Spacetime Fluctuations and the Cosmological Constant Problem

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dc.creatorMoffat, J. W.
dc.date2001-01-22
dc.date2002-03-20
dc.date.accessioned2026-07-07T03:43:44Z
dc.date.available2026-07-07T03:43:44Z
dc.descriptionSpacetime geometry is treated as a fluctuating, stochastic quantum system allowing an effective quantum gravity solution to the cosmological constant problem. A Focker-Planck equation for the probability density of spacetime metric fluctuations is solved for an FRW universe and the most probable value for the metric scale factor R is for a very small cosmological constant.
dc.descriptionLatex file. 11 pages. 1 figure
dc.identifierhttps://arxiv.org/abs/hep-ph/0101252
dc.identifierhttp://arxiv.org/abs/hep-ph/0101252
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/40332
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleSpacetime Fluctuations and the Cosmological Constant Problem
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