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Single Spin Transverse Asymmetries of Neutral Pions at Forward Rapidities in sqrt(s) = 62.4 GeV Polarized Proton Collisions in PHENIX PDF

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Single Spin Transverse Asymmetries of Neutral Pions at Forward Rapidities in √s = 62.4 GeV Polarized Proton Collisions in PHENIX Mickey Chiu for the PHENIX Collaboration 7 0 Dept.ofPhysics,UniversityofIllinois,Urbana,IL61801USA1 0 2 Abstract. In the RHIC run of 2006, PHENIX recorded data from about 20 nb 1 of transversely n − polarized p+p collisions at √s = 62.4 GeV and polarization of about 50%. Also in this last run a J PHENIX successfullycommissioneda newPbWO4 basedelectromagneticcalorimeter,theMuon PistonCalorimeter(MPC),covering2p inazimuthand3.1<h <3.7.Theforwardcoverageallows 2 2 PHENIX to measure high xF p 0 production.We presentthe currentstatus of the analysis for the singleinclusivep 0transverseasymmetryAN atforwardrapiditiesinPHENIX. 1 Keywords: Protonspin,Singletransversespinasymmetry v PACS: 13.85.Ni,13.88.+e,14.20.Dh 1 3 0 1 INTRODUCTION 0 7 Transverse single spin asymmetries in hadronic collisions have had a long history of 0 / surprises, such as the observation by the E704 collaboration of very large asymmetries x e in inclusive pion production at high xF in √s = 19.4 GeV transversely polarized p↑p - collisions[1, 2]. Naively in leading twist perturbative QCD one expects these asymme- l c tries to be powersuppressed such that A a m /p [3]. It was thought that at higher u N S q T ∼ n energies these asymmetries would be strongly suppressed. Quite surprisingly, however, : largeasymmetrieswerediscoveredtopersistevenatcolliderenergiesbyfirstSTARand v i thentheBrahmscollaboration[4, 5]. X These asymmetries are interesting because they point toward some new understand- r a ingofinternalprotonstructure,suchastheexistenceofanewnon-perturbativefunction liketheSiversfunction[6],orperhapsanon-zerotransversitydistributioninconjunction with a transversely dependent fragmentation function[7] (Collins effect). Of particular interest is that these effects occur in a regime where NLO pQCD calculations correctly predict the unpolarized cross-sections. Therefore the hope is that one can understand theseasymmetriesunambiguously,suchaswithahighertwistexpansionapproach[8,9], orbytakingintoaccountthetransversemotionofpartonsinaLOcollinearlyfactorized approach with non-perturbative, transverse-momentum dependent functions[10]. Fur- therprogressintheoreticalunderstandingrequiresmoredifferentialmeasurementssuch as the p and x dependenceoftheasymmetry,as wellas di-hadron correlations[11]to T F distinguishbetween theaboveapproaches. 1 Presentaddress:BrookhavenNationalLaboratory,Upton,NY11375 MPC DATA ANALYSIS AND CURRENT STATUS Before the 2006 run, PHENIX initiated a program to install a calorimeter inside the hole at the front of the muon magnet piston2 to extend the kinematic reach of PHENIX calorimetry to more forward rapidities. The muon piston holes are cylindri- cal with a depth of 43.1 cm and a di- ameter of 42 cm. The small size of the area, proximity to the interaction point, and sizable magnetic fields en- force tight constraints on the calorime- ter’s design, requiring a compact ma- terial with short radiation length and small moliere radius and a readout that is insensitive to magnetic fields. PHENIX chose a design, based on that 1:ThePHENIXSouthMPCLayout. of the ALICE PHOS detector[12], of a highlysegmentedlead-tungstatecrystal