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      <PublisherName>Springer Berlin Heidelberg</PublisherName>
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         <JournalID>13130</JournalID>
         <JournalDOI>10.1007/13130.1029-8479</JournalDOI>
         <JournalElectronicISSN>1029-8479</JournalElectronicISSN>
         <JournalSPIN>32745009</JournalSPIN>
         <JournalTitle>Journal of High Energy Physics</JournalTitle>
         <JournalAbbreviatedTitle>J. High Energ. Phys.</JournalAbbreviatedTitle>
         <JournalSubjectGroup>
            <JournalSubject Code="SCP" Type="Primary">Physics</JournalSubject>
            <JournalSubject Code="SCP23029" Priority="1" Type="Secondary">Elementary Particles, Quantum Field Theory</JournalSubject>
            <JournalSubject Code="SCP19048" Priority="2" Type="Secondary">Quantum Field Theories, String Theory</JournalSubject>
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            <VolumeIDStart>2023</VolumeIDStart>
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               <IssueIDStart>5</IssueIDStart>
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                  <OnlineDate>
                     <Year>2023</Year>
                     <Month>8</Month>
                     <Day>23</Day>
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                     <Year>2023</Year>
                     <Month>5</Month>
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               <IssueCopyright>
                  <CopyrightHolderName>SISSA, Trieste, Italy</CopyrightHolderName>
                  <CopyrightYear>2021</CopyrightYear>
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            <Article ID="JHEP05(2023)046">
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                  <ArticleID>20797</ArticleID>
                  <ArticleExternalID Type="arXiv">2211.05139</ArticleExternalID>
                  <ArticleDOI>10.1007/JHEP05(2023)046</ArticleDOI>
                  <ArticleCitationID>46</ArticleCitationID>
                  <ArticleSequenceNumber>46</ArticleSequenceNumber>
                  <ArticleTitle Language="En">Millicharged relics reveal massless dark photons</ArticleTitle>
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                           <CharacteristicValue Characteristic="FORCode">02</CharacteristicValue>
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                  <ArticleCategory>Regular Article - Theoretical Physics</ArticleCategory>
                  <ArticleFirstPage>1</ArticleFirstPage>
                  <ArticleLastPage>33</ArticleLastPage>
                  <ArticleHistory>
                     <RegistrationDate>
                        <Year>2023</Year>
                        <Month>5</Month>
                        <Day>5</Day>
                     </RegistrationDate>
                     <Received>
                        <Year>2022</Year>
                        <Month>11</Month>
                        <Day>21</Day>
                     </Received>
                     <Revised>
                        <Year>2023</Year>
                        <Month>4</Month>
                        <Day>12</Day>
                     </Revised>
                     <Accepted>
                        <Year>2023</Year>
                        <Month>4</Month>
                        <Day>28</Day>
                     </Accepted>
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                        <Year>2023</Year>
                        <Month>5</Month>
                        <Day>5</Day>
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                     <CopyrightYear>2023</CopyrightYear>
                     <License SubType="CC BY" Type="OpenAccess" Version="4.0">
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                           <Emphasis Type="Bold">Open Access</Emphasis>. This article is distributed under the terms of the Creative Commons Attribution License (<ExternalRef>
                              <RefSource>CC-BY 4.0</RefSource>
                              <RefTarget Address="http://creativecommons.org/licenses/by/4.0/" TargetType="URL"/>
                           </ExternalRef>), which permits any use, distribution and reproduction in any medium, provided the original author(s) and source are credited.</SimplePara>
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                     <JournalID>13130</JournalID>
                     <VolumeIDStart>2023</VolumeIDStart>
                     <VolumeIDEnd>2023</VolumeIDEnd>
                     <IssueIDStart>5</IssueIDStart>
                     <IssueIDEnd>5</IssueIDEnd>
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                  <AuthorGroup>
                     <Author AffiliationIDS="Aff1 Aff2" ID="Au1">
                        <AuthorName DisplayOrder="Western">
                           <GivenName>Asher</GivenName>
                           <FamilyName>Berlin</FamilyName>
                        </AuthorName>
                        <Contact>
                           <Email>aberlin@fnal.gov</Email>
                        </Contact>
                     </Author>
                     <Author AffiliationIDS="Aff3" ID="Au2">
