Measurements of WW and Z/γ∗Z/γ^* cross sections and their ratios in p+pp+p collisions at RHIC

preprint2020arXivOpen access
STAR CollaborationJ. AdamL. AdamczykJ. R. AdamsJ. K. AdkinsG. AgakishievM. M. AggarwalZ. AhammedI. AlekseevD. M. AndersonA. AparinE. C. AschenauerM. U. AshrafF. G. AtetallaA. AttriG. S. AverichevV. BairathiK. BarishA. BeheraR. BellwiedA. BhasinJ. BielcikJ. BielcikovaL. C. BlandI. G. BordyuzhinJ. D. BrandenburgA. V. BrandinJ. ButterworthH. CainesM. Calderón de la Barca SánchezD. CebraI. ChakaberiaP. ChaloupkaB. K. ChanF-H. ChangZ. ChangN. Chankova-BunzarovaA. ChatterjeeD. ChenJ. ChenJ. H. ChenX. ChenZ. ChenJ. ChengM. CherneyM. ChevalierS. ChoudhuryW. ChristieX. ChuH. J. CrawfordM. CsanádM. DaugherityT. G. DedovichI. M. DeppnerA. A. DerevschikovL. DidenkoX. DongJ. L. DrachenbergJ. C. DunlopT. EdmondsN. ElseyJ. EngelageG. EppleyS. EsumiO. EvdokimovA. EwiglebenO. EyserR. FatemiS. FazioP. FedericJ. FedorisinC. J. FengY. FengP. FilipE. FinchY. FisyakA. FranciscoL. FulekC. A. GagliardiT. GalatyukF. GeurtsA. GibsonK. GopalX. GouD. GrosnickW. GurynA. I. HamadA. HamedS. HarabaszJ. W. HarrisS. HeW. HeX. H. HeY. HeS. HeppelmannN. HerrmannE. HoffmanL. HolubY. HongS. HorvatY. HuH. Z. HuangS. L. HuangT. HuangX. HuangT. J. HumanicP. HuoG. IgoD. IsenhowerW. W. JacobsC. JenaA. JentschY. JiJ. JiaK. JiangS. JowzaeeX. JuE. G. JuddS. KabanaM. L. KabirS. KagamasterD. KalinkinK. KangD. KapukchyanK. KauderH. W. KeD. KeaneA. KechechyanM. KelseyY. V. KhyzhniakD. P. KikołaC. KimB. KimelmanD. KincsesT. A. KinghornI. KiselA. KiselevM. KocanL. KochendaD. D. KoetkeL. K. KosarzewskiL. KramarikP. KravtsovK. KruegerN. Kulathunga MudiyanselageL. KumarS. KumarR. Kunnawalkam ElayavalliJ. H. KwasizurR. LaceyS. LanJ. M. LandgrafJ. LauretA. LebedevR. LednickyJ. H. LeeY. H. LeungC. LiW. LiX. LiY. LiY. LiangR. LicenikT. LinY. LinM. A. LisaF. LiuH. LiuP. LiuT. LiuX. LiuY. LiuZ. LiuT. LjubicicW. J. LlopeR. S. LongacreN. S. LukowS. LuoX. LuoG. L. MaL. MaR. MaY. G. MaN. MagdyR. MajkaD. MallickS. MargetisC. MarkertH. S. MatisJ. A. MazerN. G. MinaevS. MioduszewskiB. MohantyI. MooneyZ. MoravcovaD. A. MorozovM. NagyJ. D. NamMd. NasimK. NayakD. NeffJ. M. NelsonD. B. NemesM. NieG. NigmatkulovT. NiidaL. V. NogachT. NonakaA. S. NunesG. OdyniecA. OgawaS. OhV. A. OkorokovB. S. PageR. PakA. PandavY. PanebratsevB. PawlikD. PawlowskaH. PeiC. PerkinsL. PinskyR. L. PintérJ. PlutaJ. PorterM. PosikN. K. PruthiM. PrzybycienJ. PutschkeH. QiuA. QuinteroS. K. RadhakrishnanS. RamachandranR. L. RayR. ReedH. G. RitterO. V. RogachevskiyJ. L. RomeroL. RuanJ. RusnakN. R. SahooH. SakoS. SalurJ. SandweissS. SatoW. B. SchmidkeN. SchmitzB. R. SchweidF. SeckJ. SegerM. SergeevaR. SetoP. SeybothN. ShahE. ShahalievP. V. ShanmuganathanM. ShaoA. I. SheikhW. Q. ShenS. S. ShiY. ShiQ. Y. ShouE. P. SichtermannR. SikoraM. SimkoJ. SinghS. SinghaN. SmirnovW. SolystP. SorensenH. M. SpinkaB. SrivastavaT. D. S. StanislausM. StefaniakD. J. StewartM. StrikhanovB. StringfellowA. A. P. SuaideM. SumberaB. SummaX. M. SunX. SunY. SunB. SurrowD. N. SviridaP. SzymanskiA. H. TangZ. TangA. TaranenkoT. TarnowskyJ. H. ThomasA. R. TimminsD. TlustyM. TokarevC. A. TomkielS. TrentalangeR. E. TribbleP. TribedyS. K. TripathyO. D. TsaiZ. TuT. UllrichD. G. UnderwoodI. UpsalG. Van BurenJ. VanekA. N. VasilievI. VassilievF. VidebækS. VokalS. A. VoloshinF. WangG. WangJ. S. WangP. WangY. WangZ. WangJ. C. WebbP. C. WeidenkaffL. WenG. D. WestfallH. WiemanS. W. WissinkR. WittY. WuZ. G. XiaoG. XieW. XieH. XuN. XuQ. H. XuY. F. XuY. XuZ. XuC. YangQ. YangS. YangY. YangZ. YangZ. YeL. YiK. YipY. YuH. ZbroszczykW. ZhaC. ZhangD. ZhangS. ZhangX. P. ZhangY. ZhangZ. J. ZhangZ. ZhangJ. ZhaoC. ZhongC. ZhouX. ZhuZ. ZhuM. ZurekM. Zyzak

Abstract

We report on the WW and Z/γ∗Z/γ^* differential and total cross sections as well as the W+W^+/W−W^- and (W++W−)(W^+ + W^-)/(Z/γ∗)(Z/γ^*) cross-section ratios measured by the STAR experiment at RHIC in p+pp+p collisions at s=500\sqrt{s} = 500 GeV and 510510 GeV. The cross sections and their ratios are sensitive to quark and antiquark parton distribution functions. In particular, at leading order, the WW cross-section ratio is sensitive to the dˉ/uˉ\bar{d}/\bar{u} ratio. These measurements were taken at high Q2∼MW2,MZ2Q^2 \sim M_W^2,M_Z^2 and can serve as input into global analyses to provide constraints on the sea quark distributions. The results presented here combine three STAR data sets from 2011, 2012, and 2013, accumulating an integrated luminosity of 350 pb−1^{-1}. We also assess the expected impact that our W+/W−W^+/W^- cross-section ratios will have on various quark distributions, and find sensitivity to the uˉ−dˉ\bar{u}-\bar{d} and dˉ/uˉ\bar{d}/\bar{u} distributions.

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