Growth of matter overdensities in non-minimal torsion-matter coupling theories
Manuel Gonzalez-Espinoza, Giovanni Otalora, Joel Saavedra, Nelson, Videla

TL;DR
This paper investigates how non-minimal torsion-matter coupling in $f(T)$ gravity affects the growth of matter overdensities, deriving new equations and showing potential to alleviate the $\sigma_8$ tension in cosmology.
Contribution
It extends previous $f(T)$ gravity models by including non-minimal matter-torsion coupling and analyzes its impact on matter perturbation growth and late-time cosmic acceleration.
Findings
The effective gravitational coupling is modified by the non-minimal coupling.
The model predicts a larger growth index than $\\Lambda$CDM.
It can reduce the $\\sigma_8$ tension by 4-5%.
Abstract
We study the evolution of cosmological perturbations around a homogeneous and isotropic background in the framework of the non-minimal torsion-matter coupling extension of gravity. We are concerned with the effects of the non-minimal coupling term on the growth of matter overdensities. Under the quasi-static approximation, we derive the equation which governs the evolution of matter density perturbations, and it is shown that the effective gravitational coupling 'constant' acquires an additional contribution due to the non-minimal matter-torsion coupling term. In this way, this result generalizes those previously obtained for the growth of matter overdensities in the case of minimal gravity. In order to get a feeling of our results we apply them to the important case of a power-law coupling function, which we assume to be the responsible for the late-time accelerated…
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