String Gas Cosmology
Robert H. Brandenberger
TL;DR
String Gas Cosmology proposes a non-singular early-universe scenario in which a gas of strings on a compact space, governed by T-duality and the Hagedorn temperature $T_H$, drives the dynamics and stabilizes moduli through winding and momentum modes. A long Hagedorn phase allows three spatial dimensions to expand via winding mode annihilation, while the resulting string-thermodynamic fluctuations seed nearly scale-invariant scalar perturbations and a tensor spectrum with a characteristic blue tilt, providing an observationally testable alternative to inflation. Realization requires stabilizing the dilaton (e.g., via gaugino condensation or other non-perturbative effects) alongside radion and shape moduli stabilization, yielding a potentially consistent cosmology without initial singularities. The framework makes distinctive predictions, notably a blue-tilted tensor spectrum and testable consistency relations among observable spectra and cosmic-string signatures, though it faces challenges such as Jeans instabilities and the need for a robust non-perturbative background.
Abstract
String gas cosmology is a string theory-based approach to early universe cosmology which is based on making use of robust features of string theory such as the existence of new states and new symmetries. A first goal of string gas cosmology is to understand how string theory can effect the earliest moments of cosmology before the effective field theory approach which underlies standard and inflationary cosmology becomes valid. String gas cosmology may also provide an alternative to the current standard paradigm of cosmology, the inflationary universe scenario. Here, the current status of string gas cosmology is reviewed.
