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Semileptonic Xi(c) baryon decays in the light cone QCD sum rules

Aliev, T. M.; Bilmis, S.; Savci, M.


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  <identifier identifierType="URL">https://aperta.ulakbim.gov.tr/record/239968</identifier>
  <creators>
    <creator>
      <creatorName>Aliev, T. M.</creatorName>
      <givenName>T. M.</givenName>
      <familyName>Aliev</familyName>
      <affiliation>Middle East Tech Univ, Dept Phys, TR-06800 Ankara, Turkey</affiliation>
    </creator>
    <creator>
      <creatorName>Bilmis, S.</creatorName>
      <givenName>S.</givenName>
      <familyName>Bilmis</familyName>
    </creator>
    <creator>
      <creatorName>Savci, M.</creatorName>
      <givenName>M.</givenName>
      <familyName>Savci</familyName>
      <affiliation>Middle East Tech Univ, Dept Phys, TR-06800 Ankara, Turkey</affiliation>
    </creator>
  </creators>
  <titles>
    <title>Semileptonic Xi(C) Baryon Decays In The Light Cone Qcd Sum Rules</title>
  </titles>
  <publisher>Aperta</publisher>
  <publicationYear>2021</publicationYear>
  <dates>
    <date dateType="Issued">2021-01-01</date>
  </dates>
  <resourceType resourceTypeGeneral="Text">Journal article</resourceType>
  <alternateIdentifiers>
    <alternateIdentifier alternateIdentifierType="url">https://aperta.ulakbim.gov.tr/record/239968</alternateIdentifier>
  </alternateIdentifiers>
  <relatedIdentifiers>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsIdenticalTo">10.1103/PhysRevD.104.054030</relatedIdentifier>
  </relatedIdentifiers>
  <rightsList>
    <rights rightsURI="http://www.opendefinition.org/licenses/cc-by">Creative Commons Attribution</rights>
    <rights rightsURI="info:eu-repo/semantics/openAccess">Open Access</rights>
  </rightsList>
  <descriptions>
    <description descriptionType="Abstract">Form factors of the weak Xi(c) -&amp;gt; Xi( )(A) transitions are calculated within the light cone QCD sum rules. The pollution coming from the contribution of the negative parity Xi(c)* baryon is eliminated by considering the combinations of sum rules corresponding to the different Lorentz structures. Having obtained the form factors, the branching ratios of the Xi(c -&amp;gt; )Xi(c )(Lambda)lv decays are also calculated, and our predictions are compared with the results of other approaches as well as the measurements done by the BELLE and ALICE collaborations.</description>
  </descriptions>
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