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Physics Letters B

www.elsevier.com/locate/physletb

Coherent J photoproduction at forward rapidity in ultra-peripheral Pb–Pb collisions at √

s NN = 5 . 02 TeV

.ALICE Collaboration

a r t i c l e i n f o a b s t ra c t

Articlehistory:

Received19April2019

Receivedinrevisedform15August2019 Accepted6September2019

Availableonline10September2019 Editor:M.Doser

TheALICEcollaborationperformedthefirstrapidity-differentialmeasurementofcoherentJ photopro- ductioninultra-peripheralPb–Pb collisions atacenter-of-massenergy√s

NN = 5.02 TeV.TheJ is detectedviaitsdimuondecayintheforward rapidityregion(−4.0<y<2.5) foreventswherethe hadronicactivityisrequiredtobeminimal.Theanalysisisbasedonaneventsamplecorrespondingto anintegratedluminosityofabout750 μb1.ThecrosssectionforcoherentJ productionispresented insixrapiditybins.TheresultsarecomparedwiththeoreticalmodelsforcoherentJphotoproduction.

Thesecomparisonsindicatethatgluonshadowingeffectsplayaroleinthephotoproductionprocess.The ratio ofψ to J coherentphotoproduction crosssections was measuredandfound tobeconsistent withthatmeasuredforphotoproductionoffprotons.

©2019TheAuthor.PublishedbyElsevierB.V.ThisisanopenaccessarticleundertheCCBYlicense (http://creativecommons.org/licenses/by/4.0/).FundedbySCOAP3.

1. Introduction

Ultra-peripheral collisions (UPC) between two Pb nuclei, in whichtheimpactparameterislargerthan thesumoftheir radii, providea usefulwaytostudyphotonuclear reactions [1–4].Pho- toproduction of vector mesons in these collisions has an easily identifiableexperimentalsignature:thedecayproductsofthevec- tormeson,inthecaseofthisanalysisa

μ

+

μ

pair,aretheonly signalsinanotherwiseemptydetector.Thisprocessisakintoex- clusivevector mesonproductioninelectron–proton collisions,al- readystudiedextensivelyatHERA [5].Theexchangephoton,which carriesamomentumtransfersquaredQ2,istypifiedbyverysmall valuesofQ2,andmaybedescribedasquasi-real.Theintensityof thephotonfluxscalesasthesquareofnuclearchargeresultingin large crosssections forthe photoproduction ofvector mesons in Pb–Pb collisionsat theCERN LargeHadron Collider(LHC),where themeasurementpresentedinthisLetterwasperformed.

Photoproductionof vectormesons onnucleican beeither co- herent, where the photon couples coherently to the nucleus as a whole, or incoherent, where the photon couples to a single nucleon [2]. Coherent production is characterized by low vector mesontransverse momentum (pT60 MeV/c) and by thetar- getnucleusnotbreakingup.Incoherentproduction,corresponding to quasi-elastic scattering off a single nucleon, is characterized byasomewhathigheraveragetransversemomentum(pT500 MeV/c). The target nucleusnormallybreaks up inthe incoherent production,but, except for single nucleons or nuclear fragments

E-mailaddress:alice-publications@cern.ch.

in the very forwardregion, no other particles are produced. The incoherentproduction canbe accompanied by theexcitation and dissociationof the target nucleonresulting ineven higher trans- verse momenta of the produced vector mesons, extending well above1 GeV/c [6].

Coherent photoproduction of the J meson, a charm-anti- charm bound state, is of particular interest since, for a leading order QCD calculation [7], its cross section is expected to scale as the square of the gluon parton density function (PDF) in the target hadron. The mass of the charm quark provides an energy scalelargeenough toallowforperturbativeQCD calculations.For thisprocess,a variablecorrespondingtoBjorken-xcanbedefined using the mass of the vector meson (mJ) and its rapidity (y) asx=(mJ/ψ/

sNN)exp(±y).Thoughnext-to-leadingordereffects andscale uncertainties complicate extractionof gluon PDFsfrom J photoproduction data [8], the related uncertainties are ex- pected tolargely cancelin theratioof coherentphotoproduction cross sections off nucleiand off protons [9]. Thus, coherent J photoproduction off lead nuclei (

γ

+Pb→J+Pb) provides a powerful tool to studypoorly known gluon shadowing effects at low Bjorken-x valuesranging from x105 to x102 at LHC energies [10,11].

The ALICE collaboration has pioneered the study of charmo- nium photoproduction in ultra-peripheral Pb–Pb collisionsat the LHCatacenter-of-massenergypernucleonpair√

sNN = 2.76 TeV [12–14]. Coherent J photoproduction was studied both at for- wardrapidity (−3.6<y<2.6) withtheALICEmuonspectrom- eter and at mid-rapidity (|y|<0.9) with the central barrel. The CMS collaboration studied coherent J photoproduction accom- https://doi.org/10.1016/j.physletb.2019.134926

0370-2693/©2019TheAuthor.PublishedbyElsevierB.V.ThisisanopenaccessarticleundertheCCBYlicense(http://creativecommons.org/licenses/by/4.0/).Fundedby SCOAP3.

