Conformal symmetric Bianchi type-I cosmologies in f(R) gravity

dc.contributor.authorTaser, Dogukan
dc.contributor.authorDogru, Melis Ulu
dc.date.accessioned2025-01-27T20:31:52Z
dc.date.available2025-01-27T20:31:52Z
dc.date.issued2018
dc.departmentÇanakkale Onsekiz Mart Üniversitesi
dc.description.abstractIn this study, we investigate the Bianchi type-I cosmologies with string cloud attached to perfect fluid in f(R) gravity. The field equations and their exact solutions for Bianchi type-I cosmologies with string cloud attached to a perfect fluid are found by using the conformal symmetry properties. The obtained solutions under the varied selection of arbitrary constants indicate three cosmological models. Isotropy conditions for obtained cosmological models are investigated for large value of time. Whether or not the string cloud in conformal symmetric Bianchi type-I universe supports the isotropy condition for the large value of time has been investigated. Also, we examine the contracting and decelerating features of the obtained solutions by using Raychaudhuri equation. Finally, geometrical and physical results of the solutions are discussed.
dc.identifier.doi10.1142/S0217732318501341
dc.identifier.issn0217-7323
dc.identifier.issn1793-6632
dc.identifier.issue23
dc.identifier.scopus2-s2.0-85050298851
dc.identifier.scopusqualityQ2
dc.identifier.urihttps://doi.org/10.1142/S0217732318501341
dc.identifier.urihttps://hdl.handle.net/20.500.12428/23292
dc.identifier.volume33
dc.identifier.wosWOS:000440170000006
dc.identifier.wosqualityQ2
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherWorld Scientific Publ Co Pte Ltd
dc.relation.ispartofModern Physics Letters A
dc.relation.publicationcategoryinfo:eu-repo/semantics/openAccess
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.snmzKA_WoS_20250125
dc.subjectModified gravity
dc.subjectstring cloud
dc.subjectconformal motion
dc.subjectf(R) gravity
dc.titleConformal symmetric Bianchi type-I cosmologies in f(R) gravity
dc.typeArticle

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