<?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>2026-09-19T23:46:30Z</responseDate><request verb="GetRecord" identifier="oai:dspace.mit.edu:1721.1/143302" metadataPrefix="dim">https://dspace.mit.edu/server/oai/request</request><GetRecord><record><header><identifier>oai:dspace.mit.edu:1721.1/143302</identifier><datestamp>2022-06-16T03:10:12Z</datestamp><setSpec>com_1721.1_7582</setSpec><setSpec>com_1721.1_7581</setSpec><setSpec>col_1721.1_131023</setSpec></header><metadata><dim:dim xmlns:dim="http://www.dspace.org/xmlns/dspace/dim" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:doc="http://www.lyncode.com/xoai" xsi:schemaLocation="http://www.dspace.org/xmlns/dspace/dim http://www.dspace.org/schema/dim.xsd">
   <dim:field mdschema="dc" element="contributor" qualifier="advisor">Winslow, Lindley</dim:field>
   <dim:field mdschema="dc" element="contributor" qualifier="author">Fraker, Suzannah</dim:field>
   <dim:field mdschema="dc" element="contributor" qualifier="department">Massachusetts Institute of Technology. Department of Physics</dim:field>
   <dim:field mdschema="dc" element="date" qualifier="accessioned">2022-06-15T13:11:01Z</dim:field>
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   <dim:field mdschema="dc" element="date" qualifier="issued">2022-02</dim:field>
   <dim:field mdschema="dc" element="date" qualifier="submitted">2022-05-25T22:43:34.180Z</dim:field>
   <dim:field mdschema="dc" element="identifier" qualifier="uri">https://hdl.handle.net/1721.1/143302</dim:field>
   <dim:field mdschema="dc" element="description" qualifier="abstract">Neutrinoless double beta decay (0𝜈𝛽𝛽) is a major interest in neutrino physics. Discovery of 0𝜈𝛽𝛽 would demonstrate that neutrinos are Majorana fermions and that lepton number is not a symmetry of nature, thus providing a possible explanation for the observed matter-antimatter asymmetry of the universe. KamLAND-Zen is a leading search for 0𝜈𝛽𝛽, having placed the most stringent limit on its half-life at [formula] at 90% C.L. in ¹³⁶Xe. The next phase of KamLAND-Zen is currently running and will place even more stringent limits on the half-life. The sensitivity of KamLAND-Zen is primarily limited by backgrounds, including the muon spallation background ¹⁰C. We present a machine learning algorithm based on a convolutional neural network (CNN) that is able to separate ¹⁰C events from 136Xe events in Monte Carlo simulated data. With a typical kiloton-scale detector configuration like the KamLAND-Zen detector, we find that the algorithm is capable of identifying 61.6% of the ¹⁰C at 90% signal acceptance. The algorithm is independent of vertex and energy reconstruction, so it is complementary to current methods and can be expanded to other background sources.</dim:field>
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   <dim:field mdschema="dc" element="publisher">Massachusetts Institute of Technology</dim:field>
   <dim:field mdschema="dc" element="rights">In Copyright - Educational Use Permitted</dim:field>
   <dim:field mdschema="dc" element="rights">Copyright MIT</dim:field>
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   <dim:field mdschema="dc" element="title">Deep Learning for the KamLAND-Zen Search for 0𝜈𝛽𝛽</dim:field>
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   	&lt;Title>Deep Learning for the KamLAND-Zen Search for 0𝜈𝛽𝛽&lt;/Title>
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   	&lt;PublicationDate>2022-02&lt;/PublicationDate>
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        	&lt;DisplayName>Fraker, Suzannah&lt;/DisplayName>
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   	&lt;Abstract>Neutrinoless double beta decay (0𝜈𝛽𝛽) is a major interest in neutrino physics. Discovery of 0𝜈𝛽𝛽 would demonstrate that neutrinos are Majorana fermions and that lepton number is not a symmetry of nature, thus providing a possible explanation for the observed matter-antimatter asymmetry of the universe. KamLAND-Zen is a leading search for 0𝜈𝛽𝛽, having placed the most stringent limit on its half-life at [formula] at 90% C.L. in ¹³⁶Xe. The next phase of KamLAND-Zen is currently running and will place even more stringent limits on the half-life. The sensitivity of KamLAND-Zen is primarily limited by backgrounds, including the muon spallation background ¹⁰C. We present a machine learning algorithm based on a convolutional neural network (CNN) that is able to separate ¹⁰C events from 136Xe events in Monte Carlo simulated data. With a typical kiloton-scale detector configuration like the KamLAND-Zen detector, we find that the algorithm is capable of identifying 61.6% of the ¹⁰C at 90% signal acceptance. The algorithm is independent of vertex and energy reconstruction, so it is complementary to current methods and can be expanded to other background sources.&lt;/Abstract>
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