Quantum Stress Tensor Fluctuations and their Physical Effects

dc.creatorFord, L. H.
dc.creatorWu, Chun-Hsien
dc.date2007-10-19
dc.date.accessioned2026-07-07T11:12:25Z
dc.date.available2026-07-07T11:12:25Z
dc.descriptionWe summarize several aspects of recent work on quantum stress tensor fluctuations and their role in driving fluctuations of the gravitational field. The role of correlations and anticorrelations is emphasized. We begin with a review of the properties of the stress tensor correlation function. We next consider some illuminating examples of non-gravitational effects of stress tensors fluctuations, specifically fluctuations of the Casimir force and radiation pressure fluctuations. We next discuss passive fluctuations of spacetime geometry and some of their operational signatures. These include luminosity fluctuations, line broadening, and angular blurring of a source viewed through a fluctuating gravitational field. Finally, we discuss the possible role of quantum stress tensor fluctuations in the early universe, especially in inflation. The fluctuations of the expansion of a congruence of comoving geodesics grows during the inflationary era, due to non-cancellation of anticorrelations that would have occurred in flat spacetime. This results in subsequent non-Gaussian density perturbations and allows one to infer an upper bound on the duration of inflation. This bound is consistent with adequate inflation to solve the horizon and flatness problems.
dc.description15 pages, 1 figure; invited talk presented at the 3rd Mexican Meeting on Experimental and Theoretical Physics, Mexico City, September 10-14, 2007
dc.identifierhttps://arxiv.org/abs/0710.3787
dc.identifierhttp://arxiv.org/abs/0710.3787
dc.identifierAIPConf.Proc.977:145-159,2008
dc.identifierdoi:10.1063/1.2902780
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/191376
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleQuantum Stress Tensor Fluctuations and their Physical Effects
dc.typetext

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