On the Construction of Nonsingular Pre-Big-Bang and Ekpyrotic Cosmologies and the Resulting Density Perturbations

TL;DR

This paper constructs nonsingular bouncing cosmological models inspired by Pre-Big-Bang and Ekpyrotic scenarios using quantum corrections, analyzing their perturbation spectra and stability.

Contribution

It introduces higher-order quantum correction terms to achieve nonsingular, bouncing solutions in Ekpyrotic models and examines their perturbation spectra and stability.

Findings

Nonsingular bouncing solutions are possible with quantum corrections.

The curvature perturbation spectrum has a large blue tilt ($n_R=3$).

Small-scale instabilities are present in the models.

Abstract

We consider the construction of nonsingular Pre-Big-Bang and Ekpyrotic type cosmological models realized by the addition to the action of specific higher-order terms stemming from quantum corrections. We study models involving general relativity coupled to a single scalar field with a potential motivated by the Ekpyrotic scenario. We find that the inclusion of the string loop and quantum correction terms in the string frame makes it possible to obtain solutions of the variational equations which are nonsingular and bouncing in the Einstein frame, even when a negative exponential potential is present, as is the case in the Ekpyrotic scenario. We analyze the spectra of perturbations produced during the bouncing phase and find that the spectrum of curvature fluctuations in the model proposed originally to implement the Ekpyrotic scenario has a large blue tilt ($n_R= 3$). Except for instabilities introduced on small scales, the result agrees with what is obtained by imposing continuity of the induced metric and of the extrinsic curvature across a constant scalar field (up to $k^2$ corrections equal to the constant energy density) matching surface between the contracting and the expanding Einstein Universes. We also discuss nonsingular cosmological solutions obtained when a Gauss-Bonnet term with a coefficient suitably dependent on the scalar matter field is added to the action in the Einstein frame with a potential for the scalar field present.