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dc.contributor.authorCamci, U
dc.contributor.authorYavuz, I
dc.date.accessioned2021-03-02T20:27:52Z
dc.date.available2021-03-02T20:27:52Z
dc.date.issued2003
dc.identifier.citationCamci U., Yavuz I., "Classifications of Kantowski-Sachs, Bianchi types I and III spacetimes according to Ricci collineations", INTERNATIONAL JOURNAL OF MODERN PHYSICS D, cilt.12, sa.1, ss.89-100, 2003
dc.identifier.issn0218-2718
dc.identifier.othervv_1032021
dc.identifier.otherav_022289e3-156b-47b6-addc-7a93412e44f3
dc.identifier.urihttp://hdl.handle.net/20.500.12627/7381
dc.identifier.urihttps://doi.org/10.1142/s0218271803002354
dc.description.abstractThe Ricci collineation classifications of Kantowski-Sachs, Bianchi types I and III space-times are studied according to their degenerate and non-degenerate Ricci tensor. When the Ricci tensor is degenerate, the special cases are classified and it is shown that there are many cases of Ricci collineations (RCs) with infinite number of degrees of freedom, and the group of RCs is ten-dimensional in some spacial cases. Furthermore, it is found that when the Ricci tensor is non-degenerate, the group of RCs is finite-dimensional, and we have only either four which coincides with the isometries or six proper RCs in addition to the four isometries.
dc.language.isoeng
dc.subjectFizik
dc.subjectTemel Bilimler
dc.subjectAstronomi ve Astrofizik
dc.subjectTemel Bilimler (SCI)
dc.subjectUzay bilimi
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.titleClassifications of Kantowski-Sachs, Bianchi types I and III spacetimes according to Ricci collineations
dc.typeMakale
dc.relation.journalINTERNATIONAL JOURNAL OF MODERN PHYSICS D
dc.contributor.department, ,
dc.identifier.volume12
dc.identifier.issue1
dc.identifier.startpage89
dc.identifier.endpage100
dc.contributor.firstauthorID167082


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