Cosmological Perturbation Theory in Slow-Roll Spacetimes

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dc.creatorLosic, B.
dc.creatorUnruh, W. G.
dc.date2008-04-27
dc.date2008-09-17
dc.date.accessioned2026-07-07T11:50:17Z
dc.date.available2026-07-07T11:50:17Z
dc.descriptionWe present a gauge invariant argument that a nonlocal measure of second-order metric and matter perturbations dominate that of linear fluctuations in its effect on the gravitational field in 'slow-rolling' spacetimes.
dc.descriptionVersion accepted by PRL (however, with correct non PRL format for arxiv posting). Clarified and expanded
dc.identifierhttps://arxiv.org/abs/0804.4296
dc.identifierhttp://arxiv.org/abs/0804.4296
dc.identifierPhys.Rev.Lett.101:111101,2008
dc.identifierdoi:10.1103/PhysRevLett.101.111101
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/203514
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleCosmological Perturbation Theory in Slow-Roll Spacetimes
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