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panied by neutron emission in the semi-forward rapidity range 1.8<|y|<2.3 [15]. The ALICE and CMS results on J photo- productionwerecomparedwithpredictionsfrommodelsavailable atthat time, andsuggested that moderateshadowing inthe nu- cleus was necessary to describe themeasurements. In particular, thenucleargluonshadowingfactorRg,i.e.theratioofthenuclear gluondensitydistributiontotheprotongluondistribution,wasex- tracted from the ALICE measurements [10], and found to be, at thescaleofthecharmquark mass, Rg(x103)=0.61+00..0504 and Rg(x102)=0.74+00..1112.The ALICEcollaboration also measured thecoherentcrosssectionforψphotoproductionatmid-rapidity, andtheresults supported, within theexperimental uncertainties, themoderate-shadowingscenario [14].

InthisLetter, we presentthefirst measurementof thecoher- entJ photoproduction inultra-peripheral Pb–Pb collisionsata center-of-mass energyper nucleon pair √

sNN = 5.02 TeV. The measurement was performedwiththe ALICEmuon spectrometer coveringtherapidityrange−4.0<y<2.5.Theresultspresented herearebasedon datatakenin2015andin2018, duringRun 2 of the LHC. The recorded data sample is some 200 times larger thanthedatausedinthe √

sNN = 2.76 TeVPb–Pb analysis [12].

Thenewresultisbasedontheabsoluteluminosity normalization incontrast toprevious measurement based onthe normalization relative to the continuum

γ γ

μ

+

μ

cross section predicted by STARlight [16]. Thesetwo improvements implya considerable reduction in the statistical and systematic uncertainties and the possibilitytostudytherapiditydependenceintheforwardregion.

2. Detectordescription

The ALICE detector and its performance are described in [17,18]. Muonsfrom J decays are measured in the single-arm muonspectrometer,whileotheractivityisvetoedusingtheSilicon Pixel Detector (SPD), the V0 and ALICE Diffractive (AD) detec- tors. The muon spectrometer covers the pseudorapidity interval

4.0<

η

<2.5.It consistsof a teninteraction length absorber followed by five tracking stations, the third of which is placed inside a dipole magnet with a 3 T·m integrated magnetic field, a 7.2 interaction length iron wall, and a trigger system located downstreamoftheironwall.Eachtrackingstationismadeoftwo planesofcathodepadchambers,whilethetriggersystemconsists offourplanesofresistiveplatechambersarrangedintwostations.

Muon tracks are reconstructed using the tracking algorithm de- scribedin [19].Thecentralregion|

η

|<1.4iscoveredbytheSPD consisting of two cylindrical layers of silicon pixel sensors. The V0detectoriscomposed ofthe V0AandV0Csub-detectors, con- sisting of 32 cells each andcovering the pseudorapidity interval 2.8<

η

<5.1 and −3.7<

η

<1.7, respectively. The newly in- stalledADdetectoriscomposedoftheADCandADAsub-detectors locatedat−19.5 and+16.9 mfromtheinteractionpointcovering thepseudorapidityranges−7.0<

η

<4.9 and 4.7<

η

<6.3,re- spectively [20].TheV0andADdetectorsarescintillatortilearrays withatimeresolutionbetterthan1ns,allowingonetodistinguish betweenbeam-beamandbeam-gasinteractions.

3. Dataanalysis

Theanalysispresentedinthispublicationisbasedonasample ofevents collected during the 2015and 2018Pb–Pb data taking periodsat√

sNN = 5.02 TeV,characterizedbysimilarbeamcon- ditionsandinteractionrates.Themuonspectrometerperformance wasstableduringthewholeRun 2thusallowingforthemerging ofthetwo datasets.Thetrigger requiredtwooppositely charged tracks in the muon spectrometer, and vetoes on V0A, ADA and ADC beam-beam interactions. The single muon trigger threshold

was set to a transversemomentum pT=1 GeV/c [21]. The inte- grated luminosities of 216 μb1 in2015 and538 μb1 in2018, with relative systematic uncertainty of 5%, were estimated from the counts of a reference trigger, based on multiplicity selection intheV0detector.Thereferencetriggercrosssectionwasderived from Glauber-model-based estimatesof the inelastic Pb–Pb cross section [22].

Events with only two tracks with opposite electric charge (unlike-sign)inthemuon spectrometerwereselected offline.The pseudorapidity ofeachtrackwas requiredto bewithin therange

4.0<

η

<2.5. The tracks hadto fulfill the requirements,de- scribedin [12],ontheradialcoordinateofthetrackattheendof theabsorberandontheextrapolationtothenominalvertex.Track segmentsinthetrackingchambershadtobematchedwithcorre- spondingsegmentsinthetriggerchambers.

