Cosmological Structure Problem of the Pre-Big Bang Scenario
J. Hwang

TL;DR
This paper calculates the density and gravitational wave spectra in a string cosmology pre-big bang scenario, finding significant deviations from observed large-scale structure spectra, thus questioning its viability for explaining current observations.
Contribution
It provides detailed spectral predictions for density and gravitational waves in the pre-big bang string cosmology model, highlighting discrepancies with observational data.
Findings
Spectra are tilted with n ~ 4 and n_T ~ 3, differing from observed values.
Pre-big bang scenario may not generate observable large-scale structures.
Quantum corrections might be necessary for better agreement.
Abstract
We calculate the density and gravitational wave spectrums generated in a version of string cosmology termed pre-big bang scenario. The large scale structures are originated from quantum fluctuations of the metric and dilaton field during a pole-like inflation stage driven by a potential-less dilaton field realized in the low-energy effective action of string theory. The generated classical density field and the gravitational wave in the second horizon crossing epoch show tilted spectrums with n ~ 4 and n_T ~ 3, respectively. These differ from the observed spectrum of the large angular scale anisotropy of the cosmic microwave background radiation which supports scale invariant ones with n ~ 1 and n_T ~ 0. This suggests that the pre-big bang stage is not suitable for generating the present day observable large scale structures, and suggests the importance of investigating the quantum…
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