                        <AuthorName DisplayOrder="Western">
                           <GivenName>Jeff</GivenName>
                           <GivenName>A.</GivenName>
                           <FamilyName>Dror</FamilyName>
                        </AuthorName>
                        <Contact>
                           <Email>jdror1@ucsc.edu</Email>
                        </Contact>
                     </Author>
                     <Author AffiliationIDS="Aff1" CorrespondingAffiliationID="Aff1" ID="Au3">
                        <AuthorName DisplayOrder="Western">
                           <GivenName>Xucheng</GivenName>
                           <FamilyName>Gan</FamilyName>
                        </AuthorName>
                        <Contact>
                           <Email>xg767@nyu.edu</Email>
                        </Contact>
                     </Author>
                     <Author AffiliationIDS="Aff1" ID="Au4">
                        <AuthorName DisplayOrder="Western">
                           <GivenName>Joshua</GivenName>
                           <GivenName>T.</GivenName>
                           <FamilyName>Ruderman</FamilyName>
                        </AuthorName>
                        <Contact>
                           <Email>ruderman@nyu.edu</Email>
                        </Contact>
                     </Author>
                     <Affiliation ID="Aff1">
                        <OrgID Level="Institution" Type="GRID">grid.137628.9</OrgID>
                        <OrgID Level="Institution" Type="ISNI">0000 0004 1936 8753</OrgID>
                        <OrgDivision>Center for Cosmology and Particle Physics, Department of Physics</OrgDivision>
                        <OrgName>New York University</OrgName>
                        <OrgAddress>
                           <City>New York</City>
                           <State>NY</State>
                           <Postcode>10003</Postcode>
                           <Country Code="US">USA</Country>
                        </OrgAddress>
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                     <Affiliation ID="Aff2">
                        <OrgID Level="Institution" Type="GRID">grid.417851.e</OrgID>
                        <OrgID Level="Institution" Type="ISNI">0000 0001 0675 0679</OrgID>
                        <OrgName>Theoretical Physics Department, Fermilab</OrgName>
                        <OrgAddress>
                           <Postbox>P.O. Box 500</Postbox>
                           <City>Batavia</City>
                           <State>IL</State>
                           <Postcode>60510</Postcode>
                           <Country Code="US">USA</Country>
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                        <OrgID Level="Institution" Type="GRID">grid.205975.c</OrgID>
                        <OrgID Level="Institution" Type="ISNI">0000 0001 0740 6917</OrgID>
                        <OrgName>Department of Physics, University of California Santa Cruz, and Santa Cruz Institute for Particle Physics</OrgName>
                        <OrgAddress>
                           <Street>1156 High St.</Street>
                           <City>Santa Cruz</City>
                           <State>CA</State>
                           <Postcode>95064</Postcode>
                           <Country Code="US">USA</Country>
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                  <Abstract ID="Abs1" Language="En" OutputMedium="All">
                     <Heading>A<Emphasis Type="SmallCaps">bstract</Emphasis>
                     </Heading>
                     <Para ID="Par1">The detection of massless kinetically-mixed dark photons is notoriously difficult, as the effect of this mixing can be removed by a field redefinition in vacuum. In this work, we study the prospect of detecting massless dark photons in the presence of a cosmic relic directly charged under this dark electromagnetism. Such millicharged particles, in the form of dark matter or dark radiation, generate an effective dark photon mass that drives photon-to-dark photon oscillations in the early universe. We also study the prospect for such models to alleviate existing cosmological constraints on massive dark photons, enlarging the motivation for direct tests of this parameter space using precision terrestrial probes.</Para>
                  </Abstract>
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                     <Heading>K<Emphasis Type="SmallCaps">eywords</Emphasis>
                     </Heading>
                     <Keyword>Cosmology of Theories BSM</Keyword>
                     <Keyword>Early Universe Particle Physics</Keyword>
                     <Keyword>Particle Nature of Dark Matter</Keyword>
                  </KeywordGroup>
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                     <SimplePara>A<Emphasis Type="SmallCaps">r</Emphasis>X<Emphasis Type="SmallCaps">iv e</Emphasis>P<Emphasis Type="SmallCaps">rint</Emphasis>: <ExternalRef>
                           <RefSource>2211.05139</RefSource>
                           <RefTarget Address="https://arxiv.org/abs/2211.05139" TargetType="URL"/>
                        </ExternalRef>
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