Transit cosmological models coupled with zero-mass scalar-field with high redshift in higher derivative theory
Archana Dixit, Dinesh Chandra Maurya, and Anirudh Pradhan

TL;DR
This paper explores flat FRW cosmological models with a zero-mass scalar field in higher derivative gravity, presenting accelerating and transit models consistent with observations and analyzing their physical parameters.
Contribution
It introduces new cosmological models involving zero-mass scalar fields in higher derivative gravity, including transit phase models with observationally consistent parameters.
Findings
Transit redshift z_t=0.414 matches observations
EoS parameter crosses -1, indicating phantom behavior
Models yield universe age consistent with current estimates
Abstract
The present study deals with a flat FRW cosmological model filled with perfect fluid coupled with the zero-mass scalar field in the higher derivative theory of gravity. We have obtained two types of universe models, the first one is the accelerating universe (power-law cosmology) and the second one is the transit phase model (hyperbolic expansion-law). We have obtained various physical and kinematic parameters and discussed them with observationally constrained values of . The transit redshift value is obtained where the transit model shows signature-flipping and is consistent with recent observations. In our models, the present values of EoS parameter crosses the cosmological constant value . Also, the present age of the universe is calculated.
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