Two f(T,𝒯) gravity models with a bouncing scale factor produce non-singular bounces with NEC and SEC violations, but the dominant energy condition claim and Model II formulas contain errors.
The scale factor must be finite and non- vanishing at the bouncing epoch, thus resolving the initial singularity problem
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Non-singular bouncing cosmology in $f(T, \mathcal{T})$ gravity with energy condition violations
Two f(T,𝒯) gravity models with a bouncing scale factor produce non-singular bounces with NEC and SEC violations, but the dominant energy condition claim and Model II formulas contain errors.