Additional offline vetoes on the V0A, ADA and ADC detector signals were applied to ensure the exclusive production of the muon pair. Exclusivity in the muon spectrometer region was as- suredbyrequiringamaximumof2firedcellsinV0C.Onlineand offline veto requirements may result in significant inefficiencies (denoted as veto inefficiencies) in the exclusive J cross sec- tion measurementsduetoadditional V0andAD detectoractivity induced byindependenthadronicorelectromagneticpile–uppro- cessesaccompanyingthecoherentJphotoproduction.Theprob- abilityofhadronicpile–updidnotexceed0.2%,howevertherewas a significant pile–up contribution fromthe electromagnetic elec- tron pair production process

γ γ

e+e. The veto inefficiency induced by thesepile–up effectsin the V0A,V0C, ADA andADC detectors, was estimated using the events selected with an un- biased trigger based only on the timing of bunches crossing the interaction region. The veto rejection probability, defined as the probability todetect activityinthesesub-detectors, wasfound to scale linearlywith the expected number of collisions per bunch crossingreaching10%inV0A.Thevetoinefficiencycorrectionfac- tors were determinedby weightingthe correspondingvetorejec- tion probabilities over periods with different pile–up conditions, taking the luminosity of each period as a weight. The veto in- efficiency of the V0A online and offline selection was found to be pV0A=(4.0.2)%, where the uncertainty is related to the limited statistics in the unbiased trigger sample. The veto ineffi- ciencies in ADA (pADA) and ADC(pADC) were found to be about 0.2%, because these detectors are far away from the interaction pointandarethusmuchlessaffectedbysofte+e pairs.Theveto inefficiency inV0C,associatedwiththerequirementofmaximum 2 fired cells, was found to be negligible. The average veto effi- ciency correction factor

veto=95.0%, and thisis applied to raw J yields to account for hadronic and electromagnetic pile–up processes,wascalculatedasaproductofindividualvetoinefficien- cies veto=(1−pV0A)(1−pADA)(1−pADC).

The acceptance and efficiency of J and ψ reconstruction were evaluated using a large sample of coherent andincoherent J andψ events generated by STARlight2.2.0 [23] withdecay muonstrackedinamodeloftheapparatusimplementedinGEANT 3.21 [24]. Themodelincludesarealistic descriptionofthedetec- tor performance during datataking as well as its variation with time.Theacceptanceandefficiencyoffeed-downψJ+

π π

decays were also evaluated using the STARlight generator under theassumptionthatfeed-downJ mesonsinheritthetransverse polarizationoftheirψparents,asindicatedbypreviousmeasure- ments [25]. The same samples were also used for modeling the signalshapeanddifferentbackgroundcontributions.

A sample enriched in coherent candidates was obtained by selecting dimuons with transverse momentum pT<0.25 GeV/c.

The invariant mass distributions for selected unlike-sign muon pairs are shown in Fig. 1, left, in the full dimuon rapidity range

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Fig. 1.Left:invariant massdistributionformuonpairssatisfyingtheeventselectiondescribedinthetext.Thedashedgreenlinecorrespondstothebackground.Thesolid magentaandredlinescorrespondtoCrystalBallfunctionsrepresentingJandψsignals,respectively.Thesolidbluelinecorrespondstothesumofbackgroundandsignal functions.Right:transversemomentumdistributionformuonpairsintherange2.85<mμμ<3.35 GeV/c2(aroundtheJmass).

4.0<y<2.5 and inFig. 2 insixrapidity subranges. The in- variantmassdistributionsare fittedwithafunctionmodelingthe backgroundandtwoCrystalBallfunctions [26] fortheJandthe ψpeaks.Theshapeofthebackgroundatlargeinvariantmassesis welldescribed by an exponentialdistribution, asexpectedifitis dominatedby theprocess

γ γ

μ

+

μ

.However, atmassesbe- low theJ,the distribution isstrongly influencedby the muon trigger condition. In order to model this, the whole background distribution is fitted using a template made from reconstructed STARlighteventscorresponding tothe

γ γ

μ

+

μ

process. The resultsofthefitareparametrizedusingafourth-orderpolynomial, whichturns smoothly into an exponential tailasfrom 4 GeV/c2. Thecoefficientsofthepolynomialarethenkeptfixedinthefitto theexperimentaldata,whiletheslopeoftheexponentialtermand thenormalizationare left free.The fittedslope isfound toagree within 2.5standard deviations withthe value obtained fromthe generatedsample.

TherawinclusiveJ andψyields, N(J/ψ)andN(ψ),were obtained by fitting the dimuon invariant mass spectrum in the range 2.2<mμμ<6 GeV/c2. The slope parameters in the Crys- tal Ball functions were fixed from fits to the respective Monte Carlo sets. The width parameter

σ

J was left free for the J, andwas fixed to

σ

ψ=

σ

J·(

σ

ψMC /

σ

JMC) for the ψ, where the ratio

σ

ψMC /

σ

JMC1.09 of theψ totheJ widths wasobtained fromthefitstocorrespondingMonteCarlosets.Themassparame- teroftheCrystalBallfunctionwasleftunconstrainedfortheJ. Duetothe smallψ statistics,the ψ mass wasfixed sothat the differencewithrespecttotheJ massisthesameasquoted by thePDG [27]. The J massmJ=3.0993±0.0009 GeV/c2, ob- tainedfromthefit inthefull rapidity range−4.0<y<2.5,is inagreementwiththePDGvaluewithin3standarddeviations.

