Spherically symmetric solutions of Einstein + non-polynomial gravities

Simple item page
dc.creatorDeser, S.
dc.creatorSarioglu, O.
dc.creatorTekin, B.
dc.date2007-05-11
dc.date.accessioned2026-07-07T10:15:58Z
dc.date.available2026-07-07T10:15:58Z
dc.descriptionWe obtain the static spherically symmetric solutions of a class of gravitational models whose additions to the General Relativity (GR) action forbid Ricci-flat, in particular, Schwarzschild geometries. These theories are selected to maintain the (first) derivative order of the Einstein equations in Schwarzschild gauge. Generically, the solutions exhibit both horizons and a singularity at the origin, except for one model that forbids spherical symmetry altogether. Extensions to arbitrary dimension with a cosmological constant, Maxwell source and Gauss-Bonnet terms are also considered.
dc.description6 pages, no figures, REVTeX 4
dc.identifierhttps://arxiv.org/abs/0705.1669
dc.identifierhttp://arxiv.org/abs/0705.1669
dc.identifierGen.Rel.Grav.40:1-7,2008
dc.identifierdoi:10.1007/s10714-007-0508-1
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/173352
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleSpherically symmetric solutions of Einstein + non-polynomial gravities
dc.typetext

Files

Collections

arXiv