Flat rotation curves in Chern-Simons modified gravity

Simple item page
dc.creatorKonno, Kohkichi
dc.creatorMatsuyama, Toyoki
dc.creatorAsano, Yasuhiro
dc.creatorTanda, Satoshi
dc.date2008-07-04
dc.date.accessioned2026-07-07T11:52:16Z
dc.date.available2026-07-07T11:52:16Z
dc.descriptionWe investigate the spacetime of a slowly rotating black hole in the Chern-Simons modified gravity. The long range feature of frame-dragging effect under the Chern-Simon gravity well explains the flat rotation curves of galaxies which is a central evidence of dark matter. Our solution provides a different scenario of rotating space from Goedel's solution.
dc.description4 pages, Accepted for publication in Phys. Rev. D
dc.identifierhttps://arxiv.org/abs/0807.0679
dc.identifierhttp://arxiv.org/abs/0807.0679
dc.identifierPhys.Rev.D78:024037,2008
dc.identifierdoi:10.1103/PhysRevD.78.024037
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/204175
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleFlat rotation curves in Chern-Simons modified gravity
dc.typetext

Files

Collections

arXiv