A closed-universe bounce model with a reconstructed scalar Lagrangian is presented and tuned to match Planck and BICEP/Keck constraints on the spectral index and tensor-to-scalar ratio.
Einstein’s 1917 static model of the universe: a centennial review,
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Inflation after Curvature Bounce
A closed-universe bounce model with a reconstructed scalar Lagrangian is presented and tuned to match Planck and BICEP/Keck constraints on the spectral index and tensor-to-scalar ratio.