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First LHC results on coherent J/psi photoproduction in ultra-peripheral Pb-Pb collisions at sqrt{s_NN} = 2.76 TeV PDF

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Preview First LHC results on coherent J/psi photoproduction in ultra-peripheral Pb-Pb collisions at sqrt{s_NN} = 2.76 TeV

y Coherent J/ photoproduction in ultra-peripheral Pb-Pb collisions at √s = 2.76 TeV 1 NN J.D. Tapia Takaki (for the ALICE Collaboration) 2 3 1 0 InstitutedePhysiqueNucléaired’Orsay(IPNO), 2 UniversitéParis-Sud,CNRS-IN2P3,Orsay,France. n a J Abstract. ThefirstLHCmeasurementonultra-peripheralheavy-ioncollisionswascarriedoutwith theALICEexperiment.Inthispaper,ALICEresultsonexclusiveJ/y studiesinPb-Pbcollisionsat 3 2 √sNN =2.76TeV,intherapidityregion-3.6<y<-2.6,aregiven.ThecoherentJ/y crosssection was found to be ds coh/dy = 1.00 0.18 (stat) +0.24 (syst) mb. These studies favour theoretical J/y ± 0.26 ] modelsthatincludestrongmodificationstothenu−cleargluondensity,alsoknownasnucleargluon x shadowing. e - p Keywords: Ultra-peripheralcollisions,heavyquarkonia e PACS: 14.40.Pq,13.40.-f,13.25.Gv,25.75.-q h [ INTRODUCTION 1 v 7 Ultra-peripheral heavy-ion collisions (UPC) can take place when the ions pass by each 5 5 other with impact parameters larger than the sum of their radii. UPC reactions are 5 governed by two-photon and photonuclear interactions, while those of hadronic nature . 1 are strongly suppressed [2, 3]. This is so as the electromagnetic field of the nucleus 0 enhancestheintensityofthevirtualphotonflux.Notethatthenumberofphotonsscales 3 1 likeZ2, where Z is the nucleus charge. Thevirtuality of thephoton is 1/R 30 MeV/c, : whereR is theradius ofthenucleus. ∼ v i In recent years, there has been an increasing interest in ultra-peripheral collisions X forvariouscollidingsystemsat different energies. In particular, exclusivevectormeson r a production in heavy-ion reactions is expected to probe the nuclear gluon density [4, 5], for which their is considerable uncertainty at low values of Bjorken-x. At the forward rapidities studied here, the relevant values of x are 10 2 and 10 5. Note that either − − nucleus can serve as photon emitter or photon tar∼get. Exclus∼ive J/y production has been recently measured in Au-Au collisions at RHIC [6]. However, their measurement suffered from very low statistics. Hence, no conclusions concerning nuclearshadowing weremade. Thispaperwillfocus on thefirst LHCmeasurement onexclusivephotoproductionof 1 Presented at DIFFRACTION 2012: International Workshop on Diffraction in High-Energy Physics. PuertodelCarmen,CanaryIslands,10-15September2012. 2 [email protected] J/y vector mesons produced in Pb-Pb collisions at √s = 2.76 TeV [1]. This paper NN begins by describing the experimental apparatus and the collected data, it will then go ontodiscusstheanalysisstepsandthewaythecoherentJ/y crosssectionwasobtained. This paper will also mention how J/y photoproduction is treated by several theoretical models, as well as givingthe comparison of the measured cross section to the available predictions.Finally,asummarywillbegiven. ALICE DETECTOR The ALICE detector is described elsewhere [7]. The ALICE muon system consists of a spectrometer covering the pseudo-rapidity region -4.0 <h < -2.5. It was designed to identifymuonswithamomentumlargerthan4GeV/c.Itconsistsofafrontabsorberfol- lowedbya3T mdipolemagnet,fivetrackingstationsbasedonCathodePadChambers, · a passive muon-filter wall, and two trigger stations composed of Resistive Plate Cham- bers. In this analysis, the Silicon Pixel Detector, the Zero Degree Calorimeters and the VZERO counters were also used. The VZERO consists of two arrays of 32 scintillator counters each, which are placed around the beam pipe on either side of the interac- tion region: VZERO-A and VZERO-C cover the pseudo-rapidity range 2.8 < h <5.1 and -3.7< h <-1.7, respectively. Finally, two sets of hadronic Zero-Degree Calorime- ters (ZDCs) are located at 116 m on either side of the Interaction Point. These detect neutrons emitted in the very forward region, for example neutrons emitted following electromagneticdissociation. ANALYSIS STEPS AND RESULTS Thisanalysiswascarriedoutonadatasamplecorrespondingtoanintegratedluminosity of 55 m b 1 collected during the 2011 Pb