String Gas Cosmology and Structure Formation
Robert H. Brandenberger (McGill), Ali Nayeri (Harvard), Subodh P., Patil (McGill), Cumrun Vafa (Harvard)

TL;DR
String gas cosmology's Hagedorn phase can generate nearly scale-invariant scalar fluctuations and predicts a slight blue tilt in gravitational wave spectrum, offering an alternative to inflation-based models.
Contribution
This paper provides detailed computations supporting the mechanism of structure formation in string gas cosmology without requiring inflation.
Findings
Scalar metric fluctuations are nearly scale-invariant.
Gravitational wave spectrum exhibits a slight blue tilt.
Supports string gas cosmology as a viable alternative to inflation.
Abstract
It has recently been shown that a Hagedorn phase of string gas cosmology may provide a causal mechanism for generating a nearly scale-invariant spectrum of scalar metric fluctuations, without the need for an intervening period of de Sitter expansion. A distinctive signature of this structure formation scenario would be a slight blue tilt of the spectrum of gravitational waves. In this paper we give more details of the computations leading to these results.
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Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Pulsars and Gravitational Waves Research
