<?xml version="1.0" encoding="UTF-8"?><Publisher>
   <PublisherInfo>
      <PublisherName>Springer Berlin Heidelberg</PublisherName>
      <PublisherLocation>Berlin/Heidelberg</PublisherLocation>
      <PublisherImprintName>Springer</PublisherImprintName>
   </PublisherInfo>
   <Journal OutputMedium="Online">
      <JournalInfo JournalProductType="ArchiveJournal" NumberingStyle="Unnumbered" OutputMedium="Online">
         <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>
            <JournalSubject Code="SCP19070" Priority="3" Type="Secondary">Classical and Quantum Gravitation, Relativity Theory</JournalSubject>
            <JournalSubject Code="SCP19080" Priority="4" Type="Secondary">Quantum Physics</JournalSubject>
            <SubjectCollection Code="SC12">Physics and Astronomy</SubjectCollection>
         </JournalSubjectGroup>
      </JournalInfo>
      <Volume OutputMedium="Online">
         <VolumeInfo OutputMedium="Online" TocLevels="0" VolumeType="Regular">
            <VolumeIDStart>2024</VolumeIDStart>
            <VolumeIDEnd>2024</VolumeIDEnd>
            <VolumeIssueCount>12</VolumeIssueCount>
         </VolumeInfo>
         <Issue IssueType="Regular" OutputMedium="Online">
            <IssueInfo IssueType="Regular" OutputMedium="Online" TocLevels="0">
               <IssueIDStart>6</IssueIDStart>
               <IssueIDEnd>6</IssueIDEnd>
               <IssueArticleCount>216</IssueArticleCount>
               <IssueHistory>
                  <OnlineDate>
                     <Year>2024</Year>
                     <Month>9</Month>
                     <Day>23</Day>
                  </OnlineDate>
                  <CoverDate>
                     <Year>2024</Year>
                     <Month>6</Month>
                  </CoverDate>
                  <PricelistYear>2024</PricelistYear>
               </IssueHistory>
               <IssueCopyright>
                  <CopyrightHolderName>SISSA, Trieste, Italy</CopyrightHolderName>
                  <CopyrightYear>2021</CopyrightYear>
               </IssueCopyright>
            </IssueInfo>
            <Article ID="JHEP06(2024)172">
               <ArticleInfo ArticleType="OriginalPaper" ContainsESM="No" Language="En" NumberingStyle="ContentOnly" OutputMedium="Online" TocLevels="0">
                  <ArticleID>23792</ArticleID>
                  <ArticleExternalID Type="arXiv">2402.19208</ArticleExternalID>
                  <ArticleDOI>10.1007/JHEP06(2024)172</ArticleDOI>
                  <ArticleCitationID>172</ArticleCitationID>
                  <ArticleSequenceNumber>172</ArticleSequenceNumber>
                  <ArticleTitle Language="En">Deciphering the Belle II data on <InlineEquation ID="IEq1">
                        <EquationSource Format="MATHML">
                           <math xmlns:xlink="http://www.w3.org/1999/xlink" display="inline">
                              <mi>B</mi>
                              <mo>→</mo>
                              <mi mathvariant="italic">Kν</mi>
                              <mover accent="true">
                                 <mi>ν</mi>
                                 <mo stretchy="true">¯</mo>
                              </mover>
                           </math>
                        </EquationSource>
                        <EquationSource Format="TEX">$$ B\to K\nu \overline{\nu} $$</EquationSource>
                     </InlineEquation> decay in the (dark) SMEFT with minimal flavour violation</ArticleTitle>
                  <ArticleCategory>Regular Article - Theoretical Physics</ArticleCategory>
                  <ArticleFirstPage>1</ArticleFirstPage>
                  <ArticleLastPage>48</ArticleLastPage>
                  <ArticleHistory>
                     <RegistrationDate>
                        <Year>2024</Year>
                        <Month>6</Month>
                        <Day>25</Day>
                     </RegistrationDate>
                     <Received>
                        <Year>2024</Year>
                        <Month>3</Month>
                        <Day>15</Day>
                     </Received>
                     <Accepted>
                        <Year>2024</Year>
                        <Month>5</Month>
                        <Day>29</Day>
                     </Accepted>
                     <OnlineDate>
                        <Year>2024</Year>
                        <Month>6</Month>
                        <Day>25</Day>
                     </OnlineDate>
                  </ArticleHistory>
                  <ArticleCopyright>
                     <CopyrightHolderName>The Author(s)</CopyrightHolderName>
                     <CopyrightYear>2024</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>
                     </License>
                  </ArticleCopyright>
                  <ArticleGrants Type="OpenChoice">
                     <MetadataGrant Grant="OpenAccess"/>
                     <AbstractGrant Grant="OpenAccess"/>
                     <BodyPDFGrant Grant="OpenAccess"/>
                     <BodyHTMLGrant Grant="OpenAccess"/>
                     <BibliographyGrant Grant="OpenAccess"/>
                     <ESMGrant Grant="OpenAccess"/>
                  </ArticleGrants>
                  <ArticleContext>
                     <JournalID>13130</JournalID>
                     <VolumeIDStart>2024</VolumeIDStart>
                     <VolumeIDEnd>2024</VolumeIDEnd>
                     <IssueIDStart>6</IssueIDStart>
