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.
On the generation of a scale invariant spectrum of adiabatic fluctuations in cosmological models with a contracting phase.Phys
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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.