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As our primary focus is on the parameters of the power spectra, we will concentrate solely on the initial two phases

Although the expression for the scale factor, the corresponding Lagrangian would be considerably extensive, the reconstruction technique remains the same · 2000

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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 3

    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.