                     <IssueIDEnd>6</IssueIDEnd>
                  </ArticleContext>
               </ArticleInfo>
               <ArticleHeader>
                  <AuthorGroup>
                     <Author AffiliationIDS="Aff1" ID="Au1" ORCID="http://orcid.org/0000-0001-9909-9829">
                        <AuthorName DisplayOrder="Western">
                           <GivenName>Biao-Feng</GivenName>
                           <FamilyName>Hou</FamilyName>
                        </AuthorName>
                        <Contact>
                           <Email>resonhou@zknu.edu.cn</Email>
                        </Contact>
                     </Author>
                     <Author AffiliationIDS="Aff1 Aff2" ID="Au2" ORCID="http://orcid.org/0000-0002-3962-3577">
                        <AuthorName DisplayOrder="Western">
                           <GivenName>Xin-Qiang</GivenName>
                           <FamilyName>Li</FamilyName>
                        </AuthorName>
                        <Contact>
                           <Email>xqli@ccnu.edu.cn</Email>
                        </Contact>
                     </Author>
                     <Author AffiliationIDS="Aff1" ID="Au3" ORCID="http://orcid.org/0009-0004-7172-5196">
                        <AuthorName DisplayOrder="Western">
                           <GivenName>Meng</GivenName>
                           <FamilyName>Shen</FamilyName>
                        </AuthorName>
                        <Contact>
                           <Email>shenmeng@mails.ccnu.edu.cn</Email>
                        </Contact>
                     </Author>
                     <Author AffiliationIDS="Aff1 Aff3" ID="Au4" ORCID="http://orcid.org/0000-0002-9327-0557">
                        <AuthorName DisplayOrder="Western">
                           <GivenName>Ya-Dong</GivenName>
                           <FamilyName>Yang</FamilyName>
                        </AuthorName>
                        <Contact>
                           <Email>yangyd@ccnu.edu.cn</Email>
                        </Contact>
                     </Author>
                     <Author AffiliationIDS="Aff1" CorrespondingAffiliationID="Aff1" ID="Au5" ORCID="http://orcid.org/0000-0002-5647-2563">
                        <AuthorName DisplayOrder="Western">
                           <GivenName>Xing-Bo</GivenName>
                           <FamilyName>Yuan</FamilyName>
                        </AuthorName>
                        <Contact>
                           <Email>y@ccnu.edu.cn</Email>
                        </Contact>
                     </Author>
                     <Affiliation ID="Aff1">
                        <OrgID Level="Institution" Type="ROR">https://ror.org/03x1jna21</OrgID>
                        <OrgID Level="Institution" Type="GRID">grid.411407.7</OrgID>
                        <OrgID Level="Institution" Type="ISNI">0000 0004 1760 2614</OrgID>
                        <OrgDivision>Institute of Particle Physics and Key Laboratory of Quark and Lepton Physics (MOE)</OrgDivision>
                        <OrgName>Central China Normal University</OrgName>
                        <OrgAddress>
                           <City>Wuhan</City>
                           <Postcode>430079</Postcode>
                           <State>Hubei</State>
                           <Country Code="CN">China</Country>
                        </OrgAddress>
                     </Affiliation>
                     <Affiliation ID="Aff2">
                        <OrgID Level="Institution" Type="ROR">https://ror.org/02v51f717</OrgID>
                        <OrgID Level="Institution" Type="GRID">grid.11135.37</OrgID>
                        <OrgID Level="Institution" Type="ISNI">0000 0001 2256 9319</OrgID>
                        <OrgDivision>Center for High Energy Physics</OrgDivision>
                        <OrgName>Peking University</OrgName>
                        <OrgAddress>
                           <City>Beijing</City>
                           <Postcode>100871</Postcode>
                           <Country Code="CN">China</Country>
                        </OrgAddress>
                     </Affiliation>
                     <Affiliation ID="Aff3">
                        <OrgID Level="Institution" Type="ROR">https://ror.org/00s13br28</OrgID>
                        <OrgID Level="Institution" Type="GRID">grid.462338.8</OrgID>
                        <OrgID Level="Institution" Type="ISNI">0000 0004 0605 6769</OrgID>
                        <OrgDivision>Institute of Particle and Nuclear Physics</OrgDivision>
                        <OrgName>Henan Normal University</OrgName>
                        <OrgAddress>
                           <City>Xinxiang</City>
                           <Postcode>453007</Postcode>
                           <Country Code="CN">China</Country>
                        </OrgAddress>
                     </Affiliation>
                  </AuthorGroup>
                  <Abstract ID="Abs1" Language="En" OutputMedium="All">
                     <Heading>A<Emphasis Type="SmallCaps">bstract</Emphasis>
                     </Heading>
                     <Para ID="Par1">Recently, the Belle II collaboration announced the first measurement of the branching ratio <InlineEquation ID="IEq2">
                           <EquationSource Format="MATHML">
                              <math xmlns:xlink="http://www.w3.org/1999/xlink" display="inline">
