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dc.contributor.authorCaliskan, Aylin
dc.contributor.authorGudekli, Ertan
dc.date.accessioned2021-03-04T13:41:14Z
dc.date.available2021-03-04T13:41:14Z
dc.identifier.citationGudekli E., Caliskan A., "Perfect fluid LRS Bianchi type -I-Universe model in F (R, T)", 34th International Physics Congress on Turkish Physical Society, TPS 2018, Konacik-Bodrum, Türkiye, 5 - 09 Eylül 2018, cilt.2042
dc.identifier.otherav_7dbd30b6-8453-48fe-ac9e-54244f77557c
dc.identifier.othervv_1032021
dc.identifier.urihttp://hdl.handle.net/20.500.12627/85892
dc.identifier.urihttps://doi.org/10.1063/1.5078924
dc.identifier.urihttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=85057162476&origin=inward
dc.description.abstract© 2018 Author(s).In this study, the LRS (Local Rotational Symmetric) perfectly fluid Bianchi type -I-cosmological model is considered with the F(R, T) gravity. The particular case of f1(R) = λ1R and f2(T) = λ2T are considered where λ1 and λ2 are real constant. [3].
dc.language.isoeng
dc.subjectFİZİK, MULTİDİSİPLİNER
dc.subjectDisiplinlerarası Fizik ve İlgili Bilim ve Teknoloji Alanları
dc.subjectTemel Bilimler
dc.subjectTemel Bilimler (SCI)
dc.subjectFizik
dc.subjectFİZİK, UYGULAMALI
dc.titlePerfect fluid LRS Bianchi type -I-Universe model in F (R, T)
dc.typeBildiri
dc.contributor.departmentİstanbul Üniversitesi , ,
dc.identifier.volume2042
dc.contributor.firstauthorID152631


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