Strangeness Enhancement in Cu+Cu and Au+Au Collisions at \sqrt{s_{NN}} = 200 GeV

preprint2012arXivOpen access
STAR CollaborationH. AgakishievM. M. AggarwalZ. AhammedA. V. AlakhverdyantsI. AlekseevJ. AlfordB. D. AndersonC. D. AnsonD. ArkhipkinG. S. AverichevJ. BalewskiL. S. BarnbyD. R. BeavisN. K. BeheraR. BellwiedM. J. BetancourtR. R. BettsA. BhasinA. K. BhatiH. BichselJ. BielcikJ. BielcikovaB. BiritzL. C. BlandW. BorowskiJ. BouchetE. BraidotA. V. BrandinA. BridgemanS. G. BrovkoE. BrunaS. BueltmannI. BunzarovT. P. BurtonX. Z. CaiH. CainesM. Calderón de la Barca SánchezD. CebraR. CendejasM. C. CervantesZ. ChajeckiP. ChaloupkaS. ChattopadhyayH. F. ChenJ. H. ChenJ. Y. ChenL. ChenJ. ChengM. CherneyA. ChikanianK. E. ChoiW. ChristieP. ChungM. J. M. CodringtonR. CorlissJ. G. CramerH. J. CrawfordS. DashA. Davila LeyvaL. C. De SilvaR. R. DebbeT. G. DedovichA. A. DerevschikovR. Derradi de SouzaL. DidenkoP. DjawothoS. M. DograX. DongJ. L. DrachenbergJ. E. DraperJ. C. DunlopL. G. EfimovM. ElnimrJ. EngelageG. EppleyM. EstienneL. EunO. EvdokimovR. FatemiJ. FedorisinR. G. FerschP. FilipE. FinchV. FineY. FisyakC. A. GagliardiD. R. GangadharanA. GeromitsosF. GeurtsP. GhoshY. N. GorbunovA. GordonO. GrebenyukD. GrosnickS. M. GuertinA. GuptaW. GurynB. HaagO. HajkovaA. HamedL-X. HanJ. W. HarrisJ. P. Hays-WehleM. HeinzS. HeppelmannA. HirschE. HjortG. W. HoffmannD. J. HofmanB. HuangH. Z. HuangT. J. HumanicL. HuoG. IgoP. JacobsW. W. JacobsP. G. JonesC. JenaF. JinJ. JosephE. G. JuddS. KabanaK. KangJ. KapitanK. KauderH. KeD. KeaneA. KechechyanD. KettlerD. P. KikolaJ. KirylukA. KisielV. KizkaA. G. KnospeD. D. KoetkeT. KolleggerJ. KonzerI. KoraltL. KorolevaW. KorschL. KotchendaV. KouchpilP. KravtsovK. KruegerM. KrusL. KumarP. KurnadiM. A. C. LamontJ. M. LandgrafS. LaPointeJ. LauretA. LebedevR. LednickyJ. H. LeeW. LeightM. J. LeVineC. LiL. LiN. LiW. LiX. LiY. LiZ. M. LiM. A. LisaF. LiuH. LiuJ. LiuT. LjubicicW. J. LlopeR. S. LongacreW. A. LoveY. LuE. V. LukashovX. LuoG. L. MaY. G. MaD. P. MahapatraR. MajkaO. I. MallL. K. MangotraR. ManweilerS. MargetisC. MarkertH. MasuiH. S. MatisYu. A. MatulenkoD. McDonaldT. S. McShaneA. MeschaninR. MilnerN. G. MinaevS. MioduszewskiA. MischkeM. K. MitrovskiB. MohantyM. M. MondalB. MorozovD. A. MorozovM. G. MunhozM. NaglisB. K. NandiT. K. NayakP. K. NetrakantiJ. M. NelsonL. V. NogachS. B. NurushevG. OdyniecA. OgawaK. OhA. OhlsonV. OkorokovE. W. OldagD. OlsonM. PachrB. S. PageS. K. PalY. PanditY. PanebratsevT. PawlakH. PeiT. PeitzmannC. PerkinsW. PerytS. C. PhatakP. PileM. PlaninicM. A. PloskonJ. PlutaD. PlykuN. PoljakA. M. PoskanzerB. V. K. S. PotukuchiC. B. PowellD. PrindleC. PruneauN. K. PruthiP. R. PujahariJ. PutschkeH. QiuR. RaniwalaS. RaniwalaR. L. RayR. RedwineR. ReedH. G. RitterJ. B. RobertsO. V. RogachevskiyJ. L. RomeroA. RoseL. RuanJ. RusnakN. R. SahooS. SakaiI. SakrejdaT. SakumaS. SalurJ. SandweissE. SangalineA. SarkarJ. SchambachR. P. ScharenbergA. M. SchmahT. R. SchusterJ. SeeleJ. SegerI. SelyuzhenkovP. SeybothE. ShahalievM. ShaoM. SharmaS. S. ShiQ. Y. ShouE. P. SichtermannF. SimonR. N. SingarajuM. J. SkobyN. SmirnovH. M. SpinkaB. SrivastavaT. D. S. StanislausD. StaszakS. G. SteadmanJ. R. StevensR. StockM. StrikhanovB. StringfellowA. A. P. SuaideM. C. SuarezN. L. SubbaM. 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. TokarevV. N. TramS. TrentalangeR. E. TribbleP. TribedyO. D. TsaiT. UllrichD. G. UnderwoodG. Van BurenG. van NieuwenhuizenJ. A. Vanfossen Jr.R. VarmaG. M. S. VasconcelosA. N. VasilievF. VidebækY. P. ViyogiS. VokalM. WadaM. WalkerF. WangG. 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. YepesK. YipI-K. YooM. ZawiszaH. ZbroszczykW. ZhanJ. B. ZhangS. ZhangW. M. ZhangX. P. ZhangY. ZhangZ. P. ZhangJ. ZhaoC. ZhongW. ZhouX. ZhuY. H. ZhuR. ZoulkarneevY. Zoulkarneeva

Abstract

We report new STAR measurements of mid-rapidity yields for the ΛΛ, Λˉ\barΛ, KS0K^{0}_{S}, Ξ−Ξ^{-}, Ξˉ+\barΞ^{+}, Ω−Ω^{-}, Ωˉ+\barΩ^{+} particles in Cu+Cu collisions at \sNN{200}, and mid-rapidity yields for the ΛΛ, Λˉ\barΛ, KS0K^{0}_{S} particles in Au+Au at \sNN{200}. We show that at a given number of participating nucleons, the production of strange hadrons is higher in Cu+Cu collisions than in Au+Au collisions at the same center-of-mass energy. We find that aspects of the enhancement factors for all particles can be described by a parameterization based on the fraction of participants that undergo multiple collisions.

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