TherawinclusiveJ yields obtainedfrominvariant massfits containcontributionsfromthecoherentandincoherentJ pho- toproduction,whichcanbeseparatedintheanalysisoftransverse momentumspectra.The pT distributionsfordimuonsintherange 2.85<mμμ<3.35 GeV/c2 are shownin Fig. 1,right, in the full dimuon rapidity range −4.0< y<2.5 and in Fig. 3 in sixra- piditysubranges.ThesedistributionswerefittedwithMonteCarlo templates produced using STARlight, corresponding to different productionmechanisms:coherentJ,incoherentJ,feed-down J fromcoherentψ decays,feed-downJ fromincoherentψ decaysandcontinuumdimuonsfromthe

γ γ

μ

+

μ

process.In

order to describe the high-pT tail, the incoherentJ photopro- ductionaccompanied bynucleon dissociationwasalso takeninto accountinthefitswiththetemplatebasedontheH1parametriza- tionofthedissociativeJ photoproduction [28] (denotedasdis- sociativeJ inthefollowing):

dN dpT

pT

1

+

bpd

npd

p2T

npd

.

(1)

The H1 collaboration provided two sets of measurements corre- spondingtodifferentphoton–protoncenter-of-massenergyranges:

25 GeV<Wγp <80 GeV (low-energy data set) and 40 GeV<

p<110 GeV (high-energy dataset). The fit parametersbpd= 1.79±0.12(GeV/c)2andnpd=3.58±0.15 fromthehigh-energy data set were used by default, while the corresponding uncer- taintiesandthelow-energyvaluesbpd=1.0.2(GeV/c)2 and npd=3.58(fixed)wereusedforsystematicchecks.

The templates were fitted to the data leaving the normaliza- tion free for coherent J, incoherent J and dissociative J production.Thenormalizationofthe

γ γ

μ

+

μ

spectrumwas fixed to the one obtainedfrom the invariant mass fits. The nor- malization of the coherent and incoherent feed-down J tem- plates was constrained to thenormalization ofprimary coherent and incoherent J templates, according to the feed-down frac- tions extractedfrom the measurement ofraw inclusive J and ψ yields,asdescribed below.The extractedincoherentJ frac- tion fI= NN(incoh J(coh J/ψ )/ψ ) forpT<0.25 GeV/c rangesfrom(4.0.6)% to (6.0.8)% depending on the rapidity interval andis consis- tent withbeingconstant within theuncertainties ofthe fits.The contributionofincoherentJ withnucleondissociationwas also takenintoaccountinthisfraction.

4. Resultsanddiscussion

4.1. RatioofcoherentψandJ/ψcrosssections

Theobtaineddimuoninvariantmassspectracanbeusedtoex- tract theratio of coherent ψ andJ cross sections R=σσ(J/ψ )) andthefractionoffeed-downJ fromψdecaysintherawJ yields.Thefitstotheinvariantmassdistributionsfordimuonswith pair pT<0.25 GeV/c in thefull rapidity range−4.0<y<2.5 resultinthefollowingratioofthemeasuredrawinclusiveψand Jyields:

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Fig. 2.Invariant mass distributions in six rapidity bins for muon pairs satisfying the event selection described in the text.

RN

=

N

)

N

(

J

/ψ ) =

0

.

0250

±

0

.

0030

(

stat

.),

(2) The rawψ and J yields in thisratiocontain contributions both fromcoherentandincoherent ψ and J photoproduction.

However, according to the dimuon pT fits, the fraction fI of in- coherentJ inthe rawJ yields doesnot exceed 6% and, ac- cordingtoSTARlight [23] andcalculationswithinthecolordipole approach [29],thefractionofincoherentψintherawψyieldsis expectedtobesimilar.TheRN ratiocanthereforebeconsideredas agoodestimate oftheratioofcoherentJ andψ yields,since theincoherentfractionsofψandJ yieldslargelycancelinthe

ratio. Besides, the raw J yields contain significant feed-down contributioncomingfromψJ+anything decays.Takinginto account thisfeed-downcontribution,one can expressthe RN ra- tiointermsofprimarycoherentψandJphotoproductioncross sections

σ

)and

σ

(J/ψ)integratedoveralltransversemomenta intherapidityrange−4.0<y<2.5:

RN

=

σ(J/ψ )B R(Jμμ)(J/ψ )σ+σ)B R)B Rμμ)J/ψ ))J/ψ )B R(Jμμ) (3)

(5)

Fig. 3.Transverse momentum distributions in six rapidity intervals for muon pairs satisfying the event selection described in the text.

where

(J/ψ)=12.0%,

)=15.8% and

J/ψ)=7.2%

are the efficiency corrections for primary coherent J, ψ and feed-downJ fromcoherentψdecaysestimatedwithSTARlight, whileB R(J

μμ

)=(5.961±0.033)%, B R(ψ

μμ

)=(0.80± 0.06)%, B R(ψJ+anything)=(61.0.6)% are the corre- spondingbranchingratios [27].Equation (3) canbeusedtoexpress theratio of primary coherent ψ andJ photoproductioncross sections,R,intermsofthemeasuredyieldratioRN:

R

=

B Rμμ)(ψ)RRNNB RB R(JμμJ/ψ ))(J/ψ )J/ψ )B R(Jμμ)

(4)

Substituting the measured RN value from Eq. (2) and the corre- spondingefficiencyvaluesandbranchingratios,onegets:

R

=

0

.

150

±

0

.

018

(

stat

.) ±

0

.

021

(

syst

.) ±

0

.

007

(

BR

),

(5) where the uncertainties on branching ratios B R(J

μμ

) and B R(ψ

μμ

)were addedinquadrature,whilethemainsources of systematic uncertainties are the variation of the fit range, of the signal andbackground shapes, andofthe dimuon transverse momentumcut.

