http://arxiv.org/abs/2011.00626
We introduce a set of generic conditions for the slow contracting Universe and for a narrowed-down category of models called fast-roll models. We present general conditions for super horizon freeze-out of scalar and tensor perturbations and show that any fast-roll model satisfies them, as in the case of inflation. We are interested in the “Sourced Bounce” scenario, where perturbations are sourced by a $U(1)$ gauge field coupled to a bouncer scalar field. The requirement of a slightly red tilted scalar spectrum greatly restricts the allowed couplings between the scalar and the gauge field. We show that a viable slightly red scalar spectrum is achievable. However, within the fast-roll approximation, the tensor-to-scalar ratio is in general $r\simeq 1/9$, inconsistent with current observations. We demonstrate the general result with an explicit example we dub “Intermediate contraction”. We prove that small modifications in fast-roll that do not alter the Green’s functions do not result in $r<0.06$ consistent with the data for more than an e-fold. Hence, a successful “Sourced Bounce” requires a different source or a significant deviation from fast-roll.
M. Artymowski, I. Ben-Dayan and U. Thattarampilly
Mon, 23 Aug 21
51/54
Comments: This version matches the Published version of this article. We have added an extended discussion on irrelevance of sub horizon modes
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