Classification of Spherically Symmetric Static Spacetimes according to their Matter Collineations

Simple item page
dc.creatorSharif, M.
dc.creatorAziz, Sehar
dc.date2003-01-10
dc.date.accessioned2026-07-07T11:29:59Z
dc.date.available2026-07-07T11:29:59Z
dc.descriptionThe spherically symmetric static spacetimes are classified according to their matter collineations. These are studied when the energy-momentum tensor is degenerate and also when it is non-degenerate. We have found a case where the energy-momentum tensor is degenerate but the group of matter collineations is finite. For the non-degenerate case, we obtain either {\it four}, {\it five}, {\it six} or {\it ten} independent matter collineations in which four are isometries and the rest are proper. We conclude that the matter collineations coincide with the Ricci collineations but the constraint equations are different which on solving can provide physically interesting cosmological solutions.
dc.description15 pages, no figure, Latex
dc.identifierhttps://arxiv.org/abs/gr-qc/0301041
dc.identifierhttp://arxiv.org/abs/gr-qc/0301041
dc.identifierGen.Rel.Grav.35:1093-1106,2003
dc.identifierdoi:10.1023/A:1024073002648
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/196892
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleClassification of Spherically Symmetric Static Spacetimes according to their Matter Collineations
dc.typetext

Files

Collections

arXiv