Приказ основних података о документу

dc.creatorĆirković, Predrag
dc.creatorMilošević, Jovan
dc.creatorNađđerđ, Laslo
dc.creatorWang, Fuqiang
dc.creatorZhu, Xiangrong
dc.date.accessioned2021-02-09T11:06:51Z
dc.date.available2021-02-09T11:06:51Z
dc.date.issued2020
dc.identifier.issn2469-9985
dc.identifier.urihttps://vinar.vin.bg.ac.rs/handle/123456789/8928
dc.description.abstractThe elliptic flow (v(2)) event-by-event fluctuations in PbPb collisions at 5.02 TeV are analyzed within the HYDJET + + model. Using the multiparticle, so-called Q-cumulant method, v(2){2}, v(2){4}, v(2){6}, and v(2){8} are calculated and used to study their ratios and to construct skewness (gamma(exp)(1)) as a measure of the asymmetry of the elliptic flow distribution. Additionally, in order to check if there is a hydrodynamics nature in the elliptic collectivity generated by the HYDJET + + model, the ratio of v(2){6} - v(2){8} and v(2){4} - v(2){6} distributions is calculated. The analysis is performed as a function of the collision centrality. In order to check the HYDJET + + model responses, the results of this analysis are compared to the corresponding experimental measurements from the ALICE, ATLAS, and CMS experiments. A rather good qualitative agreement is found.en
dc.language.isoen
dc.relationBilateral Cooperation between the Republic of Serbia and the People's Republic of China [451-03-478/2018-09/04 "Phenomenology in high energy physics"]
dc.relationinfo:eu-repo/grantAgreement/MESTD/Basic Research (BR or ON)/171019/RS//
dc.relationNational Natural Science Foundation of China (NSFC) [11847315]
dc.relationUnited States Department of Energy (DOE) [DE-SC0012910]
dc.rightsopenAccess
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/
dc.sourcePhysical Review C
dc.titleSkewness of the elliptic flow distribution in sNN =5.02 TeV PbPb collisions from the HYDJET++ modelen
dc.typearticleen
dc.rights.licenseBY
dcterms.abstractМилошевић, Јован; Зху, Xиангронг; Ћирковић, Предраг; Wанг, Фуqианг; Нађђерђ, Ласло;
dc.rights.holder© 2020 by the authors
dc.citation.volume101
dc.citation.issue3
dc.citation.spage034907
dc.identifier.wos000519701700003
dc.identifier.doi10.1103/PhysRevC.101.034907
dc.citation.rankM21
dc.type.versionpublishedVersion
dc.identifier.scopus2-s2.0-85082736685
dc.identifier.fulltexthttps://vinar.vin.bg.ac.rs/bitstream/id/22421/PhysRevC.101.034907.pdf


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Приказ основних података о документу