Implications of non-analytical f(R) gravity at Solar-System scales

dc.creatorLecian, O. M.
dc.creatorMontani, G.
dc.date2008-07-28
dc.date.accessioned2026-07-07T12:40:14Z
dc.date.available2026-07-07T12:40:14Z
dc.descriptionWe motivate and analyze the weak-field limit of a non-analytical Lagrangian for the gravitational field. After investigating the parameter space of the model, we impose constraints on the parameters characterizing this class of theories imposed by Solar-System data, i.e. we establish the validity range where this solution applies and refine the constraints by the comparison with planetary orbits. As a result, we claim that this class of models is viable within different astrophysical scales.
dc.description9 pages, no figures
dc.identifierhttps://arxiv.org/abs/0807.4428
dc.identifierhttp://arxiv.org/abs/0807.4428
dc.identifierClass.Quant.Grav.26:045014,2009
dc.identifierdoi:10.1088/0264-9381/26/4/045014
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/219381
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleImplications of non-analytical f(R) gravity at Solar-System scales
dc.typetext

Files

Collections