Rotating Braneworld Black Holes

Simple item page
dc.creatorAliev, Alikram N.
dc.date2006-12-26
dc.date.accessioned2026-07-07T07:37:05Z
dc.date.available2026-07-07T07:37:05Z
dc.descriptionWe present a Kerr-Newman type stationary and axisymmetric solution that describes rotating black holes with a tidal charge in the Randall-Sundrum braneworld. The tidal charge appears as an imprint of nonlocal gravitational effects from the bulk space. We also discuss the physical properties of these black holes and their possible astrophysical appearance.
dc.descriptionTo appear in the Proceedings of the Eleventh Marcel Grossmann Meeting, Berlin, Germany, 23-29 Jule 2006, 3pp., World Scientific, Singapore (2007)
dc.identifierhttps://arxiv.org/abs/astro-ph/0612735
dc.identifierhttp://arxiv.org/abs/astro-ph/0612735
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/120656
dc.subjectAstrophysics
dc.titleRotating Braneworld Black Holes
dc.typetext

Files

Collections

arXiv