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Chatrchyan, S.; Khachatryan, V.; Sirunyan, A. M.; Tumasyan, A.; Adam, W.; Bergauer, T.; Dragicevic, M.; Eroe, J.; Fabjan, C.; Friedl, M.; Fruehwirth, R.; Ghete, V. M.; Hammer, J.; Hoch, M.; Hoermann, N.; Hrubec, J.; Jeitler, M.; Kiesenhofer, W.; Krammer, M.; Liko, D.; Liko, D.
<?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/227439</identifier> <creators> <creator> <creatorName>Chatrchyan, S.</creatorName> <givenName>S.</givenName> <familyName>Chatrchyan</familyName> <affiliation>Yerevan Phys Inst, Yerevan 375036, Armenia</affiliation> </creator> <creator> <creatorName>Khachatryan, V.</creatorName> <givenName>V.</givenName> <familyName>Khachatryan</familyName> <affiliation>Yerevan Phys Inst, Yerevan 375036, Armenia</affiliation> </creator> <creator> <creatorName>Sirunyan, A. M.</creatorName> <givenName>A. M.</givenName> <familyName>Sirunyan</familyName> <affiliation>Yerevan Phys Inst, Yerevan 375036, Armenia</affiliation> </creator> <creator> <creatorName>Tumasyan, A.</creatorName> <givenName>A.</givenName> <familyName>Tumasyan</familyName> <affiliation>Yerevan Phys Inst, Yerevan 375036, Armenia</affiliation> </creator> <creator> <creatorName>Adam, W.</creatorName> <givenName>W.</givenName> <familyName>Adam</familyName> <affiliation>Inst Hochenergiephys OeAW, Vienna, Austria</affiliation> </creator> <creator> <creatorName>Bergauer, T.</creatorName> <givenName>T.</givenName> <familyName>Bergauer</familyName> <affiliation>Inst Hochenergiephys OeAW, Vienna, Austria</affiliation> </creator> <creator> <creatorName>Dragicevic, M.</creatorName> <givenName>M.</givenName> <familyName>Dragicevic</familyName> <affiliation>Inst Hochenergiephys OeAW, Vienna, Austria</affiliation> </creator> <creator> <creatorName>Eroe, J.</creatorName> <givenName>J.</givenName> <familyName>Eroe</familyName> <affiliation>Inst Hochenergiephys OeAW, Vienna, Austria</affiliation> </creator> <creator> <creatorName>Fabjan, C.</creatorName> <givenName>C.</givenName> <familyName>Fabjan</familyName> <affiliation>Inst Hochenergiephys OeAW, Vienna, Austria</affiliation> </creator> <creator> <creatorName>Friedl, M.</creatorName> <givenName>M.</givenName> <familyName>Friedl</familyName> <affiliation>Inst Hochenergiephys OeAW, Vienna, Austria</affiliation> </creator> <creator> <creatorName>Fruehwirth, R.</creatorName> <givenName>R.</givenName> <familyName>Fruehwirth</familyName> <affiliation>Inst Hochenergiephys OeAW, Vienna, Austria</affiliation> </creator> <creator> <creatorName>Ghete, V. M.</creatorName> <givenName>V. M.</givenName> <familyName>Ghete</familyName> <affiliation>Inst Hochenergiephys OeAW, Vienna, Austria</affiliation> </creator> <creator> <creatorName>Hammer, J.</creatorName> <givenName>J.</givenName> <familyName>Hammer</familyName> </creator> <creator> <creatorName>Hoch, M.</creatorName> <givenName>M.</givenName> <familyName>Hoch</familyName> <affiliation>Inst Hochenergiephys OeAW, Vienna, Austria</affiliation> </creator> <creator> <creatorName>Hoermann, N.</creatorName> <givenName>N.</givenName> <familyName>Hoermann</familyName> <affiliation>Inst Hochenergiephys OeAW, Vienna, Austria</affiliation> </creator> <creator> <creatorName>Hrubec, J.</creatorName> <givenName>J.</givenName> <familyName>Hrubec</familyName> <affiliation>Inst Hochenergiephys OeAW, Vienna, Austria</affiliation> </creator> <creator> <creatorName>Jeitler, M.</creatorName> <givenName>M.</givenName> <familyName>Jeitler</familyName> <affiliation>Inst Hochenergiephys OeAW, Vienna, Austria</affiliation> </creator> <creator> <creatorName>Kiesenhofer, W.</creatorName> <givenName>W.</givenName> <familyName>Kiesenhofer</familyName> <affiliation>Inst Hochenergiephys OeAW, Vienna, Austria</affiliation> </creator> <creator> <creatorName>Krammer, M.</creatorName> <givenName>M.</givenName> <familyName>Krammer</familyName> <affiliation>Inst Hochenergiephys OeAW, Vienna, Austria</affiliation> </creator> <creator> <creatorName>Liko, D.</creatorName> <givenName>D.</givenName> <familyName>Liko</familyName> <affiliation>Inst Hochenergiephys OeAW, Vienna, Austria</affiliation> </creator> <creator> <creatorName>Liko, D.</creatorName> <givenName>D.</givenName> <familyName>Liko</familyName> <affiliation>Inst Hochenergiephys OeAW, Vienna, Austria</affiliation> </creator> </creators> <titles> <title>Inclusive B-Jet Production In Pp Collisions At Root S=7 Tev</title> </titles> <publisher>Aperta</publisher> <publicationYear>2012</publicationYear> <dates> <date dateType="Issued">2012-01-01</date> </dates> <resourceType resourceTypeGeneral="Text">Journal article</resourceType> <alternateIdentifiers> <alternateIdentifier alternateIdentifierType="url">https://aperta.ulakbim.gov.tr/record/227439</alternateIdentifier> </alternateIdentifiers> <relatedIdentifiers> <relatedIdentifier relatedIdentifierType="DOI" relationType="IsIdenticalTo">10.1007/JHEP04(2012)084</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"><p>The inclusive b-jet production cross section in pp collisions at a center-of-mass energy of 7TeV is measured using data collected by the CMS experiment at the LHC. The cross section is presented as a function of the jet transverse momentum in the range 18 &lt; p(T) &lt; 200 GeV for several rapidity intervals. The results are also given as the ratio of the b-jet production cross section to the inclusive jet production cross section. The measurement is performed with two different analyses, which differ in their trigger selection and b-jet identification: a jet analysis that selects events with a b jet using a sample corresponding to an integrated luminosity of 34 pb(-1), and a muon analysis requiring a b jet with a muon based on an integrated luminosity of 3 pb(-1). In both approaches the b jets are identified by requiring a secondary vertex. The results from the two methods are in agreement with each other and with next-to-leading order calculations, as well as with predictions based on the PYTHIA event generator.</p></description> </descriptions> </resource>
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