Bouncing solutions in non-minimally coupled dark matter cosmology produce approximately scale-invariant scalar perturbations with compatible tensor-to-scalar ratio from the contracting phase.
Non-minimally coupled dark matter: effective pressure and structure formation.JCAP, 2012(7):027, July 2012
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Cosmology with a Non-minimally Coupled Dark Matter Fluid II. Cosmological Perturbations
Bouncing solutions in non-minimally coupled dark matter cosmology produce approximately scale-invariant scalar perturbations with compatible tensor-to-scalar ratio from the contracting phase.