The measured ratio ofthe ψ and J cross sectionsis com- patiblewiththeexclusivephotoproductioncrosssectionratio R= 0.166±0.007(stat.)±0.008(syst.)±0.007(BR) measured by the

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Table 1

Jyields,efficiencies, fIand fDfractionsandcoherentJcrosssections.

Rapidity range NJ fD fI dσJcoh/dy(mb)

(−4.00,−2.50) 21747±190 0.120 0.055 0.055±0.001 2.549±0.022(stat.)+00..209237(syst.) (4.00,3.75) 974±36 0.051 0.055 0.064±0.008 1.615±0.060(stat.)+00..135147(syst.) (−3.75,−3.50) 3217±70 0.140 0.055 0.058±0.004 1.938±0.042(stat.)+00..166190(syst.) (−3.50,−3.25) 5769±98 0.204 0.055 0.060±0.003 2.377±0.040(stat.)+00..212229(syst.) (3.25,3.00) 6387±105 0.191 0.055 0.052±0.002 2.831±0.047(stat.)+00..253280(syst.) (−3.00,−2.75) 4229±85 0.119 0.055 0.049±0.003 3.018±0.061(stat.)+00..259294(syst.) (−2.75,−2.50) 1190±47 0.029 0.054 0.049±0.006 3.531±0.139(stat.)+00..294362(syst.)

H1collaborationinep collisions [30] andwiththeratio R0.19 measured by the LHCb collaboration in pp collisions [31]. The measured ratio also agrees with predictions based on the Lead- ing Twist Approximation [32] for Pb–Pb UPC ranging from 0.13 to 0.18 depending on the model parameters. The ψ-to-J co- herentcross section ratioisexpectedtohavea mild dependence onthecollisionenergyandvectormesonrapidity [32] (at mosta few percent). Therefore the measured ratio can be directly com- pared to the unexpectedly large ψ-to-J coherent cross sec- tion ratio 0.34+00..0807, measured by ALICE in the ψl+l and ψl+l

π

+

π

channels at central rapidity in Pb–Pb UPC at

sNN = 2.76 TeV [14].Theratioatcentral rapidityismorethan a factortwo larger butstill stays compatiblewithin 2.5standard deviationswiththe forwardrapiditymeasurement, owingmainly tothelargeuncertaintiesofthecentralrapiditymeasurementthat willbeimprovedbytheanalysisofthemuchlargerUPCdatasam- plecollectedwiththeALICEcentralbarrelinRun2.

ThemeasuredcrosssectionratioRwasusedtoextractthefrac- tionoffeed-downJfromψrelativetotheprimaryJyield:

fD

=

N

(

feed-down J

/ψ )

N

(

primary J

/ψ ) =

R

J

/ψ)

(

J

/ψ )

B R

J

/ψ )

(6) The fraction fD=8.5%±1.5% was obtained forthe full rapidity rangewithoutanypTcut,wherestatistical,systematicandbranch- ingratiouncertainties wereaddedinquadrature.Thefractionre- ducesto fD=5.5%±1.0% forpT<0.25 GeV/cbecausefeed-down J are characterized by wider transverse momentum distribu- tionscomparedtoprimaryJ.

4.2. CoherentJ/ψcrosssection

ThecoherentJdifferentialcrosssectionisgivenby:

d

σ

Jcoh

dy

=

N

(

J

/ψ)

(

1

+

fI

+

fD

) (

J

/ψ)

BR

(

J

μμ )

vetoLint y (7) TherawJyieldvalues,efficiencies, fI and fD fractionsandco- herent J cross sectionswithrelevantstatistical andsystematic uncertainties are summarized in Table 1. The associated system- aticuncertaintiesarebrieflydescribedinthefollowing.

Thefirstsourceofsystematicuncertaintyisrelatedtothesep- arationofperipheral andultra-peripheral collisions.Coherent-like J photoproduction, observed in peripheral collisions of heavy ions [33],maycontributeafew percenttotherawJ yields in casehadronicactivityisnotdetectedbytheV0andADdetectors.

In order to reduce a possible contamination from J produced inperipheral hadronicevents, theanalysiswas repeatedwithan additionalrequirementthattherebenotrackletsdetectedatmid- rapidity in theSPD (where a trackletis a segment formedby at leastonehitineachofthetwodetectorlayers),resultingin12.6%

to 15.0% lower J yields depending on the rapidity range. The vetoinefficiency associated withthis additionalSPD requirement

wasestimatedwithunbiasedtriggerssimilartowhatwasdonefor the V0and AD vetoinefficiencies. The averagefraction ofevents withatleastoneSPDtrackletwasfoundtobe pSPD=9.0.2%.

TheyieldscorrectedfortheadditionalSPDvetoinefficiencyof9.4%

resultincrosssections3.6%to6.0%lowerthantheonesobtained without the SPD veto. This cross section difference is taken into accountinthesystematicuncertainty.

The systematic uncertainties on the efficiencies obtained by variationofthegeneratedrapidityshapesrangefrom0.1%to0.8%, depending on therapidity interval. The trackingefficiencyuncer- taintyof3%wasestimatedbycomparingthesingle-muontracking efficiencyvalues obtainedinMC anddata, witha procedure that exploitstheredundancyofthetracking-chamberinformation [34].

