1 Ocak 2017 Dergi makalesi Açık Erişim

Sirunyan, A. M.; Tumasyan, A.; Adam, W.; Asilar, E.; Bergauer, T.; Brandstetter, J.; Brondolin, E.; Dragicevic, M.; Eroe, J.; Flechl, M.; Friedl, M.; Fruehwirth, R.; Ghete, V. M.; Hartl, C.; Hoermann, N.; Hrubec, J.; Jeitler, M.; Koenig, A.; Kraetschmer, I.; Liko, D.; Liko, D.

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  <identifier identifierType="URL">https://aperta.ulakbim.gov.tr/record/47637</identifier>
  <creators>
    <creator>
      <creatorName>Sirunyan, A. M.</creatorName>
      <givenName>A. M.</givenName>
      <familyName>Sirunyan</familyName>
      <affiliation>Yerevan Phys Inst, Yerevan, Armenia</affiliation>
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    <creator>
      <creatorName>Tumasyan, A.</creatorName>
      <givenName>A.</givenName>
      <familyName>Tumasyan</familyName>
      <affiliation>Yerevan Phys Inst, Yerevan, Armenia</affiliation>
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      <creatorName>Adam, W.</creatorName>
      <givenName>W.</givenName>
      <familyName>Adam</familyName>
      <affiliation>Inst Hochenergiephys, Vienna, Austria</affiliation>
    </creator>
    <creator>
      <creatorName>Asilar, E.</creatorName>
      <givenName>E.</givenName>
      <familyName>Asilar</familyName>
      <affiliation>Inst Hochenergiephys, Vienna, Austria</affiliation>
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    <creator>
      <creatorName>Bergauer, T.</creatorName>
      <givenName>T.</givenName>
      <familyName>Bergauer</familyName>
      <affiliation>Inst Hochenergiephys, Vienna, Austria</affiliation>
    </creator>
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      <creatorName>Brandstetter, J.</creatorName>
      <givenName>J.</givenName>
      <familyName>Brandstetter</familyName>
      <affiliation>Inst Hochenergiephys, Vienna, Austria</affiliation>
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      <creatorName>Brondolin, E.</creatorName>
      <givenName>E.</givenName>
      <familyName>Brondolin</familyName>
      <affiliation>Inst Hochenergiephys, Vienna, Austria</affiliation>
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    <creator>
      <creatorName>Dragicevic, M.</creatorName>
      <givenName>M.</givenName>
      <familyName>Dragicevic</familyName>
      <affiliation>Inst Hochenergiephys, Vienna, Austria</affiliation>
    </creator>
    <creator>
      <creatorName>Eroe, J.</creatorName>
      <givenName>J.</givenName>
      <familyName>Eroe</familyName>
      <affiliation>Inst Hochenergiephys, Vienna, Austria</affiliation>
    </creator>
    <creator>
      <creatorName>Flechl, M.</creatorName>
      <givenName>M.</givenName>
      <familyName>Flechl</familyName>
      <affiliation>Inst Hochenergiephys, Vienna, Austria</affiliation>
    </creator>
    <creator>
      <creatorName>Friedl, M.</creatorName>
      <givenName>M.</givenName>
      <familyName>Friedl</familyName>
      <affiliation>Inst Hochenergiephys, Vienna, Austria</affiliation>
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      <creatorName>Fruehwirth, R.</creatorName>
      <givenName>R.</givenName>
      <familyName>Fruehwirth</familyName>
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      <creatorName>Ghete, V. M.</creatorName>
      <givenName>V. M.</givenName>
      <familyName>Ghete</familyName>
      <affiliation>Inst Hochenergiephys, Vienna, Austria</affiliation>
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      <creatorName>Hartl, C.</creatorName>
      <givenName>C.</givenName>
      <familyName>Hartl</familyName>
      <affiliation>Inst Hochenergiephys, Vienna, Austria</affiliation>
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    <creator>
      <creatorName>Hoermann, N.</creatorName>
      <givenName>N.</givenName>
      <familyName>Hoermann</familyName>
      <affiliation>Inst Hochenergiephys, Vienna, Austria</affiliation>
    </creator>
    <creator>
      <creatorName>Hrubec, J.</creatorName>
      <givenName>J.</givenName>
      <familyName>Hrubec</familyName>
      <affiliation>Inst Hochenergiephys, Vienna, Austria</affiliation>
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    <creator>
      <creatorName>Jeitler, M.</creatorName>
      <givenName>M.</givenName>
      <familyName>Jeitler</familyName>
    </creator>
    <creator>
      <creatorName>Koenig, A.</creatorName>
      <givenName>A.</givenName>
      <familyName>Koenig</familyName>
      <affiliation>Inst Hochenergiephys, Vienna, Austria</affiliation>
    </creator>
    <creator>
      <creatorName>Kraetschmer, I.</creatorName>
      <givenName>I.</givenName>
      <familyName>Kraetschmer</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>Liko, D.</creatorName>
      <givenName>D.</givenName>
      <familyName>Liko</familyName>
      <affiliation>Inst Hochenergiephys, Vienna, Austria</affiliation>
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  <titles>
    <title>Measurements Of The Charm Jet Cross Section And Nuclear Modification Factor In Ppb Collisions At Root Snn=5.02Tev</title>
  </titles>
  <publisher>Aperta</publisher>
  <publicationYear>2017</publicationYear>
  <dates>
    <date dateType="Issued">2017-01-01</date>
  </dates>
  <resourceType resourceTypeGeneral="Text">Journal article</resourceType>
  <alternateIdentifiers>
    <alternateIdentifier alternateIdentifierType="url">https://aperta.ulakbim.gov.tr/record/47637</alternateIdentifier>
  </alternateIdentifiers>
  <relatedIdentifiers>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsIdenticalTo">10.1016/j.physletb.2017.06.053</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">The CMS Collaboration presents the first measurement of the differential cross section of jets from charm quarks produced in proton-lead (pPb) collisions at a nucleon-nucleon center-of-mass energy of root sNN= 5.02 TeV, as well as results from charm quark jets in proton-proton (pp) collisions at root s=2.76and 5.02TeV. By comparing the yields of the pPb and pp collision systems at the same energy, a nuclear modification factor for charm jets from 55 to 400GeV/cin pPb collisions at root sNN=5.02 TeV of R-pA= 0.92 +/- 0.07 (stat) +/- 0.11(syst) is obtained. This is consistent with an absence of final-state energy loss for charm quarks in pPb collisions. In addition, the fraction of jets coming from charm quarks is found to be consistent with that predicted by PYTHIA 6 for pp collisions at root s=2.76 and 5.02TeV, and is independent of the jet transverse momentum from 55 to 400 GeV/c. (C) 2017 The Author(s). Published by Elsevier B.V.</description>
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