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         <JournalTitle>Journal of High Energy Physics</JournalTitle>
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                  <OnlineDate>
                     <Year>2025</Year>
                     <Month>6</Month>
                     <Day>7</Day>
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                     <Year>2025</Year>
                     <Month>5</Month>
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               <IssueCopyright>
                  <CopyrightHolderName>SISSA, Trieste, Italy</CopyrightHolderName>
                  <CopyrightYear>2021</CopyrightYear>
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            <Article ID="JHEP05(2025)052">
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                  <ArticleID>26127</ArticleID>
                  <ArticleExternalID Type="arXiv">2412.17777</ArticleExternalID>
                  <ArticleDOI>10.1007/JHEP05(2025)052</ArticleDOI>
                  <ArticleCitationID>52</ArticleCitationID>
                  <ArticleSequenceNumber>52</ArticleSequenceNumber>
                  <ArticleTitle Language="En" OutputMedium="All">Dark gauge-mediated supersymmetry breaking with a massless dark photon</ArticleTitle>
                  <ArticleCategory>Regular Article - Theoretical Physics</ArticleCategory>
                  <ArticleFirstPage>1</ArticleFirstPage>
                  <ArticleLastPage>45</ArticleLastPage>
                  <ArticleHistory>
                     <RegistrationDate>
                        <Year>2025</Year>
                        <Month>5</Month>
                        <Day>7</Day>
                     </RegistrationDate>
                     <Received>
                        <Year>2024</Year>
                        <Month>12</Month>
                        <Day>27</Day>
                     </Received>
                     <Revised>
                        <Year>2025</Year>
                        <Month>3</Month>
                        <Day>24</Day>
                     </Revised>
                     <Accepted>
                        <Year>2025</Year>
                        <Month>3</Month>
                        <Day>27</Day>
                     </Accepted>
                     <OnlineDate>
                        <Year>2025</Year>
                        <Month>5</Month>
                        <Day>7</Day>
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                     <CopyrightHolderName>The Author(s)</CopyrightHolderName>
                     <CopyrightYear>2025</CopyrightYear>
                     <License SubType="CC BY" Type="OpenAccess" Version="4.0">
                        <SimplePara>
                           <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>
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                     <IssueIDStart>5</IssueIDStart>
                     <IssueIDEnd>5</IssueIDEnd>
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               <ArticleHeader>
                  <AuthorGroup>
                     <Author AffiliationIDS="Aff1" ID="Au1" ORCID="https://orcid.org/0000-0001-5285-5535">
                        <AuthorName DisplayOrder="Western">
                           <GivenName>Brian</GivenName>
                           <FamilyName>Batell</FamilyName>
                        </AuthorName>
                        <Contact>
                           <Email>batell@pitt.edu</Email>
                        </Contact>
                     </Author>
                     <Author AffiliationIDS="Aff2" ID="Au2" ORCID="https://orcid.org/0009-0004-5603-4549">
                        <AuthorName DisplayOrder="Western">
                           <GivenName>Yechan</GivenName>
                           <FamilyName>Kim</FamilyName>
                        </AuthorName>
                        <Contact>
                           <Email>cj7801@kaist.ac.kr</Email>
                        </Contact>
                     </Author>
                     <Author AffiliationIDS="Aff2" CorrespondingAffiliationID="Aff2" ID="Au3" ORCID="https://orcid.org/0000-0002-7333-3741">
                        <AuthorName DisplayOrder="Western">
                           <GivenName>Hye-Sung</GivenName>
                           <FamilyName>Lee</FamilyName>
                        </AuthorName>
                        <Contact>
                           <Email>hyesung.lee@kaist.ac.kr</Email>
                        </Contact>
                     </Author>
                     <Author AffiliationIDS="Aff2 Aff3" ID="Au4" ORCID="https://orcid.org/0000-0001-7235-5423">
                        <AuthorName DisplayOrder="Western">
                           <GivenName>Jiheon</GivenName>
                           <FamilyName>Lee</FamilyName>
                        </AuthorName>
                        <Contact>
                           <Email>anffl0101@kaist.ac.kr</Email>
