Scalar Field Cosmology in f(R,T) Gravity with Λ
- Авторлар: Aygün S.1, Aktaş C.2, Sahoo P.2, Bishi B.2
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Мекемелер:
- Department of Physics
- Department of Mathematics
- Шығарылым: Том 24, № 3 (2018)
- Беттер: 302-307
- Бөлім: Article
- URL: https://journals.rcsi.science/0202-2893/article/view/176218
- DOI: https://doi.org/10.1134/S0202289318030039
- ID: 176218
Дәйексөз келтіру
Аннотация
We study the behavior of cosmological parameters, massive and massless scalar fields (normal or phantom) with a scalar potential in f(R, T) theory of gravity for a flat Friedmann-Robertson-Walker (FRW) universe. To get exact solutions to the modified field equations, we use the f(R, T) = R + 2f(T) model by Harko et al. (T. Harko et al., Phys. Rev. D 84, 024020 (2011)), where R is the Ricci scalar and T is the trace of the energy momentum tensor. Our cosmological parameter solutions agree with the recent observational data. Finally, we discuss our results with various graphics.
Авторлар туралы
Sezgin Aygün
Department of Physics
Хат алмасуға жауапты Автор.
Email: saygun@comu.edu.tr
Түркия, Çanakkale, 17020
Can Aktaş
Department of Mathematics
Email: saygun@comu.edu.tr
Түркия, Çanakkale, 17020
Pradyumn Sahoo
Department of Mathematics
Email: saygun@comu.edu.tr
Үндістан, Hyderabad, 500078
Binaya Bishi
Department of Mathematics
Email: saygun@comu.edu.tr
Үндістан, Phagwara, Jalandhar, Panjab, 144401