Perfect fluid LRS Bianchi type -I-Universe model in F (R, T)

dc.contributor.author	Caliskan, Aylin
dc.contributor.author	Gudekli, Ertan
dc.date.accessioned	2021-03-04T13:41:14Z
dc.date.available	2021-03-04T13:41:14Z
dc.identifier.citation	Gudekli 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.other	av_7dbd30b6-8453-48fe-ac9e-54244f77557c
dc.identifier.other	vv_1032021
dc.identifier.uri	http://hdl.handle.net/20.500.12627/85892
dc.identifier.uri	https://doi.org/10.1063/1.5078924
dc.identifier.uri	https://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.iso	eng
dc.subject	FİZİK, MULTİDİSİPLİNER
dc.subject	Disiplinlerarası Fizik ve İlgili Bilim ve Teknoloji Alanları
dc.subject	Temel Bilimler
dc.subject	Temel Bilimler (SCI)
dc.subject	Fizik
dc.subject	FİZİK, UYGULAMALI
dc.title	Perfect fluid LRS Bianchi type -I-Universe model in F (R, T)
dc.type	Bildiri
dc.contributor.department	İstanbul Üniversitesi , ,
dc.identifier.volume	2042
dc.contributor.firstauthorID	152631

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