{"title":"Evolution of elliptic flow of produced particles from Au+Au collisions at sNN=4.5−200 Gev in a hybrid model","authors":"A. Demanov, P. Parfenov, A. Taranenko","doi":"10.1063/5.0067505","DOIUrl":null,"url":null,"abstract":"Azimuthal anisotropy of produced particles is one of the important observables sensitive to the transport properties of the strongly interacting matter created in relativistic heavy-ion collisions. In this work, we report on the calculations of elliptic flow (v2) of identified charged hadrons produced in Au+Au collisions at sNN=4.5−200 Gev from a viscous hydro+cascade hybrid model vHLLE+UrQMD and provide the direct comparison with published results from STAR and PHENIX experiments. The results would be useful as predictions for the upcoming beam energy scan experiments at NICA Collider.","PeriodicalId":296008,"journal":{"name":"PROCEEDINGS OF THE 24TH INTERNATIONAL SCIENTIFIC CONFERENCE OF YOUNG SCIENTISTS AND SPECIALISTS (AYSS-2020)","volume":" 34","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2021-09-24","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"3","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"PROCEEDINGS OF THE 24TH INTERNATIONAL SCIENTIFIC CONFERENCE OF YOUNG SCIENTISTS AND SPECIALISTS (AYSS-2020)","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1063/5.0067505","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 3
Abstract
Azimuthal anisotropy of produced particles is one of the important observables sensitive to the transport properties of the strongly interacting matter created in relativistic heavy-ion collisions. In this work, we report on the calculations of elliptic flow (v2) of identified charged hadrons produced in Au+Au collisions at sNN=4.5−200 Gev from a viscous hydro+cascade hybrid model vHLLE+UrQMD and provide the direct comparison with published results from STAR and PHENIX experiments. The results would be useful as predictions for the upcoming beam energy scan experiments at NICA Collider.
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