                                 <mi mathvariant="script">B</mi>
                                 <mfenced close=")" open="(">
                                    <mrow>
                                       <msup>
                                          <mi>B</mi>
                                          <mo>+</mo>
                                       </msup>
                                       <mo>→</mo>
                                       <msup>
                                          <mi>K</mi>
                                          <mo>+</mo>
                                       </msup>
                                       <mi>ν</mi>
                                       <mover accent="true">
                                          <mi>ν</mi>
                                          <mo stretchy="true">¯</mo>
                                       </mover>
                                    </mrow>
                                 </mfenced>
                              </math>
                           </EquationSource>
                           <EquationSource Format="TEX">$$ \mathcal{B}\left({B}^{+}\to {K}^{+}\nu \overline{\nu}\right) $$</EquationSource>
                        </InlineEquation>, which is found to be about 2<Emphasis Type="Italic">.</Emphasis>7<Emphasis Type="Italic">σ</Emphasis> higher than the Standard Model (SM) prediction. We decipher the data with two new physics scenarios: the underlying quark-level <InlineEquation ID="IEq3">
                           <EquationSource Format="MATHML">
                              <math xmlns:xlink="http://www.w3.org/1999/xlink" display="inline">
                                 <mi>b</mi>
                                 <mo>→</mo>
                                 <mi mathvariant="italic">sν</mi>
                                 <mover accent="true">
                                    <mi>ν</mi>
                                    <mo stretchy="true">¯</mo>
                                 </mover>
                              </math>
                           </EquationSource>
                           <EquationSource Format="TEX">$$ b\to s\nu \overline{\nu} $$</EquationSource>
                        </InlineEquation> transition is, besides the SM contribution, further affected by heavy new mediators that are much heavier than the electroweak scale, or amended by an additional decay channel with undetected light final states like dark matter or axion-like particles. These two scenarios can be most conveniently analyzed in the SM effective field theory (SMEFT) and the dark SMEFT (DSMEFT) framework, respectively. We consider the flavour structures of the resulting effective operators to be either generic or satisfy the minimal flavour violation (MFV) hypothesis, both for the quark and lepton sectors. In the first scenario, once the MFV assumption is made, only one SM-like low-energy effective operator induced by the SMEFT dimension-six operators can account for the Belle II excess, whose parameter space is, however, excluded by the Belle upper bound of the branching ratio <InlineEquation ID="IEq4">
                           <EquationSource Format="MATHML">
                              <math xmlns:xlink="http://www.w3.org/1999/xlink" display="inline">
                                 <mi mathvariant="script">B</mi>
                                 <mfenced close=")" open="(">
                                    <mrow>
                                       <msup>
                                          <mi>B</mi>
                                          <mn>0</mn>
                                       </msup>
                                       <mo>→</mo>
                                       <msup>
                                          <mi>K</mi>
                                          <mrow>
                                             <mo>∗</mo>
                                             <mn>0</mn>
                                          </mrow>
                                       </msup>
                                       <mi>ν</mi>
                                       <mover accent="true">
                                          <mi>ν</mi>
                                          <mo stretchy="true">¯</mo>
                                       </mover>
                                    </mrow>
                                 </mfenced>
                              </math>
                           </EquationSource>
                           <EquationSource Format="TEX">$$ \mathcal{B}\left({B}^0\to {K}^{\ast 0}\nu \overline{\nu}\right) $$</EquationSource>
                        </InlineEquation>. In the second scenario, it is found that the Belle II excess can be accommodated by 22 of the DSMEFT operators involving one or two scalar, fermionic, or vector dark matters as well as axion-like particles. These operators also receive dominant constraints from the <Emphasis Type="Italic">B</Emphasis>
                        <Superscript>0</Superscript> → <Emphasis Type="Italic">K</Emphasis>
                        <Superscript>*0</Superscript> + inv and <Emphasis Type="Italic">B</Emphasis>
                        <Subscript>
                           <Emphasis Type="Italic">s</Emphasis>
                        </Subscript> → inv decays. Once the MFV hypothesis is assumed, the number of viable operators is reduced to 14, and the <Emphasis Type="Italic">B</Emphasis>
