On Ellis' programme within fourth order gravity

Simple item page
dc.creatorSchmidt, H. -J.
dc.date2001-06-11
dc.date.accessioned2026-07-07T03:25:59Z
dc.date.available2026-07-07T03:25:59Z
dc.descriptionFor the non-tachyonic curvature squared action we show that the expanding Bianchi-type I models tend to the dust-filled Einstein-de Sitter model for t tending to infinity if the metric is averaged over the typical oscillation period. Applying a conformal equivalence between curvature squared action and a minimally coupled scalar field (which holds for all dimensions > 2) the problem is solved by discussing a massive scalar field in an anisotropic cosmological model.
dc.description9 pages, LaTeX, no figure
dc.identifierhttps://arxiv.org/abs/gr-qc/0106036
dc.identifierhttp://arxiv.org/abs/gr-qc/0106036
dc.identifierAstron.Nachr. 309 (1988) 307
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/33928
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleOn Ellis' programme within fourth order gravity
dc.typetext

Files

Collections

arXiv