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• W3048607102 endingPage "101478" @default.
• W3048607102 startingPage "101478" @default.
• W3048607102 abstract "We investigate the behavior of the scalar field in $f (R, T )$ gravity (Harko et al., Phys. Rev. D 84, 024020, 2011) inside the structure of a flat FRW cosmological model, where $R$ and $T$ have their usual meaning. The deterministic solution of FEs has been settled by considering the scale factor $S(t) = t^{m}e^{kt}$, where $m$ and $k$ are positive constant. Here we utilize three ongoing imperatives ($H_{0}=73.8$ and $ q_{0}=-0.73$) from SNe Ia Union observation (Cunha, Phys. Rev. D 79, 047301, 2009); ($H_{0}=73.8$ and $ q_{0}=-0.55$) from Type Ia Supernova (SNIa) observation in joined with (BAO) and (CMB) observation (Giostri et al., J. Cosmol. Astropart. Phys. 03, 027, 2012); and ($H_{0}=69.2$ and $q_{0}=-0.52)$ from (OHD+JLA) observation (Yu et al., Astrophys. J. 856, 3, 2018). We have measured and graphed several cosmological parameters and found that these findings are appropriate in comparison with the universe's physical and kinematic properties and also compatible with ongoing observations. The correspondence between the scalar field models of tachyon, k-essence, and quintessence is investigated by us. Our model explains the potentials and the dynamics of the scalar fields in the FRW universe. The reconstructed potential is very sensible and has a scaling arrangement. Subsequently, our study supports recent observations." @default.
• W3048607102 created "2020-08-18" @default.
• W3048607102 creator A5007622015 @default.
• W3048607102 creator A5010583085 @default.
• W3048607102 creator A5021728811 @default.
• W3048607102 date "2021-02-01" @default.
• W3048607102 modified "2023-09-26" @default.
• W3048607102 title "Compatibility between the scalar field models of tachyon, k-essence and quintessence in f(R, T) gravity" @default.
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• W3048607102 doi "https://doi.org/10.1016/j.newast.2020.101478" @default.
• W3048607102 hasPublicationYear "2021" @default.
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