Reconstruction, Thermodynamics and Stability of $\Lambda$CDM Model in $f(T,\mathcal{T})$ Gravity
Ednaldo L. B. Junior, Manuel E. Rodrigues, Ines G. Salako, Mahouton, J. S. Houndjo

TL;DR
This paper reconstructs the $ ext{Lambda}$CDM model within $f(T, ext{T})$ gravity, analyzing its thermodynamics, stability, and how it describes cosmological evolution, revealing conditions for energy-momentum conservation and thermodynamic laws.
Contribution
It introduces a novel reconstruction of $ ext{Lambda}$CDM in $f(T, ext{T})$ gravity, exploring stability and thermodynamics, and identifies conditions for conservation and physical viability.
Findings
The $ ext{Lambda}$CDM action includes linear, constant, and non-linear terms in $f(T, ext{T})$.
Energy-momentum conservation requires $F_g$ to be linear in $ ext{T}$.
The model is stable under perturbations except for the geometric part in de Sitter space.
Abstract
We reconstruct the CDM model for Theory, where is the torsion scalar and the trace of the energy-momentum tensor. The result shows that the action of CDM is a combination of a linear term, a constant () and a non-linear term given by the product , with being a generic function. We show that to maintain conservation of energy-momentum tensor should impose that must be linear on the trace . This reconstruction decays in the Theory for , with a constant. Our reconstruction describes the cosmological eras to the present time. The model present stability within the geometric and matter perturbations for the choice , where $y=(T^{1/3}/16\pi G)\left(16\pi…
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