Evidence for Nonlinear Gluon Effects in QCD and their AA Dependence at STAR

preprint2022arXivOpen access
STAR CollaborationM. S. AbdallahB. E. AboonaJ. AdamL. AdamczykJ. R. AdamsJ. K. AdkinsG. AgakishievI. AggarwalM. M. AggarwalZ. AhammedA. AitbaevI. AlekseevD. M. AndersonA. AparinE. C. AschenauerM. U. AshrafF. G. AtetallaG. S. AverichevV. BairathiW. BakerJ. G. Ball CapK. BarishA. BeheraR. BellwiedP. BhagatA. BhasinJ. BielcikJ. BielcikovaI. G. BordyuzhinJ. D. BrandenburgA. V. BrandinX. Z. CaiH. CainesM. Calderón de la Barca SánchezD. CebraI. ChakaberiaP. ChaloupkaB. K. ChanF-H. ChangZ. ChangA. ChatterjeeS. ChattopadhyayD. ChenJ. ChenJ. H. ChenX. ChenZ. ChenJ. ChengS. ChoudhuryW. ChristieX. ChuH. J. CrawfordM. CsanádM. DaugherityT. G. DedovichI. M. DeppnerA. A. DerevschikovA. DhamijaL. Di CarloL. DidenkoP. DixitX. DongJ. L. DrachenbergE. DuckworthJ. C. DunlopJ. EngelageG. EppleyS. EsumiO. EvdokimovA. EwiglebenO. EyserR. FatemiF. M. FawziS. FazioC. J. FengY. FengE. FinchY. FisyakA. FranciscoC. FuC. A. GagliardiT. GalatyukF. GeurtsN. GhimireA. GibsonK. GopalX. GouD. GrosnickA. GuptaW. GurynA. HamedY. HanS. HarabaszM. D. HarastyJ. W. HarrisH. HarrisonS. HeW. HeX. H. HeY. HeS. HeppelmannN. HerrmannE. HoffmanL. HolubC. HuQ. HuY. HuH. HuangH. Z. HuangS. L. HuangT. HuangX. HuangY. HuangT. J. HumanicD. IsenhowerM. IsshikiW. W. JacobsC. JenaA. JentschY. JiJ. JiaK. JiangX. JuE. G. JuddS. KabanaM. L. KabirS. KagamasterD. KalinkinK. KangD. KapukchyanK. KauderH. W. KeD. KeaneA. KechechyanM. KelseyY. V. KhyzhniakD. P. KikołaB. KimelmanD. KincsesI. KiselA. KiselevA. G. KnospeH. S. KoL. KochendaA. KorobitsinL. K. KosarzewskiL. KramarikP. KravtsovL. KumarS. KumarR. Kunnawalkam ElayavalliJ. H. KwasizurR. LaceyS. LanJ. M. LandgrafJ. LauretA. LebedevR. LednickyJ. H. LeeY. H. LeungN. LewisC. LiW. LiX. LiY. LiX. LiangY. LiangR. LicenikT. LinY. LinM. A. LisaF. LiuH. LiuP. LiuT. LiuX. LiuY. LiuZ. LiuT. LjubicicW. J. LlopeR. S. LongacreE. LoydT. LuN. S. LukowX. F. LuoL. MaR. MaY. G. MaN. MagdyD. MallickS. L. ManukhovS. MargetisC. MarkertH. S. MatisJ. A. MazerN. G. MinaevS. MioduszewskiB. MohantyM. M. MondalI. MooneyD. A. MorozovA. MukherjeeM. NagyJ. D. NamMd. NasimK. NayakD. NeffJ. M. NelsonD. B. NemesM. NieG. NigmatkulovT. NiidaR. NishitaniL. V. NogachT. NonakaA. S. NunesG. OdyniecA. OgawaS. OhV. A. OkorokovK. OkuboB. S. PageR. PakJ. PanA. PandavA. K. PandeyY. PanebratsevP. ParfenovA. PaulB. PawlikD. PawlowskaC. PerkinsJ. PlutaB. R. PokhrelJ. PorterM. PosikV. ProzorovaN. K. PruthiM. PrzybycienJ. PutschkeH. QiuA. QuinteroC. RaczS. K. RadhakrishnanN. RahaR. L. RayR. ReedH. G. RitterM. RobotkovaO. V. RogachevskiyJ. L. RomeroD. RoyL. RuanA. K. SahooN. R. SahooH. SakoS. SalurE. SamigullinJ. SandweissS. SatoW. B. SchmidkeN. SchmitzB. R. SchweidF. SeckJ. SegerR. SetoP. SeybothN. ShahE. ShahalievP. V. ShanmuganathanM. ShaoT. ShaoR. SharmaA. I. SheikhD. Y. ShenS. S. ShiY. ShiQ. Y. ShouE. P. SichtermannR. SikoraJ. SinghS. SinghaP. SinhaM. J. SkobyN. SmirnovY. SöhngenW. SolystY. SongH. M. SpinkaB. SrivastavaT. D. S. StanislausM. StefaniakD. J. StewartM. StrikhanovB. StringfellowA. A. P. SuaideM. SumberaB. SummaX. M. SunX. SunY. SunB. SurrowD. N. SviridaZ. W. SwegerP. SzymanskiA. H. TangZ. TangA. TaranenkoT. TarnowskyJ. H. ThomasA. R. TimminsD. TlustyT. TodorokiM. TokarevC. A. TomkielS. TrentalangeR. E. TribbleP. TribedyS. K. TripathyT. TruhlarB. A. TrzeciakO. D. TsaiZ. TuT. UllrichD. G. UnderwoodI. UpsalG. Van BurenJ. VanekA. N. VasilievI. VassilievV. VerkestF. VidebækS. VokalS. A. VoloshinF. WangG. WangJ. S. WangP. WangX. WangY. WangZ. WangJ. C. WebbP. C. WeidenkaffG. D. WestfallH. WiemanS. W. WissinkR. WittJ. WuY. WuB. XiZ. G. XiaoG. XieW. XieH. XuN. XuQ. H. XuY. XuZ. XuG. YanC. YangQ. YangS. YangY. YangZ. YeL. YiK. YipY. YuH. ZbroszczykW. ZhaC. ZhangD. ZhangJ. ZhangS. ZhangY. ZhangZ. J. ZhangZ. ZhangF. ZhaoJ. ZhaoM. ZhaoC. ZhouY. ZhouX. ZhuM. ZurekM. Zyzak

Abstract

The STAR Collaboration reports measurements of back-to-back azimuthal correlations of di-π0π^0s produced at forward pseudorapidities (2.6<η<4.02.6<η<4.0) in pp+pp, p+p+Al, and p+p+Au collisions at a center-of-mass energy of 200 GeV. We observe a clear suppression of the correlated yields of back-to-back π0π^0 pairs in p+p+Al and p+p+Au collisions compared to the pp+pp data. The observed suppression of back-to-back pairs as a function of transverse momentum suggests nonlinear gluon dynamics arising at high parton densities. The larger suppression found in p+p+Au relative to p+p+Al collisions exhibits a dependence of the saturation scale, Qs2Q_s^2, on the mass number, AA. A linear scaling of the suppression with A1/3A^{1/3} is observed with a slope of −0.09-0.09 ±\pm 0.010.01.

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