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FLRW cosmological model in f(R,T) gravity

In this paper, the Friedmann-Lemaitre-Robertson-Walker cosmological models with a perfect fluid in the f(R,T) theory of gravity are re-discussed. There are several ways to generate solutions. One way is to assume a barotropic equation of state. The other is to use a deceleration parameter that varie...

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Detaylı Bibliyografya
Yazar: Aroonkumar Beesham
Materyal Türü: Artigo
Dil:Inglês
Baskı/Yayın Bilgisi: V.N. Karazin Kharkiv National University Publishing 2024-12-01
Seri Bilgileri:East European Journal of Physics
Konular:
Online Erişim:https://periodicals.karazin.ua/eejp/article/view/24443
Etiketler: Etiketle
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