Abstract
dc:description.abstractWe 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 × 3Rights
dc:rights- Licence
- 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