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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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gr-qc 1

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2024 1

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representative citing papers

Inflation after Curvature Bounce

gr-qc · 2024-12-30 · reject · novelty 4.0

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.

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  • Inflation after Curvature Bounce gr-qc · 2024-12-30 · reject · none · ref 6 · internal anchor

    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.