running. A dedicated UPC trigger was active − to select dimuonsin an otherwiseempty detector, both from gg and from J/y decays. It demandedthefollowingeventcharacteristics:(i)asinglemuontriggerabovea1GeV/c p -threshold;(ii)at leastone hitin theVZERO-C detector, and (iii)no hitsin VZERO- T A. A detailed description of the event selection can be found in [1]. Standard cuts to ensure a good muon selection were required [8], followed by other cuts to suppress the remaining hadronic background. In particular, the VZERO offline timing was required to be compatible with crossing beams, and only events with a neutron ZDC signal below 6 TeV were kept. This cut does not remove any events with a J/y produced with a transverse momentum below 0.3 GeV/c, but reduces hadronic contamination at higher p . This analysis deals with exclusive reactions, i.e. Pb+Pb Pb+Pb + T J/y . For this reason, only events with exactly two oppositely charged →muons were selected.Afterapplyingtheseselections,theJ/y yieldwasdescribed asthesumoffour physics processes: coherent and incoherent J/y photoproduction, gg continuum, and J/y candidates from the y ′ decay. Coherent J/y candidates are those where the photon couples coherently to all nucleons in the reaction (target nucleus normally does not break up). On the other hand, incoherent J/y photoproduction occurs when the photon couples to a single nucleon, i.e. the quasi-elastic scattering off a single nucleon. In this Pb+Pb fi Pb+Pb+J/y s = 2.76 TeV NN ) c ALICE V/ 35 -3.6<y<-2.6 e M 30 Data 0 Sum 4 ( 25 Coherent J/y s / Incoherent J/y ate 20 J/y from y ’ decays did 15 g g fi m +m - n a 10 c yJ/ 5 0 0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 Dimuon p (GeV/c) t FIGURE1. Dimuon p distributionforeventssatisfyingtheeventselectiondescribedinthetext,with T the p -range extended to p < 0.8 GeV/c. The data points are fitted using four different Monte Carlo T T templates:coherentJ/y production(dashed-blue),incoherentJ/y production(dotted-red),J/y sfrom y ′ decay (dash-dotted - violet), and gg m +m − (dash-dotted - green). The solid histogram (black) → is the sum. The fitting function shapes were provided by STARLIGHT events [9] folded with realistic simulations. case, the target nucleus normally breaks up, but except from singlenucleons or nuclear fragments in the very forward region no other particles are produced. In both cases the J/y p is very low; the expected average transverse momentumis about 60 MeV/c and T 500 MeV/c for coherent and incoherent photoproduction, respectively. Figure 1 shows the dimuon p distributionintegrated over2.8 < M < 3.4 GeV/c2. The clear peak at T inv low p is due to coherent interactions, while the tail extending out to 0.8 GeV/c comes T from incoherent production. Taking also into account the finite detector resolution, dimuons where required to have p < 0.3 GeV/c, resulting in 117 J/y candidates. By T performing a fit to the corresponding dimuon invariant mass spectrum, the extracted number of J/y is N = 96 12 (stat) 6 (syst). To perform the fit, a maximum yield ± ± likelihood method on the set of events satisfying the selections described was used, consideringa Crystal Ball function to describe thesignal and an exponentialto account for the underlying continuum. The exponential slope parameter of the gg continuum is -1.4 0.2GeV 1c2 ingoodagreementwiththecorrespondingMonteCarloexpectation − (-1.3±9 0.01 GeV 1c2). This indicates the absence of hadronic background in the − ± kinematicregionsconsidered.Theestimatedfeed-down contributionfrom the y ′ decay is11 6%fordimuon p <0.3GeV/c,whilethecorrespondingincoherentcontribution T is12±+14%. 4 The−QED continuumpairproduction was used fornormalisationpurposes. Although in principle it can be calculated with high accuracy, the fact that the photon coupling to the nuclei is Z√a (with Z =82 here) rather than just √a increases the uncertainty from higher order terms. There is also an uncertainty associated with the minimum momentum transfer and the nuclear form factor. For these reasons, the uncertainty in the STARLIGHT two-photon cross section was estimated to be 20% [1]. The other sourcesof systematicerrors aregivenin [1]. Thedifferentialcoherent J/y cross section isds coh/dy=1.00 0.16(stat)+0.24(syst) mb. J/y ± 0.26 Figure2showsthecompariso−nbetweenthemeasuredcrosssectionandvariousmod- els