The systematic uncertainty on the dimuon trigger efficiency has two origins: the intrinsic efficiencies of the muon trigger cham- bersandtheresponse ofthetrigger algorithm.Thefirst onewas determined byvarying thetriggerchamberefficiencies intheMC byanamountequaltothestatisticaluncertaintyontheirmeasure- mentwithadata-drivenmethodandamountsto1.5%.Thesecond onewasestimatedbycomparingthetriggerresponsefunctionbe- tweendataandMC,resultinginefficiencydifferencesrangingfrom 5% to6%depending ontherapidityinterval.Finally,thereisa1%

contributionrelatedtothe precisionrequiredtomatchtrackseg- mentsreconstructedinthetrackingandtriggerchambers.

Severaltestswereperformedtoestimatetheuncertaintyonthe raw J signal extraction. These include the uncertainty on the JsignalshapeestimatedbyfittingtheCrystalBallslopeparam- eters instead of fixing them fromMonte-Carlo templates andby replacing the single-sided Crystal Ball witha double-sided Crys- talBallfunction.Thevariationofthecontinuumbackgroundshape duetothe uncertaintyonthetriggerresponse function,variation oftheinvariantmassintervalsby±0.1 GeV/c2 andofthedimuon pT selectionby±0.05 GeV/c werealsoconsidered.Thesystematic uncertaintyon therawJ yield, estimatedasrootmeansquare oftheresultsobtainedfromalltests,isabout2%withaslightra- piditydependence.

Severalsources ofsystematicuncertainties areassociatedwith different contributions to the pT spectrum: the fractionof feed- down J,theshape andcontributionofthe

γ γ

μ

+

μ

tem- plate, the shape for the coherent J andthe shape for the in- coherent J with nucleon dissociation. These contributions are shortly detailed in the following. First, the fraction fD of feed- downJwithpT below0.25GeV/c wasvariedintherangefrom 4.4to6.4%correspondingtothetotalsystematicuncertaintyofthe measured ψ-to-J crosssection ratio.Second, theshape ofthe

γ γ

μ

+

μ

pTtemplatefromSTARlightdoesnotincludepossi- blecontributions fromincoherentemission ofphotons,character- izedbymuchwidertransversemomentumdistributionsextending well above 1 GeV/c. In order to account for these contributions, the shape of the

γ γ

μ

+

μ

pT template was changed from STARlight to that obtained from the side-bands surrounding the J peakintheinvariant massspectra,resultingin1%systematic

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Source Value

Lumi. normalization ±5.0%

Branching ratio ±0.6%

SPD, V0 and AD veto from3.6% to6.0%

MC rapidity shape from±0.1% to±0.8%

Tracking ±3.0%

Trigger from±5.2% to±6.2%

Matching ±1.0%

Signal extraction ±2.0%

fDfraction ±0.7%

γ γyield ±1.2%

pTshape for coherent J ±0.1%

bpdparameter ±0.1%

Total from+89..32% to+810.9.3%

uncertaintyonthemeasured coherentcrosssection. Third,a0.2%

systematicuncertaintywasdeterminedviathevariationofthe

γ γ

contribution according to the statistical uncertainty in the back- groundtermcalculatedfromtheinvariantmassfits.Amodification ofthetransversemomentumspectraforthecoherentJ accord- ing to the model [35], results in a 0.1% systematic uncertainty.

Finally,the template shape for the incoherent J with nucleon dissociationwasvariedbyexchangingtheH1high-energyrunpa- rametersforthosedetermined fromthe low-energyrunresulting ina0.1%systematicuncertaintyonthecoherentcrosssection.

The systematic uncertainties are summarized in Table 2. The totalsystematicuncertaintyisthequadraticsumofallthesources listed in the table. Luminosity normalization, veto efficiencyand branchingratiouncertainties are fullycorrelated. Theuncertainty onthesignalextractionisconsideredasuncorrelatedasafunction ofrapidity.Finally,allother sourcesofuncertaintyare considered aspartiallycorrelatedacrossdifferentrapidityintervals.

4.3.Discussion

The measured differential cross section of coherent J pho- toproductionin the rapidity range −4.0<y<2.5 is shownin Fig. 4 and compared with various models. The covered rapidity range corresponds to a Bjorken-x of gluons either in the range 1.105<x<5.105or0.102<x<3.102 depending onwhich nucleusemitted the photon.According to models [32], the fraction of high Bjorken-x gluons(x∼102) is dominantat forwardrapiditiesandrangesfrom∼60% at y= −2.5 to∼95% at y= −4.

TheImpulseApproximation,takenfromSTARlight [16],isbased on the data from the exclusive J photoproduction off protons andneglects all nuclear effects except forcoherence. The square rootof theratioofexperimental pointsandthe ImpulseApprox- imation cross section is about 0.8, reflecting the magnitude of the nuclear gluon shadowing factor at typical Bjorken-x values around102,undertheassumptionthatthecontributionfromlow Bjorken-x∼105canbeneglected [10].

