Matter collineation classification of Bianchi type II spacetime

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dc.authoridCamci, Ugur/0000-0003-3431-2574
dc.contributor.authorCamci, U.
dc.contributor.authorSahin, E.
dc.date.accessioned2025-01-27T20:41:09Z
dc.date.available2025-01-27T20:41:09Z
dc.date.issued2006
dc.departmentÇanakkale Onsekiz Mart Üniversitesi
dc.description.abstractIn this paper we classified the matter collineations (MCs) of Bianchi type II spacetime according to the degenerate and non-degenerate energy-momentum tensor. It is shown that when the energy-momentum tensor is degenerate, most of the cases yield infinite dimensional MCs whereas some cases give finite dimensional Lie algebras in which there are three, four or five MCs. For the non-degenerate matter tensor cases we obtained that the Lie algebra of MCs is finite dimensional, in which the number of MCs are also three, four or five. Furthermore, we discussed the physical implications of the obtained MCs in the case of perfect fluid as source.
dc.identifier.doi10.1007/s10714-006-0312-3
dc.identifier.endpage1346
dc.identifier.issn0001-7701
dc.identifier.issn1572-9532
dc.identifier.issue9
dc.identifier.scopus2-s2.0-33747890856
dc.identifier.scopusqualityQ2
dc.identifier.startpage1331
dc.identifier.urihttps://doi.org/10.1007/s10714-006-0312-3
dc.identifier.urihttps://hdl.handle.net/20.500.12428/24038
dc.identifier.volume38
dc.identifier.wosWOS:000240057300001
dc.identifier.wosqualityQ2
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherSpringer/Plenum Publishers
dc.relation.ispartofGeneral Relativity and Gravitation
dc.relation.publicationcategoryinfo:eu-repo/semantics/openAccess
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.snmzKA_WoS_20250125
dc.subjectmatter collineations
dc.subjectBianchi type II spacetime
dc.titleMatter collineation classification of Bianchi type II spacetime
dc.typeArticle

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