Testing the viability of $f(T, \mathcal{T})$ gravity models via effective equation of state constraints
M. Koussour, O. Donmez, S. Bekov, A. Syzdykova, S. Muminov, A.I., Ashirova

TL;DR
This study tests the $f(T, \\mathcal{T})$ gravity model against observational data, finding it consistent with current cosmic acceleration evidence and supporting its potential as a dark energy framework.
Contribution
It introduces a specific $f(T, \\mathcal{T})$ model and constrains its parameters using observational data, demonstrating its viability for explaining cosmic acceleration.
Findings
Best-fit parameters align with observational data
Supports a universe transitioning from deceleration to acceleration
EoS parameter indicates quintessence-like dark energy
Abstract
This paper rigorously examines the potential of the theory as a promising framework for understanding the dark sector of the universe, particularly in relation to cosmic acceleration. The theory extends gravitational dynamics by incorporating both the torsion scalar and the trace of the energy-momentum tensor . Further, we explore the functional form , where is a free parameter that modulates the matter's influence on spacetime evolution. To evaluate this model, we employ an effective EoS parameter dependent on redshift , to solve the field equations and analyze the evolution of the Hubble parameter . Using a joint dataset () and the Markov Chain Monte Carlo (MCMC) method with Bayesian analysis, we obtain the best-fit parameter values: $H_0 = 68.04 \pm…
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Taxonomy
TopicsGeophysics and Gravity Measurements · Cosmology and Gravitation Theories · Computational Physics and Python Applications