STARlightisbasedontheVectorMesonDominancemodeland aparametrizationoftheexistingdataonJ photoproductionoff protons [23].AGlauber-likeformalismisusedtocalculatetheJ photoproductioncross section inPb–Pb UPC accountingformul- tipleinteractionswithinthenucleusbutnot accountingforgluon shadowingcorrections.TheSTARlightmodeloverpredictsthedata, indicatingtheimportanceofgluonshadowingeffects,butthedis- crepancyismuchlowerthanfortheImpulseApproximation.

Guzey,KryshenandZhalov[32] providetwocalculations(GKZ), one based onthe EPS09 LOparametrization of theavailable nu- clear shadowing data [42] and the other on the Leading Twist

Fig. 4.MeasuredcoherentdifferentialcrosssectionofJphotoproductioninultra- peripheralPb–Pb collisionsat

sNN = 5.02 TeV.Theerrorbarsrepresentthesta- tisticaluncertainties,theboxesaroundthepointsthesystematicuncertainties.The theoreticalcalculations [10,16,23,32,36–41] describedinthetextarealsoshown.

ThegreenbandrepresentstheuncertaintiesoftheEPS09LOcalculation.

Approximation (LTA) of nuclear shadowing based on the combi- nationoftheGribov-GlaubertheoryandthediffractivePDFsfrom HERA [43].Both theLTAmodelandtheEPS09curve, correspond- ingtotheEPS09LOcentralset,underpredictthedatabutremain compatiblewithitatthemostforwardrapidities.Thedatatends tofollowtheupperlimitofuncertainties oftheEPS09calculation corresponding to the upper bound of uncertainties on the gluon shadowingfactorintheEPS09LOframework.

Severaltheoreticalgroupsprovidedpredictionswithinthecolor dipoleapproachcoupledtotheColorGlassCondensate(CGC)for- malismwithdifferentassumptionsonthedipole-protonscattering amplitude.PredictionsbyGonçalves,Machadoetal.(GM)basedon IIMand b-CGCmodels forthe scatteringamplitude underpredict thedata [36,37]. PredictionsbyLappi andMäntysaari(LM) based ontheIPsat model [38,39] givereasonable agreementthough the rangeofpredictionsdoesnotspanalltheexperimentalpoints.Re- cent predictions by Luszczak and Schafer (LS BGK-I) within the color-dipole formulation of the Glauber-Gribov theory [44] are in agreement with data at semi-forward rapidities, |y|<3, but slightlyunderpredictthedataatmoreforwardrapidities.

Cepila, Contreras and Krelina (CCK) provided two predic- tions based on the extension of the energy-dependent hot-spot model [40] tothenuclearcase:usingthestandardGlauber-Gribov formalism (GG-HS) and using geometric scaling (GS-HS) to ob- tain the nuclear saturation scale [41]. The GG-HS model agrees withdataatmostforwardrapiditiesbutunderpredictsitatsemi- forwardrapidities.The GS-HSmodel(notshown)strongly under- predictsthedata.

5. Conclusions

The first rapidity-differential measurement on the coherent photoproductionofJ inthe rapidityinterval−4<y<2.5 in ultra-peripheral Pb–Pb collisions at√

sNN = 5.02 TeV has been presentedandcomparedwithmodelcalculations.TheImpulseAp- proximationandSTARlightmodelsoverpredictthedata,indicating the importance of gluon shadowing effects. The model basedon thecentralsetoftheEPS09gluonshadowingparametrization, the LeadingTwist Approximation,andthehot-spotmodelcoupledto

(8)

the Glauber-Gribov formalism underpredict the data but remain compatiblewithitatmostforwardrapidities.Themajorityofcolor dipolemodelsunderpredictthedata.

The nucleargluon shadowing factorof about0.8at Bjorken-x values around 102 and a hard scale around the charm quark mass was estimated from the comparison of the measured co- herent J cross section withthe Impulse Approximation under theassumption that the contributionfromlow Bjorken x105 can be neglected. Future studies on coherent heavy vector me- sonphotoproduction accompaniedbyneutron emissionmayhelp to decouplelow-xandhigh-x contributions andprovidevaluable constraints on poorly known gluon shadowing effects at Bjorken x105 [45].

The ratio of the ψ and J cross sections is in reasonable agreement both withthe ratio ofphotoproduction cross sections offprotonsmeasuredbytheH1andLHCbcollaborationsandwith LTApredictionsforPb–Pb UPC.

Acknowledgements

The ALICE Collaboration would like to thank all its engineers andtechnicians fortheir invaluablecontributionstotheconstruc- tion of the experiment and the CERN accelerator teams for the outstanding performance of the LHC complex. The ALICECollab- oration gratefully acknowledges the resources and support pro- videdbyall GridcentresandtheWorldwide LHCComputingGrid (WLCG) collaboration. The ALICE Collaboration acknowledges the followingfundingagencies fortheirsupport inbuildingandrun- ningtheALICEdetector: A.I. AlikhanyanNationalScience Labora- tory(YerevanPhysicsInstitute)Foundation(ANSL),StateCommit- teeofScienceandWorldFederationofScientists(WFS),Armenia;

