Bianchi Type-I Universe in Lyra Manifold with Quadratic Equation of State

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dc.contributor.authorSen, R.
dc.contributor.authorAygun, S.
dc.date.accessioned2025-01-27T20:56:11Z
dc.date.available2025-01-27T20:56:11Z
dc.date.issued2017
dc.departmentÇanakkale Onsekiz Mart Üniversitesi
dc.description32nd International Physics Congress of Turkish-Physical-Society (TPS) -- SEP 06-09, 2016 -- Bodrum, TURKEY
dc.description.abstractIn this study, we have solved Einstein field equations for Bianchi type I universe model in Lyra manifold with quadratic equation of state (EoS) p = alpha rho(t)(2) - rho(t). Where alpha not equal 0 is an important constant. Cosmic pressure, density and displacement vector (beta(2)) are related with a constant. In this study beta(2) is a decreasing function of time and behaves like a cosmological constant. These solutions agree with the studies of lialford, Pradhan and Singh, Aygun et al., Agarwal et al., Yadav and liaque as well as SN la observations.
dc.description.sponsorshipTurkish Phys Soc
dc.identifier.doi10.1063/1.4976455
dc.identifier.isbn978-0-7354-1483-9
dc.identifier.issn0094-243X
dc.identifier.scopus2-s2.0-85015979419
dc.identifier.scopusqualityQ4
dc.identifier.urihttps://doi.org/10.1063/1.4976455
dc.identifier.urihttps://hdl.handle.net/20.500.12428/26329
dc.identifier.volume1815
dc.identifier.wosWOS:000435205100111
dc.identifier.wosqualityN/A
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherAmer Inst Physics
dc.relation.ispartofProceedings of The Turkish Physical Society 32nd International Physics Congress (Tps32)
dc.relation.publicationcategoryKonferans Öğesi - Uluslararası - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.snmzKA_WoS_20250125
dc.subjectScalar-Tensor Theory
dc.subjectCosmological Models
dc.titleBianchi Type-I Universe in Lyra Manifold with Quadratic Equation of State
dc.typeConference Object

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