The paper claims a torsion-based F(R,T) model can replace dark matter but provides no derivations, likelihoods, or data, leaving the claim unsupported.
Warm Intermediate Inflation in $F(T)$ Gravity
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abstract
We investigate warm intermediate scenario of the cosmological inflation in $F(T)$ gravity in the limit of high dissipation. The inflationary expansion is driven by the scalar inflaton while the gravitational dynamics follow from the $F(T)$ gravity. We calculate the relevant inflationary observables such as scalar-tensor ratio, power-spectrum indices of density perturbations and gravitational waves and the e-folding parameter. We obtain a ratio of slow-roll parameters to be constant. Our calculations support the warm-intermediate inflationary scenario in a spacetime with torsion. Moreover our results are compatible with the astrophysical observations of cosmic microwave background and Planck data.
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Dark Matter Constraints in Myrzakulov $F(R,T)$ Gravity: A Vielbein Approach in Weitzenb\"{o}ck Spacetime with Observational Data
The paper claims a torsion-based F(R,T) model can replace dark matter but provides no derivations, likelihoods, or data, leaving the claim unsupported.