Version 1
: Received: 27 February 2024 / Approved: 28 February 2024 / Online: 28 February 2024 (09:31:08 CET)
How to cite:
Singh, V.; Jokweni, S.; Beesham, A. FLRW Transit Cosmological Model in F (R,T) Gravity. Preprints2024, 2024021621. https://doi.org/10.20944/preprints202402.1621.v1
Singh, V.; Jokweni, S.; Beesham, A. FLRW Transit Cosmological Model in F (R,T) Gravity. Preprints 2024, 2024021621. https://doi.org/10.20944/preprints202402.1621.v1
Singh, V.; Jokweni, S.; Beesham, A. FLRW Transit Cosmological Model in F (R,T) Gravity. Preprints2024, 2024021621. https://doi.org/10.20944/preprints202402.1621.v1
APA Style
Singh, V., Jokweni, S., & Beesham, A. (2024). FLRW Transit Cosmological Model in F (R,T) Gravity. Preprints. https://doi.org/10.20944/preprints202402.1621.v1
Chicago/Turabian Style
Singh, V., Siwaphiwe Jokweni and Aroonkumar Beesham. 2024 "FLRW Transit Cosmological Model in F (R,T) Gravity" Preprints. https://doi.org/10.20944/preprints202402.1621.v1
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
Copyright:
This is an open access article distributed under the Creative Commons Attribution License which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
