<?xml version="1.0" encoding="UTF-8"?><?xml-stylesheet type="text/xsl" href="static/style.xsl"?><OAI-PMH xmlns="http://www.openarchives.org/OAI/2.0/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/ http://www.openarchives.org/OAI/2.0/OAI-PMH.xsd"><responseDate>2026-09-21T07:38:20Z</responseDate><request verb="GetRecord" identifier="oai:www.repository.cam.ac.uk:1810/389607" metadataPrefix="uketd_dc">https://api.repository.cam.ac.uk/server/oai/request</request><GetRecord><record><header><identifier>oai:www.repository.cam.ac.uk:1810/389607</identifier><datestamp>2025-09-24T01:42:13Z</datestamp><setSpec>com_1810_205871</setSpec><setSpec>com_1810_256064</setSpec><setSpec>col_1810_206446</setSpec></header><metadata><uketd_dc:uketddc xmlns:uketd_dc="http://naca.central.cranfield.ac.uk/ethos-oai/2.0/" xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:dcterms="http://purl.org/dc/terms/" xmlns:uketdterms="http://naca.central.cranfield.ac.uk/ethos-oai/terms/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:doc="http://www.lyncode.com/xoai" xsi:schemaLocation="http://naca.central.cranfield.ac.uk/ethos-oai/2.0/ http://naca.central.cranfield.ac.uk/ethos-oai/2.0/uketd_dc.xsd">
   <dc:title>Gravitational Waves in String Cosmology</dc:title>
   <dc:identifier xsi:type="dcterms:DOI">https://doi.org/10.17863/CAM.121427</dc:identifier>
   <dc:creator>Villa, Gonzalo</dc:creator>
   <uketdterms:advisor>Quevedo, Fernando</uketdterms:advisor>
   <dcterms: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.</dcterms:abstract>
   <uketdterms:institution>University of Cambridge</uketdterms:institution>
   <dcterms:issued>2025-05-06</dcterms:issued>
   <dc:type>Thesis</dc:type>
   <uketdterms:qualificationlevel>Doctoral</uketdterms:qualificationlevel>
   <uketdterms:qualificationname>Doctor of Philosophy (PhD)</uketdterms:qualificationname>
   <dc:language>eng</dc:language>
   <uketdterms:sponsor>STFC 2602852</uketdterms:sponsor>
   <dcterms:isReferencedBy xsi:type="dcterms:URI">https://www.repository.cam.ac.uk/handle/1810/389607</dcterms:isReferencedBy>
   <dc:identifier xsi:type="dcterms:URI">https://www.repository.cam.ac.uk/bitstreams/965d6819-fabd-4a13-ac2b-e4c2fd7f9279/download</dc:identifier>
   <uketdterms:checksum xsi:type="uketdterms:MD5">4f5e00e798a685f5e53e40cfda6631db</uketdterms:checksum>
   <dcterms:license>https://www.repository.cam.ac.uk/bitstreams/2c02226a-bfd7-4ac2-b5ea-91f93b5b8547/download</dcterms:license>
   <uketdterms:checksum xsi:type="uketdterms:MD5">87eda9de84448d1f82354d60eee3eb5f</uketdterms:checksum>
   <dc:rights>https://creativecommons.org/licenses/by/4.0/</dc:rights>
   <dc:subject>Cosmology</dc:subject>
   <dc:subject>Gravitational Waves</dc:subject>
   <dc:subject>String Theory</dc:subject>
</uketd_dc:uketddc>
</metadata></record></GetRecord></OAI-PMH>