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.
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Statistical comparison of axion-like EDE models shows n=3 yields lowest χ² and consistent photon couplings to Planck-EB and ACT-EB data, outperforming n=2 and n=∞.
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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.
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Constraining the Potential Index $n$ of the Early Dark Energy Model Using Cosmic Birefringence from Planck and ACT
Statistical comparison of axion-like EDE models shows n=3 yields lowest χ² and consistent photon couplings to Planck-EB and ACT-EB data, outperforming n=2 and n=∞.