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleCounter example to a quantum inequality
dc.typetext

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