Preprint Article Version 1 Preserved in Portico This version is not peer-reviewed

FLRW Transit Cosmological Model in F (R,T) Gravity

Version 1 : Received: 27 February 2024 / Approved: 28 February 2024 / Online: 28 February 2024 (09:31:08 CET)

A peer-reviewed article of this Preprint also exists.

Singh, V.; Jokweni, S.; Beesham, A. FLRW Transit Cosmological Model in f(R,T) Gravity. Universe 2024, 10, 272. Singh, V.; Jokweni, S.; Beesham, A. FLRW Transit Cosmological Model in f(R,T) Gravity. Universe 2024, 10, 272.

Abstract

A Friedmann-Lemaitre-Robertson-Walker space-time model with all curvatures k=0,±1 is explored in f(R,T) gravity. The solutions are obtained via the parametrization of the scale factor that leads to a model transiting from a decelerated universe to an accelerating one. The physical features of the model are discussed and analysed.

Keywords

f(R,T) gravity; dark energy; scale factor.

Subject

Physical Sciences, Astronomy and Astrophysics

Comments (0)

We encourage comments and feedback from a broad range of readers. See criteria for comments and our Diversity statement.

Leave a public comment
Send a private comment to the author(s)
* All users must log in before leaving a comment
Views 0
Downloads 0
Comments 0


×
Alerts
Notify me about updates to this article or when a peer-reviewed version is published.
We use cookies on our website to ensure you get the best experience.
Read more about our cookies here.