                        </Contact>
                     </Author>
                     <Affiliation ID="Aff1">
                        <OrgID Level="Institution" Type="ROR">https://ror.org/01an3r305</OrgID>
                        <OrgID Level="Institution" Type="GRID">grid.21925.3d</OrgID>
                        <OrgID Level="Institution" Type="ISNI">0000 0004 1936 9000</OrgID>
                        <OrgDivision>Pittsburgh Particle Physics, Astrophysics, and Cosmology Center, Department of Physics and Astronomy</OrgDivision>
                        <OrgName>University of Pittsburgh</OrgName>
                        <OrgAddress>
                           <City>Pittsburgh</City>
                           <State>PA</State>
                           <Postcode>15217</Postcode>
                           <Country Code="US">USA</Country>
                        </OrgAddress>
                     </Affiliation>
                     <Affiliation ID="Aff2">
                        <OrgID Level="Institution" Type="ROR">https://ror.org/05apxxy63</OrgID>
                        <OrgID Level="Institution" Type="GRID">grid.37172.30</OrgID>
                        <OrgID Level="Institution" Type="ISNI">0000 0001 2292 0500</OrgID>
                        <OrgDivision>Department of Physics</OrgDivision>
                        <OrgName>Korea Advanced Institute of Science and Technology</OrgName>
                        <OrgAddress>
                           <City>Daejeon</City>
                           <Postcode>34141</Postcode>
                           <Country Code="KR">Korea</Country>
                        </OrgAddress>
                     </Affiliation>
                     <Affiliation ID="Aff3">
                        <OrgID Level="Institution" Type="ROR">https://ror.org/01ggx4157</OrgID>
                        <OrgID Level="Institution" Type="GRID">grid.9132.9</OrgID>
                        <OrgID Level="Institution" Type="ISNI">0000 0001 2156 142X</OrgID>
                        <OrgDivision>Theoretical Physics Department</OrgDivision>
                        <OrgName>CERN</OrgName>
                        <OrgAddress>
                           <Street>1 Esplanade des Particules</Street>
                           <Postcode>CH-1211</Postcode>
                           <City>Geneva 23</City>
                           <Country Code="CH">Switzerland</Country>
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                  <Abstract ID="Abs1" Language="En" OutputMedium="All">
                     <Heading>A<Emphasis Type="SmallCaps">bstract</Emphasis>
                     </Heading>
                     <Para ID="Par1">We study dark gauge-mediated supersymmetry breaking (dark GMSB) in a theory with a new unbroken U(1)<Subscript>
                           <Emphasis Type="Italic">D</Emphasis>
                        </Subscript> local symmetry and massless dark photon. Messenger fields charged under both Standard Model and dark gauge symmetries produce new soft supersymmetry-breaking terms due to gauge kinetic mixing between U(1)<Subscript>
                           <Emphasis Type="Italic">Y</Emphasis>
                        </Subscript> hypercharge and U(1)<Subscript>
                           <Emphasis Type="Italic">D</Emphasis>
                        </Subscript>. We show that large kinetic mixing induces significant distortions to the superpartner spectra relative to conventional GMSB. Notably, shifts in the Higgs soft masses impact the conditions for electroweak symmetry breaking, lowering the <Emphasis Type="Italic">μ</Emphasis> parameter and yielding a relatively light Higgsino that may be accessible at the LHC. Furthermore, for very simple messenger representations, a very light bino-dark photino mixed state is present in the spectrum, which may be probed through exotic Higgs boson decays at future Higgs factories. We also examine the cosmological and phenomenological consequences of the messengers, the lightest of which is absolutely stable and carries fractional electric charge.</Para>
                  </Abstract>
                  <KeywordGroup Language="En" OutputMedium="All" Source="Author">
                     <Heading>K<Emphasis Type="SmallCaps">eywords</Emphasis>
                     </Heading>
                     <Keyword>Supersymmetry</Keyword>
                     <Keyword>New Gauge Interactions</Keyword>
                     <Keyword>New Light Particles</Keyword>
                  </KeywordGroup>
                  <ArticleNote Type="Misc">
                     <SimplePara>A<Emphasis Type="SmallCaps">r</Emphasis>X<Emphasis Type="SmallCaps">iv e</Emphasis>P<Emphasis Type="SmallCaps">rint</Emphasis>: <ExternalRef>
                           <RefSource>2412.17777</RefSource>
                           <RefTarget Address="https://arxiv.org/abs/2412.17777" TargetType="URL"/>
                        </ExternalRef>
                     </SimplePara>
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