1 Ocak 2021 Dergi makalesi Açık Erişim

Tumasyan, A.; Adam, W.; Andrejkovic, J. W.; Bergauer, T.; Chatterjee, S.; Dragicevic, M.; Del Valle, A. Escalante; Fruhwirth, R.; Jeitler, M.; Krammer, N.; Lechner, L.; Liko, D.; Mikulec, I; Paulitsch, P.; Pitters, F. M.; Schieck, J.; Schofbeck, R.; Spanring, M.; Templ, S.; Waltenberger, W.; Waltenberger, W.

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  <identifier identifierType="URL">https://aperta.ulakbim.gov.tr/record/232768</identifier>
  <creators>
    <creator>
      <creatorName>Tumasyan, A.</creatorName>
      <givenName>A.</givenName>
      <familyName>Tumasyan</familyName>
      <affiliation>Yerevan Phys Inst, Yerevan, Armenia</affiliation>
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    <creator>
      <creatorName>Adam, W.</creatorName>
      <givenName>W.</givenName>
      <familyName>Adam</familyName>
      <affiliation>Inst Hochenergiephys, Vienna, Austria</affiliation>
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    <creator>
      <creatorName>Andrejkovic, J. W.</creatorName>
      <givenName>J. W.</givenName>
      <familyName>Andrejkovic</familyName>
      <affiliation>Inst Hochenergiephys, Vienna, Austria</affiliation>
    </creator>
    <creator>
      <creatorName>Bergauer, T.</creatorName>
      <givenName>T.</givenName>
      <familyName>Bergauer</familyName>
      <affiliation>Inst Hochenergiephys, Vienna, Austria</affiliation>
    </creator>
    <creator>
      <creatorName>Chatterjee, S.</creatorName>
      <givenName>S.</givenName>
      <familyName>Chatterjee</familyName>
      <affiliation>Inst Hochenergiephys, Vienna, Austria</affiliation>
    </creator>
    <creator>
      <creatorName>Dragicevic, M.</creatorName>
      <givenName>M.</givenName>
      <familyName>Dragicevic</familyName>
      <affiliation>Inst Hochenergiephys, Vienna, Austria</affiliation>
    </creator>
    <creator>
      <creatorName>Del Valle, A. Escalante</creatorName>
      <givenName>A. Escalante</givenName>
      <familyName>Del Valle</familyName>
      <affiliation>Inst Hochenergiephys, Vienna, Austria</affiliation>
    </creator>
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      <creatorName>Fruhwirth, R.</creatorName>
      <givenName>R.</givenName>
      <familyName>Fruhwirth</familyName>
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    <creator>
      <creatorName>Jeitler, M.</creatorName>
      <givenName>M.</givenName>
      <familyName>Jeitler</familyName>
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    <creator>
      <creatorName>Krammer, N.</creatorName>
      <givenName>N.</givenName>
      <familyName>Krammer</familyName>
      <affiliation>Inst Hochenergiephys, Vienna, Austria</affiliation>
    </creator>
    <creator>
      <creatorName>Lechner, L.</creatorName>
      <givenName>L.</givenName>
      <familyName>Lechner</familyName>
      <affiliation>Inst Hochenergiephys, Vienna, Austria</affiliation>
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    <creator>
      <creatorName>Liko, D.</creatorName>
      <givenName>D.</givenName>
      <familyName>Liko</familyName>
      <affiliation>Inst Hochenergiephys, Vienna, Austria</affiliation>
    </creator>
    <creator>
      <creatorName>Mikulec, I</creatorName>
      <givenName>I</givenName>
      <familyName>Mikulec</familyName>
      <affiliation>Inst Hochenergiephys, Vienna, Austria</affiliation>
    </creator>
    <creator>
      <creatorName>Paulitsch, P.</creatorName>
      <givenName>P.</givenName>
      <familyName>Paulitsch</familyName>
      <affiliation>Inst Hochenergiephys, Vienna, Austria</affiliation>
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    <creator>
      <creatorName>Pitters, F. M.</creatorName>
      <givenName>F. M.</givenName>
      <familyName>Pitters</familyName>
      <affiliation>Inst Hochenergiephys, Vienna, Austria</affiliation>
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      <creatorName>Schieck, J.</creatorName>
      <givenName>J.</givenName>
      <familyName>Schieck</familyName>
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      <creatorName>Schofbeck, R.</creatorName>
      <givenName>R.</givenName>
      <familyName>Schofbeck</familyName>
      <affiliation>Inst Hochenergiephys, Vienna, Austria</affiliation>
    </creator>
    <creator>
      <creatorName>Spanring, M.</creatorName>
      <givenName>M.</givenName>
      <familyName>Spanring</familyName>
      <affiliation>Inst Hochenergiephys, Vienna, Austria</affiliation>
    </creator>
    <creator>
      <creatorName>Templ, S.</creatorName>
      <givenName>S.</givenName>
      <familyName>Templ</familyName>
      <affiliation>Inst Hochenergiephys, Vienna, Austria</affiliation>
    </creator>
    <creator>
      <creatorName>Waltenberger, W.</creatorName>
      <givenName>W.</givenName>
      <familyName>Waltenberger</familyName>
      <affiliation>Inst Hochenergiephys, Vienna, Austria</affiliation>
    </creator>
    <creator>
      <creatorName>Waltenberger, W.</creatorName>
      <givenName>W.</givenName>
      <familyName>Waltenberger</familyName>
      <affiliation>Inst Hochenergiephys, Vienna, Austria</affiliation>
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  </creators>
  <titles>
    <title>Search For A Heavy Higgs Boson Decaying Into Two Lighter Higgs Bosons In The Tau Tau Bb Final State At 13Tev</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/232768</alternateIdentifier>
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  <relatedIdentifiers>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsIdenticalTo">10.1007/JHEP11(2021)057</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">A search for a heavy Higgs boson H decaying into the observed Higgs boson h with a mass of 125 GeV and another Higgs boson h(S) is presented. The h and h(S) bosons are required to decay into a pair of tau leptons and a pair of b quarks, respectively. The search uses a sample of proton-proton collisions collected with the CMS detector at a center-of-mass energy of 13TeV, corresponding to an integrated luminosity of 137 fb(-1). Mass ranges of 240-3000 GeV for m(H) and 60-2800 GeV for m(hS) are explored in the search. No signal has been observed. Model independent 95% confidence level upper limits on the product of the production cross section and the branching fractions of the signal process are set with a sensitivity ranging from 125 fb (for m(H) = 240 GeV) to 2.7 fb (for m(H) = 1000 GeV). These limits are compared to maximally allowed products of the production cross section and the branching fractions of the signal process in the next-to-minimal supersymmetric extension of the standard model.</description>
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