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Third harmonic flow of charged particles in Au + Au collisions at √s<inf>NN</inf>=200 GeV

dc.creatorAdamczyk, L
dc.creatorAdkins, JK
dc.creatorAgakishiev, G
dc.creatorAggarwal, MM
dc.creatorAhammed, Z
dc.creatorAlakhverdyants, AV
dc.creatorAlekseev, I
dc.creatorAlford, J
dc.creatorAnson, CD
dc.creatorArkhipkin, D
dc.creatorAschenauer, E
dc.creatorAverichev, GS
dc.creatorBalewski, J
dc.creatorBanerjee, A
dc.creatorBarnovska, Z
dc.creatorBeavis, DR
dc.creatorBellwied, R
dc.creatorBetancourt, MJ
dc.creatorBetts, RR
dc.creatorBhasin, A
dc.creatorBhati, AK
dc.creatorBichsel, H
dc.creatorBielcik, J
dc.creatorBielcikova, J
dc.creatorBland, LC
dc.creatorBordyuzhin, IG
dc.creatorBorowski, W
dc.creatorBouchet, J
dc.creatorBrandin, AV
dc.creatorBrovko, SG
dc.creatorBruna, E
dc.creatorBültmann, S
dc.creatorBunzarov, I
dc.creatorBurton, TP
dc.creatorButterworth, J
dc.creatorCai, XZ
dc.creatorCaines, H
dc.creatorCalderón De La Barca Sánchez, M
dc.creatorCebra, D
dc.creatorCendejas, R
dc.creatorCervantes, MC
dc.creatorChaloupka, P
dc.creatorChang, Z
dc.creatorChattopadhyay, S
dc.creatorChen, HF
dc.creatorChen, JH
dc.creatorChen, JY
dc.creatorChen, L
dc.creatorCheng, J
dc.creatorCherney, M
dc.creatorChikanian, A
dc.creatorChristie, W
dc.creatorChung, P
dc.creatorChwastowski, J
dc.creatorCodrington, MJM
dc.creatorCorliss, R
dc.creatorCramer, JG
dc.creatorCrawford, HJ
dc.creatorCui, X
dc.creatorDas, S
dc.creatorDavila Leyva, A
dc.creatorDe Silva, LC
dc.creatorDebbe, RR
dc.creatorDedovich, TG
dc.creatorDeng, J
dc.creatorDerradi De Souza, R
dc.creatorDhamija, S
dc.creatorDidenko, L
dc.creatorDing, F
dc.creatorDion, A
dc.creatorDjawotho, P
dc.creatorDong, X
dc.creatorDrachenberg, JL
dc.creatorDraper, JE
dc.creatorDu, CM
dc.creatorDunkelberger, LE
dc.creatorDunlop, JC
dc.creatorEfimov, LG
dc.creatorElnimr, M
dc.creatorEngelage, J
dc.creatorEppley, G
dc.creatorEun, L
dc.creatorEvdokimov, O
dc.creatorFatemi, R
dc.creatorFazio, S
dc.creatorFedorisin, J
dc.creatorFersch, RG
dc.creatorFilip, P
dc.creatorFinch, E
dc.creatorFisyak, Y
dc.creatorFlores, E
dc.creatorGagliardi, CA
dc.creatorGangadharan, DR
dc.creatorGarand, D
dc.creatorGeurts, F
dc.creatorGibson, A
dc.creatorGliske, S
dc.creatorGorbunov, YN
dc.creatorGrebenyuk, OG
dc.creatorGrosnick, D
dc.date.accessioned2021-02-03T20:27:31Z
dc.date.available2021-02-03T20:27:31Z
dc.date.issued2013-07-15
dc.identifier.issn0556-2813
dc.identifier.issn1089-490X
dc.identifier.doihttp://dx.doi.org/10.34944/dspace/5933
dc.identifier.other183TE (isidoc)
dc.identifier.urihttp://hdl.handle.net/20.500.12613/5951
dc.description.abstractWe report measurements of the third harmonic coefficient of the azimuthal anisotropy, v3, known as triangular flow. The analysis is for charged particles in Au+Au collisions at √sNN=200 GeV, based on data from the STAR experiment at the BNL Relativistic Heavy Ion Collider. Two-particle correlations as a function of their pseudorapidity separation are fit with narrow and wide Gaussians. Measurements of triangular flow are extracted from the wide Gaussian, from two-particle cumulants with a pseudorapidity gap, and also from event plane analysis methods with a large pseudorapidity gap between the particles and the event plane. These results are reported as a function of transverse momentum and centrality. A large dependence on the pseudorapidity gap is found. Results are compared with other experiments and model calculations. © 2013 American Physical Society.
dc.format.extent014904-
dc.language.isoen
dc.relation.haspartPhysical Review C - Nuclear Physics
dc.relation.isreferencedbyAmerican Physical Society (APS)
dc.subjectnucl-ex
dc.subjectnucl-ex
dc.titleThird harmonic flow of charged particles in Au + Au collisions at √s<inf>NN</inf>=200 GeV
dc.typeArticle
dc.type.genreJournal Article
dc.relation.doi10.1103/PhysRevC.88.014904
dc.ada.noteFor Americans with Disabilities Act (ADA) accommodation, including help with reading this content, please contact scholarshare@temple.edu
dc.date.updated2021-02-03T20:27:27Z
refterms.dateFOA2021-02-03T20:27:32Z


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