Scalar Fields for Bianchi-I Model in $\boldsymbol{f(R,T)}$ Theory of Gravity
- 21 May 2024
- journal article
- research article
- Published by Pleiades Publishing Ltd in Gravitation and Cosmology
- Vol. 30 (2) , 222-228
Abstract
In physics and cosmology, scalar fields are considered basic. In this study, we are interested to inspect the conduct of massless scalar field (SF) and massive scalar field (MSF) models in \(f(R,T)\) theory for Bianchi-I universe models. We discuss two cosmological models with respect to late cosmic acceleration, using constant scalar potential and exponential scalar potential models. Also, we study the behavior of a massive scalar field. Finally, we obtain our results in \(f(R,T)\) and general relativity (GR). In addition, we obtained an LRS Bianchi-I metric as a result of the solutions we made and selection of special constants.
Keywords
This publication has 37 references indexed in Scilit:
- Anisotropic new holographic dark energy model in Saez–Ballester theory of gravitationAstrophysics and Space Science, 2018
- Bianchi type I universe filled with scalar field coupled with electromagnetic fields in f(R, T) theory of gravityIndian Journal of Physics, 2017
- Modified f(R,T) gravity theory and scalar field cosmologyAstrophysics and Space Science, 2014
- Cosmology from induced matter model applied to 5D f(R,T) theoryAstrophysics and Space Science, 2014
- String Cosmological Models in Lyra GeometryInternational Journal of Theoretical Physics, 2008
- Extended theories of gravity and their cosmological and astrophysical applicationsGeneral Relativity and Gravitation, 2007
- Plane-symmetric mesonic viscous fluid cosmological modelAstrophysics and Space Science, 1996
- Cylindrically symmetric and inhomogeneous cosmological models with viscous fluid, heat flux and electromagnetic fieldAstrophysics and Space Science, 1994
- Cosmological mesonic viscous fluid modelInternational Journal of Theoretical Physics, 1992
- Time-dependent cosmological termIl Nuovo Cimento B (1971-1996), 1986