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University of Cambridge

Gravitational Waves in String Cosmology

Abstract

dc:description.abstract

We study the production of cosmological backgrounds of gravitational waves in string theory models of the early universe. After a discussion of stochastic gravitational wave backgrounds, we describe the Cosmic Gravitational Wave Background (CGWB), its sensitivity to ultra-violet physics, and provide arguments supporting the claim that the peak amplitude cannot be made parametrically larger in field theory for a given reheating temperature. We then develop a Boltzmann equation approach to string thermodynamics and study a scenario where the early universe features a Hagedorn phase, with the energy density dominated by highly excited fun damental strings. We argue that the Hagedorn phase produces a gravitational wave background with a hierarchically larger amplitude and similar peak frequency to the CGWB. As an em bedding of the Hagedorn phase into a cosmologically viable setup, we describe brane-antibrane inflation and propose a mechanism that avoids the well-known η problem. Lastly, we study a complementary scenario where the byproduct of brane-antibrane inflation is a network of cosmic superstrings, where the background evolution induces variations of the string tension. We argue that the network dynamics features a scaling attractor and compute the associated gravitational wave spectrum. The spectrum can explain the signal measured by Pulsar Timing Arrays and a large class of models make concrete predictions for a spectral tilt in the LISA band. Our discussions provide further evidence that gravitational wave backgrounds (in particular at high frequencies) are a potential observational window into high-energy physics.

Degree

thesis:*
Name dc:type.qualificationname
Doctor of Philosophy (PhD)
Level dc:type.qualificationlevel
Doctoral
Grantor dc:publisher.institution
University of Cambridge
Year dc:date.issued
2025

Author and committee

dc:creator, dc:contributor.*
Author dc:creator
  • Villa, Gonzalo
Advisor dc:contributor.advisor
  • Quevedo, Fernando

Subjects

dc:subject × 3

Rights

dc:rights
Language dc:language
eng

Identifiers

dc:identifier.*
DOI dc:identifier.doi
https://doi.org/10.17863/CAM.121427
OAI identifier oai:identifier
oai:www.repository.cam.ac.uk:1810/389607

Chain of custody

source
Harvested from
Cambridge University
Base URL
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Last updated
2026-07-22
Source record
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citation

Villa, Gonzalo. Gravitational Waves in String Cosmology. Doctoral thesis, University of Cambridge, 2025. https://doi.org/10.17863/CAM.121427