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.; Schwarz, D.; Templ, S.; Waltenberger, W.; Waltenberger, W.

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  <identifier identifierType="URL">https://aperta.ulakbim.gov.tr/record/231774</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>
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      <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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      <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>
    </creator>
    <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>Schwarz, D.</creatorName>
      <givenName>D.</givenName>
      <familyName>Schwarz</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 New Particles In Events With Energetic Jets And Large Missing Transverse Momentum In Proton-Proton Collisions At Root S=13 Tev</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/231774</alternateIdentifier>
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    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsIdenticalTo">10.1007/JHEP11(2021)153</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 is presented for new particles produced at the LHC in proton-proton collisions at root s = 13 TeV, using events with energetic jets and large missing transverse momentum. The analysis is based on a data sample corresponding to an integrated luminosity of 101 fb(-1), collected in 2017-2018 with the CMS detector. Machine learning techniques are used to define separate categories for events with narrow jets from initial-state radiation and events with large-radius jets consistent with a hadronic decay of a W or Z boson. A statistical combination is made with an earlier search based on a data sample of 36 fb(-1), collected in 2016. No significant excess of events is observed with respect to the standard model background expectation determined from control samples in data. The results are interpreted in terms of limits on the branching fraction of an invisible decay of the Higgs boson, as well as constraints on simplified models of dark matter, on first-generation scalar leptoquarks decaying to quarks and neutrinos, and on models with large extra dimensions. Several of the new limits, specifically for spin-1 dark matter mediators, pseudoscalar mediators, colored mediators, and leptoquarks, are the most restrictive to date.</description>
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