Pre-Big-Bang in String Cosmology
M. Gasperini, G. Veneziano

TL;DR
This paper explores the pre-big-bang phase in string cosmology, driven by duality symmetries, and discusses potential observational signatures like relic gravitons and CMB distortions.
Contribution
It introduces the concept of a pre-big-bang phase arising from string dualities and examines its possible observational evidence.
Findings
Pre-big-bang phase characterized by accelerated evolution.
Potential detection of relic gravitons as evidence.
Distortions in the cosmic microwave background may indicate pre-big-bang signatures.
Abstract
The duality-type symmetries of string cosmology naturally lead to a pre-big-bang phase of accelerated evolution as dual counterpart of the decelerated expansion of standard cosmology. We discuss several properties of this scenario, including the possibility that tracks of the pre-big-bang may be found either in the spectrum of relic gravitons or in the distortion they induce on the cosmic microwave background.
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