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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.accessioned2024-07-01T03:59:14Z-
dc.date.available2024-07-01T03:59:14Z-
dc.date.issued2024-02en_US
dc.identifier.citationJournal of High Energy Physics, 2024(02), 106.  en_US
dc.identifier.issn1029-8479en_US
dc.identifier.urihttps://doi.org/10.1007/JHEP02(2024)106en_US
dc.identifier.urihttp://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/9002-
dc.description.abstractThe hydrodynamic flow-like behavior of charged hadrons in high-energy lead-lead collisions is studied through multiparticle correlations. The elliptic anisotropy values based on different orders of multiparticle cumulants, v2{2k}, are measured up to the tenth order (k = 5) as functions of the collision centrality at a nucleon-nucleon center-of-mass energy of 𝑠NN = 5.02 TeV. The data were recorded by the CMS experiment at the LHC and correspond to an integrated luminosity of 0.607 nb−1. A hierarchy is observed between the coefficients, with v2{2} > v2{4} ≳ v2{6} ≳ v2{8} ≳ v2{10}. Based on these results, centrality-dependent moments for the fluctuation-driven event-by-event v2 distribution are determined, including the skewness, kurtosis and, for the first time, superskewness. Assuming a hydrodynamic expansion of the produced medium, these moments directly probe the initial-state geometry in high-energy nucleus-nucleus collisions.en_US
dc.language.isoenen_US
dc.publisherSpringer Natureen_US
dc.subjectEvent-by-Event fluctuationen_US
dc.subjectHarmonic Flowen_US
dc.subjectHeavy Ion Experimentsen_US
dc.subjectRelativistic Heavy Ion Physicsen_US
dc.subject2024en_US
dc.subject2024-JUN-WEEK3en_US
dc.subjectTOC-JUN-2024en_US
dc.titleHigher-order moments of the elliptic flow distribution in PbPb collisions at  √sNN = 5.02 TeVen_US
dc.typeArticleen_US
dc.contributor.departmentDept. of Physicsen_US
dc.identifier.sourcetitleJournal of High Energy Physicsen_US
dc.publication.originofpublisherForeignen_US
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