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dc.contributor.authorCMS Collaborationen_US
dc.contributor.authorTumasyan, A.en_US
dc.contributor.authorALPANA, A.en_US
dc.contributor.authorDUBE, SOURABHen_US
dc.contributor.authorKANSAL, B.en_US
dc.contributor.authorLAHA, A.en_US
dc.contributor.authorPANDEY, S.en_US
dc.contributor.authorRASTOGI, A.en_US
dc.contributor.authorSHARMA, SEEMA et al.en_US
dc.date.accessioned2024-06-21T05:41:29Z
dc.date.available2024-06-21T05:41:29Z
dc.date.issued2024-03en_US
dc.identifier.citationPhysics Letters B, 850, 138518.en_US
dc.identifier.issn1873-2445en_US
dc.identifier.issn0370-2693en_US
dc.identifier.urihttps://doi.org/10.1016/j.physletb.2024.138518en_US
dc.identifier.urihttp://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/8989
dc.description.abstractThe azimuthal anisotropy of Image 1 mesons in high-multiplicity proton-lead collisions is studied using data collected by the CMS experiment at a nucleon-nucleon center-of-mass energy of . The Image 1 mesons are reconstructed using their dimuon decay channel. The anisotropy is characterized by the second Fourier harmonic coefficients, found using a two-particle correlation technique, in which the Image 1 mesons are correlated with charged hadrons. A large pseudorapidity gap is used to suppress short-range correlations. Nonflow contamination from the dijet background is removed using a low-multiplicity subtraction method, and the results are presented as a function of Image 1 transverse momentum. The azimuthal anisotropies are smaller than those found for charmonia in proton-lead collisions at the same collision energy, but are consistent with values found for Image 1 mesons in lead-lead interactions at a nucleon-nucleon center-of-mass energy of 5.02 TeV.en_US
dc.language.isoenen_US
dc.publisherElsevier B.V.en_US
dc.subjectCMSen_US
dc.subjectpPben_US
dc.subjectHeavy ionen_US
dc.subjectv2en_US
dc.subjectUpsilonen_US
dc.subjectFlowen_US
dc.subject2024en_US
dc.subject2024-JUN-WEEK1en_US
dc.subjectTOC-JUN-2024en_US
dc.titleStudy of azimuthal anisotropy of γ(1S) mesons in pPb collisions at √SNN=8.16 TeVen_US
dc.typeArticleen_US
dc.contributor.departmentDept. of Physicsen_US
dc.identifier.sourcetitlePhysics Letters Ben_US
dc.publication.originofpublisherForeignen_US
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