Compatibility between the scalar field models of tachyon, $k$-essence and quintessence in $f(R, T)$ gravity
Vinod Kumar Bhardwaj, Anirudh Pradhan, Archana Dixit

TL;DR
This paper explores the compatibility of tachyon, k-essence, and quintessence scalar field models within $f(R,T)$ gravity, analyzing their potentials and dynamics in a flat FRW universe using observational data.
Contribution
It introduces a unified analysis of multiple scalar field models in $f(R,T)$ gravity and reconstructs their potentials consistent with observational cosmological parameters.
Findings
Models align well with observational data
Reconstructed potentials exhibit scaling behavior
Scalar fields' dynamics are consistent with universe's expansion
Abstract
We investigate the behavior of the scalar field in gravity (Harko et al., Phys. Rev. D 84, 024020, 2011) inside the structure of a flat FRW cosmological model, where and have their usual meaning. The deterministic solution of FEs has been settled by considering the scale factor , where and are positive constant. Here we utilize three ongoing imperatives ( and ) from SNe Ia Union observation (Cunha, Phys. Rev. D 79, 047301, 2009); ( and ) from Type Ia Supernova (SNIa) observation in joined with (BAO) and (CMB) observation (Giostri et al., J. Cosmol. Astropart. Phys. 03, 027, 2012); and ( and 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…
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