that calculate the photon spectrum in impact parameter space in order to exclude interactions where the nuclei interact hadronically. They differ mainly by the way in which the photonuclear interaction is treated. They can be grouped into three different categories: i) those that include no nuclear effects (AB-MSTW08) [10]. Here all nu- cleons contribute to the scattering, and the forward scattering differential cross section scales with the number of nucleons squared; ii) those that use a Glauber approach to calculate the number of nucleons contributing to the scattering (STARLIGHT [9, 11], GM[12]andCSS[13]);andthosefrompartonicmodels,wherethecrosssectionispro- portional to the nuclear gluon distribution squared (AB-EPS08 [12], AB-EPS09 [12], AB-HKN07 [12] and RSZ-LTA [14]). As expected, the sensitivity to shadowing at for- ward rapidities is reduced compared to that at mid-rapidity. At forward rapidities there is a two-fold ambiguity in the photon energy and the momentum transfer from the nu- cleusactingasaphotontarget.TheAB-MSTW08andSTARLIGHTpredictionsdeviate by about three standard deviations, if the statistical and systematic errors are added in quadrature.TheRSZ-LTA,AB-EPS08 andAB-EPS09 modelsshowthebestagreement to data within one standard deviation. In addition, Figure 3 shows the ratio of the cross sections in two rapidity intervals, R = s ( 3.1 < y < 2.6)/s ( 3.6 < y < 3.1) = − − − − 1.36 0.36(stat) 0.19 (syst). Here, only AB-MSTW08 and AB-HKN07 deviate by ± ± more than one standard deviation. Taken together, these results indicate that the AB- MSTW08 model is strongly disfavoured, while the predicted STARLIGHT cross sec- tion deviates by nearly three standard deviations. Best agreement is found with models that include nuclear gluon shadowing, in agreement with EPS08 or EPS09 parameter- isations [15]. The findings of this first UPC study also suggest that in the future other heavierparticles likethe ¡ (1S) oreven the Higgs bosoncould bemeasured when using theLHCas a“photoncollider". SUMMARY In summary, ALICE has provided the first LHC measurement on exclusive J/y photo- productioninPb-Pbcollisionsat√s =2.76TeV.Theresultsofthisstudyindicatethat NN theoreticalmodelsonJ/y inUPCthatincludestrongmodificationstothenucleargluon density are favoured. A future study investigating coherent vector meson photoproduc- tionat central rapiditieswouldbeveryinterestingforunderstandingtheseeffects. ACKNOWLEDGMENTS I would like to thank the organisers of Diffraction 2012 for the opportunity to speak on thisnovelLHCmeasurementcarried out bytheALICE collaboration. Pb+Pb fi Pb+Pb+J/y s = 2.76 TeV NN b] m 7 AB-MSTW08 ALICE a) y [ CSS /d 6 SATBA-HRKLNIG0H7T sd GM 5 AB-EPS09 RSZ-LTA AB-EPS08 4 3 2 1 0 -4 -2 0 2 4 y FIGURE2. MeasuredcoherentdifferentialcrosssectionofJ/y photoproductioninultra-peripheralPb- Pbcollisionsat√sNN=2.76TeV.Theerroristhequadraticsumofthestatisticalandsystematicerrors. Thetheoreticalcalculationsdescribedinthetextarealsoshown.Therapiditydistributionsareshown. Pb+Pb fi Pb+Pb+J/y s = 2.76 TeV NN c) ALICE AB-MSTW08 STARLIGHT GM CSS RSZ-LTA AB-EPS08 AB-EPS09 AB-HKN07 1 1.5 2 2.5 3 ds /dy (-3.1 < y < -2.6) / ds /dy (-3.6 < y < -3.1) FIGURE3. Ratioofthecrosssectionsintherapidityintervals-3.1<y<-2.6and-3.6<y<-3.1.The dashedlinesinthelowertwoplotsindicatethethreemodelcategoriesdiscussedinthetext. REFERENCES 1. B.Abelevetal.[ALICECollaboration],arXiv:1209.3715[nucl-ex]. 2. C.A.Bertulani,S.R.KleinandJ.Nystrand,Ann.Rev.Nucl.Part.Sci.55(2005)271. 3. A.J.Baltzetal.Phys.Rept.458(2008)1. 4. M.G.Ryskin,Z.Phys.C57(1993)89. 5. A.D.Martin,C.Nockles,M.G.RyskinandT.Teubner,Phys.Lett.B662(2008)252. 6. S.Afanasievetal.[PHENIXCollaboration],Phys.Lett.B679(2009)321. 7. K.Aamodtetal.[ALICECollaboration],JINST3(2008)S08002. 8. K.Aamodtetal.[ALICECollaboration],Phys.Lett.B704(2011)442. 9. STARLIGHTwebsite,http://starlight.hepforge.org/. 10. A.AdeluyiandC.A.Bertulani,Phys.Rev.C85(2012)044904. 11. S.R.KleinandJ.Nystrand,Phys.Rev.C60,(1999)014903. 12. V.P.GoncalvesandM.V.T.Machado,Phys.Rev.C84(2011)011902. 13. A.Cisek,W.SchäferandA.Szczurek,Phys.Rev.C86(2012)014905. 14. V.Rebyakova,M.StrikmanandM.Zhalov,Phys.Lett.B710(2012)647. 15. K.J.Eskola,H.PaukkunenandC.A.Salgado,JHEP0904(2009)065.

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