Gravitational radiation from collapsing magnetized dust

Simple item page
dc.creatorSotani, Hajime
dc.creatorYoshida, Shijun
dc.creatorKokkotas, Kostas D.
dc.date2007-02-15
dc.date.accessioned2026-07-07T11:01:44Z
dc.date.available2026-07-07T11:01:44Z
dc.descriptionIn this article we study the influence of magnetic fields on the axial gravitational waves emitted during the collapse of a homogeneous dust sphere. We found that while the energy emitted depends weakly on the initial matter perturbations it has strong dependence on the strength and the distribution of the magnetic field perturbations. The gravitational wave output of such a collapse can be up to an order of magnitude larger or smaller calling for detailed numerical 3D studies of collapsing magnetized configurations.
dc.identifierhttps://arxiv.org/abs/gr-qc/0702091
dc.identifierhttp://arxiv.org/abs/gr-qc/0702091
dc.identifierPhys.Rev.D75:084015,2007
dc.identifierdoi:10.1103/PhysRevD.75.084015
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/188037
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleGravitational radiation from collapsing magnetized dust
dc.typetext

Files

Collections

arXiv