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dc.contributor.authorPHENIX Collaboration
dc.date.accessioned2016-06-13T04:28:08Z
dc.date.available2016-06-13T04:28:08Z
dc.date.issued2016
dc.identifier.citationPHENIX Collaboration. (2016). Measurement of higher cumulants of net-charge multiplicity distributions in Au+Au collisions at √sNN = 7.7-200 GeV. <i>Physical Review C</i>, <i>93</i>(1), Article 011901. <a href="https://doi.org/10.1103/PhysRevC.93.011901" target="_blank">https://doi.org/10.1103/PhysRevC.93.011901</a>
dc.identifier.otherCONVID_25530987
dc.identifier.otherTUTKAID_69088
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/50263
dc.description.abstractWe report the measurement of cumulants (Cn,n = 1,...,4) of the net-charge distributions measured within pseudorapidity (|η| < 0.35) in Au + Au collisions at √sNN = 7.7–200 GeV with the PHENIX experiment at the Relativistic Heavy Ion Collider. The ratios of cumulants (e.g., C1/C2, C3/C1) of the net-charge distributions, which can be related to volume independent susceptibility ratios, are studied as a function of centrality and energy. These quantities are important to understand the quantum-chromodynamics phase diagram and possible existence of a critical end point. The measured values are very well described by expectation from negative binomial distributions. We do not observe any nonmonotonic behavior in the ratios of the cumulants as a function of collision energy. The measured values of C1/C2 and C3/C1 can be directly compared to lattice quantum-chromodynamics calculations and thus allow extraction of both the chemical freeze-out temperature and the baryon chemical potential at each center-of-mass energy. The extracted baryon chemical potentials are in excellent agreement with a thermal-statistical analysis model.
dc.language.isoeng
dc.publisherAmerican Physical Society
dc.relation.ispartofseriesPhysical Review C
dc.subject.otherAu+Au collisions
dc.subject.othernet-charge distributions
dc.subject.otherbaryon chemical potentials
dc.titleMeasurement of higher cumulants of net-charge multiplicity distributions in Au+Au collisions at √sNN = 7.7-200 GeV
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-201606093005
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.date.updated2016-06-09T15:15:03Z
dc.type.coarhttp://purl.org/coar/resource_type/c_2df8fbb1
dc.description.reviewstatuspeerReviewed
dc.relation.issn2469-9985
dc.relation.numberinseries1
dc.relation.volume93
dc.type.versionpublishedVersion
dc.rights.copyright© 2016 American Physical Society. Published in this repository with the kind permission of the publisher.
dc.rights.accesslevelopenAccessfi
dc.relation.doi10.1103/PhysRevC.93.011901
dc.type.okmA1


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