Cosmological effects on f(R̄,T̄) gravity through a non-standard theory

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The modified Friedmann equations reveal distinct behavior of dark energy dynamics in K-essence gravity under a flat FLRW background.
Analysis indicates a remarkable relationship between the equation of state parameter and time for varying kinetic energy conditions.
Employing the Dirac–Born–Infeld Lagrangian, this study generates novel emergent gravity metrics that diverge from traditional models.Critical understanding of dark energy density fluctuations enhances cosmological predictions.

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Randomized trial investigates dark energy dynamics in K-essence gravity, highlighting implications in cosmology.

Panda et al. (2024) studied this question.

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