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.
The Oscillating Universe: an Alternative to Inflation
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abstract
The aim of this paper is to show, that the 'oscillating universe' is a viable alternative to inflation. We remind that this model provides a natural solution to the flatness or entropy and to the horizon problem of standard cosmology. We study the evolution of density perturbations and determine the power spectrum in a closed universe. The results lead to constraints of how a previous cycle might have looked like. We argue that most of the radiation entropy of the present universe may have originated from gravitational entropy produced in a previous cycle. We show that measurements of the power spectrum on very large scales could in principle decide whether our universe is closed, flat or open.
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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.