arraywithAvalanchePhotodiode(APD)readout.Lead-tungstateisoneofthebestcandi- datematerialsforacompactcalorimetersinceithasoneofthesmallestradiationlength (0.89cm)and moliereradius (2.0 cm)ofany knownscintillator.PHENIX installed192 crystalsofsize2.2 2.2 18cm3 inthesouthpistonholeintimeforthe2006RHICrun. × × Thecalorimetersitsaroundthebeam-pipe223cmfromtheinteractionpointandcovers 3.1<h <3.7. The layout of the south MPC is shown in figure 1. Another220 crystals willbeinstalledin thenorth pistonholefor2007. Further detailson theMPC hardware can befoundinthecontributionofA. Kazantsevintheseproceedings[13]. Thedatashownhereweretakenwith the PHENIX detector at RHIC during twodaysofthe2006 p prun,atabeam 1400 ↑ energy of √s=62.4 GeV. A total inte- 1200 grated luminosityof 20 nb 1 of data − 1000 ∼ were collected. The data are triggered 800 with the MPC using 4x4 tower energy 600 sums at a threshold of 5 GeV, cor- ∼ 400 responding to good trigger efficiency for p 0 at 10 GeV. An additional 80 200 nb 1 ofda∼tawere takenwithlongitudi- 00 0.2 0.4 0.6 0.8 1 − inv. mass mg g (GeV) nallypolarizedbeamsatthesamebeam energy[13]. 2: Theinvariantmassdistributionofphotonpairs The MPC clustering algorithm in the South MPC for p+p collisions at √s = is based on that developed for the NN 62.4 GeV. The mixed eventdistribution is shown PHENIX central arm calorimeter. In inthereddashed-dottedline. this algorithm the known shower shape from test-beam measurements is used to reconstruct the hit location and energy of photonswhen thetwophotonsareseparated enough toseetwo peaks. Alternativealgo- rithmsarebeinginvestigatedwhichwouldhavegreatereffectivenessathigherenergies, 2 This idea was first suggested by K. Imai and Y. Goto in 1996, and rediscovered recently. See http://www.phenix.bnl.gov/WWW/publish/goto/Polarimetry/pol1.html where the probability for the two decay photons to merge within the same or adjacent towersislarge, and itbecomesdifficultto separateoneversustwophotonshowers.The algorithmsareevaluatedbysimulation.Infigure2theinvariantmassdistributionmgg of clusterpairsisshown,alongwithpairsgeneratedforclustersfrommixedevents.Mixing clusters from different events provides an estimate of the combinatorial background. Notethat a region in the lowerright quadrant ofthe MPC was excluded in this plot due to issues with electronics noise. Currently, the energy scale has been checked with the MIPpeak andp 0 peak andbothhavebeen foundto beconsistenttobetterthan 10%. Thesingletransversespinrawasymmetryasafunctionoff wascalculatedusingthe square-rootformula[14, 15] A(f )= 1 e (f )= 1 ds ↑,f −ds ↓,f = 1 qNL↑,f NR↓,f −qNL↓,f NR↑,f (1) PB N PBds ↑,f +ds ↓,f PBqNL↑,f NR↓,f +qNL↓,f NR↑,f which largely cancels out differences in detector and beam asymmetries. f is the az- imuthalanglerelativetothebeampolarizationdirection,andds ,f representsthecross- ↑ section into the f direction for a vertically polarized beam with polarization P . The B asymmetryA is thentheamplitudeofthisasymmetrymodulation,A(f )=A sin(f ). N N In figure 3 we have plotted on the left (right) the raw asymmetry e (f ) for photon N pairs within the p 0 mass peak for the cases where the yellow (blue) beam is polarized. InPHENIXtheyellowbeamistheprotonbeamheadingtowardstheMPC,andtheblue beamis theoneheadingaway. 