<?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>2026-09-22T12:46:37Z</responseDate><request verb="GetRecord" identifier="oai:www.repository.cam.ac.uk:1810/389465" metadataPrefix="uketd_dc">https://api.repository.cam.ac.uk/server/oai/request</request><GetRecord><record><header><identifier>oai:www.repository.cam.ac.uk:1810/389465</identifier><datestamp>2025-09-17T01:41:24Z</datestamp><setSpec>com_1810_214758</setSpec><setSpec>com_1810_256064</setSpec><setSpec>col_1810_219492</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>Lyα emission as a sensitive probe of galactic mergers and reionization</dc:title>
   <dc:identifier xsi:type="dcterms:DOI">https://doi.org/10.17863/CAM.121337</dc:identifier>
   <dc:creator>Yuan, Yuxuan</dc:creator>
   <uketdterms:authoridentifier xsi:type="uketdterms:ORCID">0000000168160682</uketdterms:authoridentifier>
   <uketdterms:advisor>Haehnelt, Martin</uketdterms:advisor>
   <dcterms:abstract>Lyα emission has emerged as a powerful probe of the epoch of reionization. This thesis
investigates how various physical processes shape Lyα emission and its connection to cosmic
reionization, using state-of-the-art cosmological zoom-in simulations. By post-processing
these simulations, we generate synthetic Lyα spectra for comparison with observed Lyα
emitter (LAE) populations across cosmic time. Specifically, we address the following key
questions:
• How can Lyα emission be used to probe LyC escape? We systematically explore
the spatial and spectral properties of Lyα emission, finding them to be highly sensitive
to feedback physics and the structure of the interstellar medium (ISM). We identify
several Lyα parameters that reliably predict the escape fraction of Lyman continuum
(LyC) photons.
• What governs the visibility of high-redshift LAEs? We show that galaxy mergers
trigger intense starbursts, significantly boosting Lyα luminosity. Additionally, resonant
scattering produces extended red wings in the line profiles, which enhance transmission
through the neutral intergalactic medium (IGM). Our simulations successfully
reproduce several JWST observations with the assumption of minimal interstellar dust
content.
• How can we interpret the detection of a LAE at z ∼ 13? We identify two critical
factors influencing the detectability of such early galaxies: (1) how far the red wing
in the Lyα profile can extend, and (2) the reionization history and scatter in IGM
transmission.
We conclude by summarizing the main findings of this thesis and outlining promising
directions for future research in the era of JWST and beyond.</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>
   <dcterms:isReferencedBy xsi:type="dcterms:URI">https://www.repository.cam.ac.uk/handle/1810/389465</dcterms:isReferencedBy>
   <uketdterms:embargotype>embargo</uketdterms:embargotype>
   <uketdterms:embargodate>2026-09-16</uketdterms:embargodate>
   <dc:identifier xsi:type="dcterms:URI">https://www.repository.cam.ac.uk/bitstreams/f5a05348-8b17-4ba6-95a5-e49b0924dccc/download</dc:identifier>
   <uketdterms:checksum xsi:type="uketdterms:MD5">745581a2a4d93870f535ae4f8012da5b</uketdterms:checksum>
   <dcterms:license>https://www.repository.cam.ac.uk/bitstreams/6edb9b93-f895-425f-89b0-14b3c3c7b791/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>Emission line</dc:subject>
   <dc:subject>Galaxy</dc:subject>
</uketd_dc:uketddc>
</metadata></record></GetRecord></OAI-PMH>