Requiem to "Proof of Inflation" or Sourced Fluctuations in a Non-Singular Bounce
Ido Ben-Dayan, Udaykrishna Thattarampilly

TL;DR
This paper demonstrates that a non-singular bouncing universe with sourced fluctuations can produce nearly scale-invariant spectra for both scalar and tensor perturbations, challenging the idea that measuring tensor-to-scalar ratio $r$ proves inflation.
Contribution
The study explicitly models the evolution of fluctuations across the bounce, showing that the bounce enhances scalar spectra without affecting tensors, making sourced bounce models compatible with observations.
Findings
The bounce enhances scalar fluctuations depending on its duration.
The model predicts $r \\lesssim 10^{-2}$, within future observational reach.
A sourced bounce can produce observable tensor-to-scalar ratios without inflation.
Abstract
Popular wisdom suggests that measuring the tensor to scalar ratio on CMB scales is a "proof of inflation" since one generic prediction is a scale-invariant tensor spectrum while alternatives predict that is many orders of magnitude below the sensitivity of future experiments. A bouncing Universe with sourced fluctuations allows for nearly scale-invariant spectra of both scalar and tensor perturbations challenging this point of view. Past works have analyzed the model until the bounce, under the assumption that the bounce will not change the final predictions. In this work, we discard this assumption. We explicitly follow the evolution of the Universe and fluctuations across the bounce until reheating. The evolution is stable, and the existence of the sourced fluctuations does not destroy the bounce. The bounce enhances the scalar spectrum while leaving the tensor spectrum…
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Taxonomy
TopicsCosmology and Gravitation Theories · Solar and Space Plasma Dynamics · Computational Physics and Python Applications