0.04 p 0 ˛ , forward x 0.04 p 0 ˛ , backward x N F N F 0.03 0.03 0.02 0.02 0.01 0.01 0 0 -0.01 -0.01 -0.02 -0.02 -0.03 -0.03 -0.04 -0.04 -0.05 -0.05 -1.5 -1 -0.5 0 0.5 1 1.5 -1.5 -1 -0.5 0 0.5 1 1.5 f f 3: Raw asymmetries from reconstructed photon pairs within 0.05 < mgg < 0.25 GeV and 9 < Egg < 12 GeV. The asymmetry has not been corrected for combinatoric background or beampolarization. There is a non-zero asymmetry for the case where the yellow beam is polarized, corresponding to positive x with respect to the polarized beam. This asymmetry has F been seen to increase from low x to higher x , and is well described by a sin(f ) F F functionalform.Forthecaseof thepolarized bluebeam (correspondingtonegativex ) F the asymmetry is consistent with zero. As an additional cross-check, the asymmetries were found to be consistent with zero for the longitudinallypolarized runs, as expected sincethen theresidual transversepolarizationissmall. CONCLUSIONS AND FUTURE PLANS PHENIXhassuccessfullycommissionedanewforwardelectromagneticcalorimeter,the south MPC, during the 2006 RHIC run, and plans to install the north MPC in time for 2007.Withanearlyversionoftheclusteringcode,p 0’shavebeenidentifiedintheMPC andanon-zerotransverseasymmetryhasbeen seenin p p collisionsat√s=62.4GeV. ↑ Muchworkremainsinimprovingthereconstructioncodeandinunderstandinganyother artifactsofthedata,suchasnoiseissues,backgrounds,andimprovingthedetermination oftheenergyscale,beforePHENIXcnafinalizethecross-sectionandasymmetryresults from the MPC. The validity of a perturbative theoretical interpretation of this data-set is currently under study. It is known that NLO pQCD fails to correctly describe the inclusivecross-sectioncorrectlyattheseenergiesintheforwardrapidities[16].However, includingthresholdresummationshouldimprovetheagreement[17]. Besides thetransversely polarized data at 62.4 GeV, PHENIX also collected 80 nb 1 − oflongitudinallypolarizeddataat√s=62.4GeVandanother7.5 pb 1oflongitudinally − polarized data at √s = 200 GeV during the 2006 run. The installation of the MPC allows PHENIX to confirm and contribute to previous measurements at high x in F RHIC collisions. Beyond mapping out the x and p dependence of A , the high rate F T N capabilitiesofthePHENIXDAQwillallowexcellenttriggeringcapabilityfordi-hadron correlation measurements between forward p 0 and mid-rapidity hadrons. Di-hadron measurementsare particularly interesting sincethey shouldhelp to distinguishbetween an asymmetry from an initial state effect (Sivers) or a final state effect (Collins plus transversity).Additionally,di-hadron correlations constrain thekinematicsof theinitial scattered partons and therefore provide greater sensitivity to the sampled momentum fractionx ofthosepartons. REFERENCES 1. D.L.Adams,etal.,Phys.Lett.B261,201–206(1991). 2. D.L.Adams,etal.,Phys.Lett.B264,462–466(1991). 3. G.L.Kane,J.Pumplin,andW.Repko,Phys.Rev.Lett.41,1689(1978). 4. J.Adams,etal.,Phys.Rev.Lett.92,171801(2004),hep-ex/0310058. 5. F.Videbaek,AIPConf.Proc.792,993–996(2005),nucl-ex/0508015. 6. D.W.Sivers,Phys.Rev.D41,83(1990). 7. J.C.Collins,Nucl.Phys.B396,161–182(1993),hep-ph/9208213. 8. J.-w.Qiu,andG.Sterman,Phys.Rev.D59,014004(1999),hep-ph/9806356. 9. Y.Koike,AIPConf.Proc.675,449–453(2003),hep-ph/0210396. 10. M.Anselmino,etal.,Phys.Rev.D73,014020(2006),hep-ph/0509035. 11. D.Boer,andW.Vogelsang,Phys.Rev.D69,094025(2004),hep-ph/0312320. 12. CERN/LHCC99-4,ALICETDR2(1999). 13. A.Kazantsev,theseproceedings(2006). 14. G.G.Ohlsen,andP.W.Keaton,Nucl.Instrum.Meth.109,41–59(1973). 15. H.Spinka,ArgonneNationalLaboratoryReportANL-HEP-TR-99-113(1999). 16. C.Bourrely,andJ.Soffer,Eur.Phys.J.C36,371–374(2004),hep-ph/0311110. 17. D.deFlorian,andW.Vogelsang,Phys.Rev.D71,114004(2005),hep-ph/0501258.

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