The stability of a bouncing universe

Simple item page
dc.creatorNovello, M.
dc.creatorSalim, J. M.
dc.date2003-05-29
dc.date2003-12-05
dc.date.accessioned2026-07-07T04:15:17Z
dc.date.available2026-07-07T04:15:17Z
dc.descriptionWe investigate the stability of a spatially homogeneous and isotropic non-singular cosmological model. We show that the complete set of independent perturbations (the electric part of the perturbed Weyl tensor and the perturbed shear) are regular and well behaved functions which have no divergences, contrary to previous claims in the literature.
dc.description9 pages, no figures
dc.identifierhttps://arxiv.org/abs/hep-th/0305254
dc.identifierhttp://arxiv.org/abs/hep-th/0305254
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/51946
dc.subjectHigh Energy Physics - Theory
dc.titleThe stability of a bouncing universe
dc.typetext

Files

Collections

arXiv