Scalar field cosmologies with inverted potentials Auteur(s): Boisseau Bruno, Giacomini Hector, Polarski D. (Article) Publié: Journal Of Cosmology And Astroparticle Physics, vol. p. (2015) Texte intégral en Openaccess : Ref HAL: hal-01266923_v1 DOI: 10.1088/1475-7516/2015/10/033 WoS: 000365804000034 Exporter : BibTex | endNote 9 Citations Résumé: Regular bouncing solutions in the framework of a scalar-tensor gravity model were found in a recent work. We reconsider the problem in the Einstein frame (EF) in the present work. Singularities arising at the limit of physical viability of the model in the Jordan frame (JF) are either of the Big Bang or of the Big Crunch type in the EF. As a result we obtain integrable scalar field cosmological models in general relativity (GR) with inverted double-well potentials unbounded from below which possess solutions regular in the future, tending to a de Sitter space, and starting with a Big Bang. The existence of the two fixed points for the field dynamics at late times found earlier in the JF becomes transparent in the EF. |