System size and energy dependence of near-side di-hadron correlations

preprint2011arXivOpen access
STAR CollaborationG. AgakishievM. M. AggarwalZ. AhammedA. V. AlakhverdyantsI. AlekseevJ. AlfordB. D. AndersonC. D. AnsonD. ArkhipkinG. S. AverichevJ. BalewskiL. S. BarnbyD. R. BeavisR. BellwiedM. J. BetancourtR. R. BettsA. BhasinA. K. BhatiH. BichselJ. BielcikJ. BielcikovaL. C. BlandM. BombaraI. G. BordyuzhinW. BorowskiJ. BouchetE. BraidotA. V. BrandinS. G. BrovkoE. BrunaS. BueltmannI. BunzarovT. P. BurtonX. Z. CaiH. CainesM. Calderón de la Barca SánchezD. CebraR. CendejasM. C. CervantesP. ChaloupkaS. ChattopadhyayH. F. ChenJ. H. ChenJ. Y. ChenL. ChenJ. ChengM. CherneyA. ChikanianW. ChristieP. ChungM. J. M. CodringtonR. CorlissJ. G. CramerH. J. CrawfordX. CuiA. Davila LeyvaL. C. De SilvaR. R. DebbeT. G. DedovichJ. DengA. A. DerevschikovR. Derradi de SouzaS. DhamijaL. DidenkoP. DjawothoX. DongJ. L. DrachenbergJ. E. DraperC. M. DuL. E. DunkelbergerJ. C. DunlopL. G. EfimovM. ElnimrJ. EngelageG. EppleyL. EunO. EvdokimovR. FatemiJ. FedorisinR. G. FerschP. FilipE. FinchY. FisyakC. A. GagliardiL. GaillardD. R. GangadharanF. GeurtsP. GhoshS. GliskeY. N. GorbunovO. G. GrebenyukD. GrosnickA. GuptaS. GuptaW. GurynB. HaagO. HajkovaA. HamedL-X. HanJ. W. HarrisJ. P. Hays-WehleS. HeppelmannA. HirschG. W. HoffmannD. J. HofmanS. HorvatB. HuangH. Z. HuangT. J. HumanicL. HuoG. IgoW. W. JacobsC. JenaP. G. JonesJ. JosephE. G. JuddS. KabanaK. KangJ. KapitanK. KauderH. W. KeD. KeaneA. KechechyanD. KettlerD. P. KikolaJ. KirylukA. KisielV. KizkaS. R. KleinD. D. KoetkeT. KolleggerJ. KonzerI. KoraltL. KorolevaW. KorschL. KotchendaP. KravtsovK. KruegerL. KumarM. A. C. LamontJ. M. LandgrafS. LaPointeJ. LauretA. LebedevR. LednickyJ. H. LeeW. LeightM. J. LeVineC. LiL. LiW. LiX. LiY. LiZ. M. LiL. M. LimaM. A. LisaF. LiuT. LjubicicW. J. LlopeR. S. LongacreY. LuE. V. LukashovX. LuoG. L. MaY. G. MaD. P. MahapatraR. MajkaO. I. MallS. MargetisC. MarkertH. MasuiH. S. MatisD. McDonaldT. S. McShaneN. G. MinaevS. MioduszewskiM. K. MitrovskiY. MohammedB. MohantyM. M. MondalB. MorozovD. A. MorozovM. G. MunhozM. K. MustafaM. NaglisB. K. NandiC. NattrassMd. NasimT. K. NayakL. V. NogachS. B. NurushevG. OdyniecA. OgawaK. OhA. OhlsonV. OkorokovE. W. OldagR. A. N. OliveiraD. OlsonM. PachrB. S. PageS. K. PalPanY. PanditY. PanebratsevT. PawlakH. PeiC. PerkinsW. PerytP. PileM. PlaninicJ. PlutaD. PlykuN. PoljakJ. PorterA. M. PoskanzerC. B. PowellD. PrindleC. PruneauN. K. PruthiP. R. PujahariJ. PutschkeH. QiuR. RaniwalaS. RaniwalaR. L. RayR. RedwineR. ReedC. K. RileyH. G. RitterJ. B. RobertsO. V. RogachevskiyJ. L. RomeroL. RuanJ. RusnakN. R. SahooI. SakrejdaS. SalurJ. SandweissE. SangalineA. SarkarJ. SchambachR. P. ScharenbergA. M. SchmahN. SchmitzT. R. SchusterJ. SeeleJ. SegerP. SeybothN. ShahE. ShahalievM. ShaoB. SharmaM. SharmaS. S. ShiQ. Y. ShouE. P. SichtermannR. N. SingarajuM. J. SkobyN. SmirnovD. SolankiP. SorensenU. G. deSouzaH. M. SpinkaB. SrivastavaT. D. S. StanislausS. G. SteadmanJ. R. StevensR. StockM. StrikhanovB. StringfellowA. A. P. SuaideM. C. SuarezM. SumberaX. M. SunY. SunZ. SunB. SurrowD. N. SviridaT. J. M. SymonsA. Szanto de ToledoJ. TakahashiA. H. TangZ. TangL. H. TariniT. TarnowskyD. TheinJ. H. ThomasJ. TianA. R. TimminsD. TlustyM. TokarevS. TrentalangeR. E. TribbleP. TribedyB. A. TrzeciakO. D. TsaiT. UllrichD. G. UnderwoodG. Van BurenG. van NieuwenhuizenJ. A. Vanfossen, Jr.R. VarmaG. M. S. VasconcelosA. N. VasilievF. VidebæY. P. ViyogiS. VokalS. A. VoloshinA. VossenM. WadaG. WangH. WangJ. S. WangQ. WangX. L. WangY. WangG. WebbJ. C. WebbG. D. WestfallC. Whitten Jr.H. WiemanS. W. WissinkR. WittW. WitzkeY. F. WuZ. XiaoW. XieH. XuN. XuQ. H. XuW. XuY. XuZ. XuL. XueY. YangP. YepesY. YiK. YipI-K. YooM. ZawiszaH. ZbroszczykW. ZhanJ. B. ZhangS. ZhangW. M. ZhangX. P. ZhangY. ZhangZ. P. ZhangF. ZhaoJ. ZhaoC. ZhongX. ZhuY. H. ZhuY. Zoulkarneeva

Abstract

Two-particle azimuthal (ΔϕΔϕ) and pseudorapidity (ΔηΔη) correlations using a trigger particle with large transverse momentum (pTp_T) in dd+Au, Cu+Cu and Au+Au collisions at sNN\sqrt{s_{NN}} =\xspace 62.4 GeV and 200~GeV from the STAR experiment at RHIC are presented. The \ns correlation is separated into a jet-like component, narrow in both ΔϕΔϕ and ΔηΔη, and the ridge, narrow in ΔϕΔϕ but broad in ΔηΔη. Both components are studied as a function of collision centrality, and the jet-like correlation is studied as a function of the trigger and associated pTp_T. The behavior of the jet-like component is remarkably consistent for different collision systems, suggesting it is produced by fragmentation. The width of the jet-like correlation is found to increase with the system size. The ridge, previously observed in Au+Au collisions at sNN\sqrt{s_{NN}} = 200 GeV, is also found in Cu+Cu collisions and in collisions at sNN\sqrt{s_{NN}} =\xspace 62.4 GeV, but is found to be substantially smaller at sNN\sqrt{s_{NN}} =\xspace 62.4 GeV than at sNN\sqrt{s_{NN}} = 200 GeV for the same average number of participants (⟨Npart⟩ \langle N_{\mathrm{part}}\rangle). Measurements of the ridge are compared to models.

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