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dc.contributor.authorALICE Collaboration
dc.date.accessioned2019-03-15T09:05:07Z
dc.date.available2019-03-15T09:05:07Z
dc.date.issued2019
dc.identifier.citationALICE Collaboration. (2019). Azimuthal Anisotropy of Heavy-Flavor Decay Electrons in p-Pb Collisions at √sNN = 5.02 TeV. <i>Physical Review Letters</i>, <i>122</i>(7), Article 072301. <a href="https://doi.org/10.1103/PhysRevLett.122.072301" target="_blank">https://doi.org/10.1103/PhysRevLett.122.072301</a>
dc.identifier.otherCONVID_28972550
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/63142
dc.description.abstractAngular correlations between heavy-flavor decay electrons and charged particles at midrapidity (|η|<0.8) are measured in p-Pb collisions at √sNN=5.02  TeV. The analysis is carried out for the 0%–20% (high) and 60%–100% (low) multiplicity ranges. The jet contribution in the correlation distribution from high-multiplicity events is removed by subtracting the distribution from low-multiplicity events. An azimuthal modulation remains after removing the jet contribution, similar to previous observations in two-particle angular correlation measurements for light-flavor hadrons. A Fourier decomposition of the modulation results in a positive second-order coefficient (v2) for heavy-flavor decay electrons in the transverse momentum interval 1.5<pT<4  GeV/c in high-multiplicity events, with a significance larger than 5σ. The results are compared with those of charged particles at midrapidity and those of inclusive muons at forward rapidity. The v2 measurement of open heavy-flavor particles at midrapidity in small collision systems could provide crucial information to help interpret the anisotropies observed in such systems.fi
dc.format.mimetypeapplication/pdf
dc.language.isoeng
dc.publisherAmerican Physical Society
dc.relation.ispartofseriesPhysical Review Letters
dc.rightsCC BY 4.0
dc.subject.otherproton-heavy ion collisions
dc.subject.otherheavy-flavor decay electrons
dc.titleAzimuthal Anisotropy of Heavy-Flavor Decay Electrons in p-Pb Collisions at √sNN = 5.02 TeV
dc.typeresearch article
dc.identifier.urnURN:NBN:fi:jyu-201903131852
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.date.updated2019-03-13T10:15:25Z
dc.type.coarhttp://purl.org/coar/resource_type/c_2df8fbb1
dc.description.reviewstatuspeerReviewed
dc.relation.issn0031-9007
dc.relation.numberinseries7
dc.relation.volume122
dc.type.versionpublishedVersion
dc.rights.copyright© 2019 CERN, for the ALICE Collaboration
dc.rights.accesslevelopenAccessfi
dc.type.publicationarticle
dc.subject.ysohiukkasfysiikka
dc.format.contentfulltext
jyx.subject.urihttp://www.yso.fi/onto/yso/p15576
dc.rights.urlhttps://creativecommons.org/licenses/by/4.0/
dc.relation.doi10.1103/PhysRevLett.122.072301
dc.type.okmA1


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