Curvature singularities, tidal forces and the viability of Palatini f(R) gravity

dc.creatorBarausse, E.
dc.creatorSotiriou, T. P.
dc.creatorMiller, J. C.
dc.date2007-12-07
dc.date2008-04-15
dc.date.accessioned2026-07-07T11:39:13Z
dc.date.available2026-07-07T11:39:13Z
dc.descriptionIn a previous paper we showed that static spherically symmetric objects which, in the vicinity of their surface, are well-described by a polytropic equation of state with 3/2<Gamma<2 exhibit a curvature singularity in Palatini f(R) gravity. We argued that this casts serious doubt on the validity of Palatini f(R) gravity as a viable alternative to General Relativity. In the present paper we further investigate this characteristic of Palatini f(R) gravity in order to clarify its physical interpretation and consequences.
dc.description15 pages. CQG in press. Part of the material moved to an appendix, discussion on the meV scale predictions of Palatini f(R) gravity added
dc.identifierhttps://arxiv.org/abs/0712.1141
dc.identifierhttp://arxiv.org/abs/0712.1141
dc.identifierClass.Quant.Grav.25:105008,2008
dc.identifierdoi:10.1088/0264-9381/25/10/105008
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/199841
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.titleCurvature singularities, tidal forces and the viability of Palatini f(R) gravity
dc.typetext

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