                        <Superscript>+</Superscript> → <Emphasis Type="Italic">π</Emphasis>
                        <Superscript>+</Superscript> + inv and <Emphasis Type="Italic">K</Emphasis>
                        <Superscript>+</Superscript> → <Emphasis Type="Italic">π</Emphasis>
                        <Superscript>+</Superscript> + inv decays start to put further constraints on them. Within the parameter space allowed by all the current experimental data, the <Emphasis Type="Italic">q</Emphasis>
                        <Superscript>2</Superscript> distributions of the <Emphasis Type="Italic">B</Emphasis> → <Emphasis Type="Italic">K</Emphasis>
                        <Superscript>(*)</Superscript> + inv decays are then studied for each viable operator. We find that the resulting prediction of the operator <InlineEquation ID="IEq5">
                           <EquationSource Format="MATHML">
                              <math xmlns:xlink="http://www.w3.org/1999/xlink" display="inline">
                                 <msub>
                                    <mi mathvariant="script">Q</mi>
                                    <mi mathvariant="italic">qχ</mi>
                                 </msub>
                                 <mo>=</mo>
                                 <mfenced close=")" open="(">
                                    <mrow>
                                       <msub>
                                          <mover accent="true">
                                             <mi>q</mi>
                                             <mo stretchy="true">¯</mo>
                                          </mover>
                                          <mi>p</mi>
                                       </msub>
                                       <msub>
                                          <mi>γ</mi>
                                          <mi>μ</mi>
                                       </msub>
                                       <msub>
                                          <mi>q</mi>
                                          <mi>r</mi>
                                       </msub>
                                    </mrow>
                                 </mfenced>
                                 <mfenced close=")" open="(">
                                    <mrow>
                                       <mover accent="true">
                                          <mi>χ</mi>
                                          <mo stretchy="true">¯</mo>
                                       </mover>
                                       <msup>
                                          <mi>γ</mi>
                                          <mi>μ</mi>
                                       </msup>
                                       <mi>χ</mi>
                                    </mrow>
                                 </mfenced>
                              </math>
                           </EquationSource>
                           <EquationSource Format="TEX">$$ {\mathcal{Q}}_{q\chi}=\left({\overline{q}}_p{\gamma}_{\mu }{q}_r\right)\left(\overline{\chi}{\gamma}^{\mu}\chi \right) $$</EquationSource>
                        </InlineEquation> with a fermionic dark matter mass <Emphasis Type="Italic">m</Emphasis>
                        <Subscript>
                           <Emphasis Type="Italic">χ</Emphasis>
                        </Subscript> ≈ 700 MeV can closely match the Belle II event distribution in the bins 2 ≤ <Emphasis Type="Italic">q</Emphasis>
                        <Superscript>2</Superscript> ≤ 7 GeV<Superscript>2</Superscript>. In addition, we, for the first time, calculate systematically the longitudinal polarization fraction <Emphasis Type="Italic">F</Emphasis>
                        <Subscript>
                           <Emphasis Type="Italic">L</Emphasis>
                        </Subscript> of <Emphasis Type="Italic">K</Emphasis>
                        <Superscript>*</Superscript> in the <Emphasis Type="Italic">B</Emphasis> → <Emphasis Type="Italic">K</Emphasis>
                        <Superscript>*</Superscript> + inv decays within the DLEFT. By combining the decay spectra and <Emphasis Type="Italic">F</Emphasis>
                        <Subscript>
                           <Emphasis Type="Italic">L</Emphasis>
                        </Subscript>, almost all the DSMEFT operators are found to be distinguishable from each other. Finally, the future prospects at Belle II, CEPC and FCC-ee are also discussed for some of these FCNC processes.</Para>
                  </Abstract>
                  <KeywordGroup Language="En" OutputMedium="All" Source="Author">
                     <Heading>K<Emphasis Type="SmallCaps">eywords</Emphasis>
                     </Heading>
                     <Keyword>New Light Particles</Keyword>
                     <Keyword>Semi-Leptonic Decays</Keyword>
                     <Keyword>Flavour Symmetries</Keyword>
                     <Keyword>SMEFT</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>2402.19208</RefSource>
                           <RefTarget Address="https://doi.org/10.48550/arXiv.2402.19208" TargetType="URL"/>
                        </ExternalRef>
                     </SimplePara>
                  </ArticleNote>
               </ArticleHeader>
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