1 Ocak 2018 Dergi makalesi Açık Erişim

Sirunyan, A. M.; Tumasyan, A.; Adam, W.; Ambrogi, F.; Asilar, E.; Bergauer, T.; Brandstetter, J.; Dragicevic, M.; Eroe, J.; Escalante Del Valle, A.; Flechl, M.; Fruehwirth, R.; Ghete, V. M.; Hrubec, J.; Jeitler, M.; Krammer, N.; Kraetschmer, I.; Liko, D.; Madlener, T.; Mikulec, I.; Mikulec, I.

DataCite XML

<?xml version='1.0' encoding='utf-8'?>
<resource xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns="http://datacite.org/schema/kernel-4" xsi:schemaLocation="http://datacite.org/schema/kernel-4 http://schema.datacite.org/meta/kernel-4.1/metadata.xsd">
  <identifier identifierType="URL">https://aperta.ulakbim.gov.tr/record/35005</identifier>
  <creators>
    <creator>
      <creatorName>Sirunyan, A. M.</creatorName>
      <givenName>A. M.</givenName>
      <familyName>Sirunyan</familyName>
      <affiliation>Yerevan Phys Inst, Yerevan, Armenia</affiliation>
    </creator>
    <creator>
      <creatorName>Tumasyan, A.</creatorName>
      <givenName>A.</givenName>
      <familyName>Tumasyan</familyName>
      <affiliation>Yerevan Phys Inst, Yerevan, Armenia</affiliation>
    </creator>
    <creator>
      <creatorName>Adam, W.</creatorName>
      <givenName>W.</givenName>
      <familyName>Adam</familyName>
      <affiliation>Inst Hochenergiephys, Vienna, Austria</affiliation>
    </creator>
    <creator>
      <creatorName>Ambrogi, F.</creatorName>
      <givenName>F.</givenName>
      <familyName>Ambrogi</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>
    </creator>
    <creator>
      <creatorName>Bergauer, T.</creatorName>
      <givenName>T.</givenName>
      <familyName>Bergauer</familyName>
      <affiliation>Inst Hochenergiephys, Vienna, Austria</affiliation>
    </creator>
    <creator>
      <creatorName>Brandstetter, J.</creatorName>
      <givenName>J.</givenName>
      <familyName>Brandstetter</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>Eroe, J.</creatorName>
      <givenName>J.</givenName>
      <familyName>Eroe</familyName>
      <affiliation>Inst Hochenergiephys, Vienna, Austria</affiliation>
    </creator>
    <creator>
      <creatorName>Escalante Del Valle, A.</creatorName>
      <givenName>A.</givenName>
      <familyName>Escalante Del Valle</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>Fruehwirth, R.</creatorName>
      <givenName>R.</givenName>
      <familyName>Fruehwirth</familyName>
      <affiliation>Inst Hochenergiephys, Vienna, Austria</affiliation>
    </creator>
    <creator>
      <creatorName>Ghete, V. M.</creatorName>
      <givenName>V. M.</givenName>
      <familyName>Ghete</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>
    </creator>
    <creator>
      <creatorName>Jeitler, M.</creatorName>
      <givenName>M.</givenName>
      <familyName>Jeitler</familyName>
      <affiliation>Inst Hochenergiephys, Vienna, Austria</affiliation>
    </creator>
    <creator>
      <creatorName>Krammer, N.</creatorName>
      <givenName>N.</givenName>
      <familyName>Krammer</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>Madlener, T.</creatorName>
      <givenName>T.</givenName>
      <familyName>Madlener</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>Mikulec, I.</creatorName>
      <givenName>I.</givenName>
      <familyName>Mikulec</familyName>
      <affiliation>Inst Hochenergiephys, Vienna, Austria</affiliation>
    </creator>
  </creators>
  <titles>
    <title>Search For Black Holes And Sphalerons In High-Multiplicity Final States In Proton-Proton Collisions A Root S=13 Tevt</title>
  </titles>
  <publisher>Aperta</publisher>
  <publicationYear>2018</publicationYear>
  <dates>
    <date dateType="Issued">2018-01-01</date>
  </dates>
  <resourceType resourceTypeGeneral="Text">Journal article</resourceType>
  <alternateIdentifiers>
    <alternateIdentifier alternateIdentifierType="url">https://aperta.ulakbim.gov.tr/record/35005</alternateIdentifier>
  </alternateIdentifiers>
  <relatedIdentifiers>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsIdenticalTo">10.1007/JHEP11(2018)042</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 in energetic, high-multiplicity final states for evidence of physics beyond the standard model, such as black holes, string balls, and electroweak sphalerons, is presented. The data sample corresponds to an integrated luminosity of 35.9 fb(-1) collected with the CMS experiment at the LHC in proton-proton collisions at a center-of-mass energy of 13 TeV in 2016. Standard model backgrounds, dominated by multijet production, are determined from control regions in data without any reliance on simulation. No evidence for excesses above the predicted background is observed. Model-independent 95% confidence level upper limits on the cross section of beyond the standard model signals in these final states are set and further interpreted in terms of limits on semiclassical black hole, string ball, and sphaleron production. In the context of models with large extra dimensions, semiclassical black holes with minimum masses as high as 10.1 TeV and string balls with masses as high as 9.5 TeV are excluded by this search. Results of the first dedicated search for electroweak sphalerons are presented. An upper limit of 0.021 is set at 95% confidence level on the fraction of all quark-quark interactions above the nominal threshold energy of 9 TeV resulting in the sphaleron transition.</description>
  </descriptions>
</resource>