Austrian Academy of Sciences, Austrian Science Fund (FWF): [M 2467-N36] and Nationalstiftung für Forschung, Technologie und Entwicklung,Austria; MinistryofCommunicationsandHighTech- nologies, National Nuclear Research Center, Azerbaijan; Conselho NacionaldeDesenvolvimentoCientíficoeTecnológico(CNPq),Uni- versidadeFederal doRioGrande doSul(UFRGS), Financiadorade Estudos e Projetos (Finep) and Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP), Brazil; Ministry of Science &

Technology of China (MSTC), National Natural Science Founda- tionof China(NSFC) andMinistryof EducationofChina (MOEC), China; Croatian Science Foundation and Ministry of Science and Education, Croatia; Centro de Aplicaciones Tecnológicas y Desar- rolloNuclear(CEADEN),Cubaenergía,Cuba;MinistryofEducation, YouthandSportsoftheCzechRepublic,CzechRepublic;TheDan- ish Councilfor IndependentResearch NaturalSciences, theCarls- bergFoundationandDanishNationalResearchFoundation(DNRF), Denmark; Helsinki Institute of Physics (HIP), Finland; Commis- sariat à l’Energie Atomique (CEA), Institut National de Physique Nucléaire et de Physique des Particules (IN2P3) and Centre Na- tional de la Recherche Scientifique (CNRS) andRlégion des Pays de laLoire,France; Bundesministeriumfür Bildung,Wissenschaft, Forschung und Technologie (BMBF) and GSI Helmholtzzentrum fürSchwerionenforschungGmbH,Germany;GeneralSecretariatfor ResearchandTechnology,MinistryofEducation,ResearchandRe- ligions, Greece; National Research, Development and Innovation Office,Hungary;DepartmentofAtomicEnergy,GovernmentofIn- dia (DAE), Department of Science and Technology, Government ofIndia (DST), University Grants Commission,Government of In- dia(UGC)andCouncil ofScientific andIndustrialResearch(CSIR), India; Indonesian Institute ofScience, Indonesia;Centro Fermi – MuseoStoricodellaFisica e CentroStudi eRicercheEnrico Fermi andIstitutoNazionalediFisicaNucleare(INFN),Italy;Institutefor Innovative Science and Technology, Nagasaki Institute of Applied Science (IIST), Japan Society for the Promotion of Science (JSPS)

KAKENHIandJapaneseMinistryofEducation,Culture, Sports,Sci- enceand Technology (MEXT),Japan; Consejo Nacionalde Ciencia (CONACYT) y Tecnología, through Fondo de Cooperación Interna- cional enCiencia yTecnología(FONCICYT)andDirección General deAsuntosdelPersonalAcademico(DGAPA),Mexico;Nederlandse OrganisatievoorWetenschappelijkOnderzoek(NWO),Netherlands;

The ResearchCouncil ofNorway, Norway;CommissiononScience andTechnology forSustainable Developmentin theSouth (COM- SATS),Pakistan;PontificiaUniversidadCatólicadelPerú,Peru;Min- istry of Science andHigher Education and NationalScience Cen- tre, Poland; Korea Institute of Science and Technology Informa- tion and National Research Foundation of Korea (NRF), Republic of Korea; Ministry of Education andScientific Research,Institute of Atomic Physics and Ministry of Research and Innovation and Institute of Atomic Physics, Romania; Joint Institute for Nuclear Research(JINR), MinistryofEducationandScience oftheRussian Federation, National ResearchCentre KurchatovInstitute, Russian Science Foundation and Russian Foundation for Basic Research, Russia; Ministryof Education,Science, ResearchandSport ofthe Slovak Republic, Slovakia; NationalResearch Foundation of South Africa,SouthAfrica;SwedishResearchCouncil(VR)andKnut&Al- iceWallenbergFoundation(KAW),Sweden;EuropeanOrganization for Nuclear Research, Switzerland;National Science andTechnol- ogy Development Agency (NSDTA), Suranaree University of Tech- nology(SUT)andOfficeoftheHigherEducationCommissionunder NRU projectofThailand,Thailand;TurkishAtomicEnergy Agency (TAEK),Turkey;NationalAcademyofSciencesofUkraine,Ukraine;

ScienceandTechnologyFacilitiesCouncil(STFC),UnitedKingdom;

NationalScienceFoundationoftheUnitedStatesofAmerica(NSF) andUnitedStatesDepartmentofEnergy,OfficeofNuclear Physics (DOENP),UnitedStatesofAmerica.

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Referanser

RELATERTE DOKUMENTER

Ministry of Science and Education and Croatian Science Founda- tion, Croatia; Centro de Aplicaciones Tecnológicas y Desarrollo Nu- clear (CEADEN), Cubaenergía, Cuba;

Ministry of Science &amp; Technology of China (MSTC), National Natu- ral Science Foundation of China (NSFC) and Ministry of Education of China (MOEC) , China; Ministry of

Ministry of Science &amp; Technology of China (MSTC), National Natu- ral Science Foundation of China (NSFC) and Ministry of Education of China (MOEC), China; Ministry of

Ministry of Science and Education and Croatian Science Founda- tion, Croatia; Centro de Aplicaciones Tecnológicas y Desarrollo Nu- clear (CEADEN), Cubaenergía, Cuba;

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Ministry of Science and Education and Croatian Science Founda- tion, Croatia; Centro de Aplicaciones Tecnológicas y Desarrollo Nu- clear (CEADEN), Cubaenergía, Cuba;

33 ( a ) Institute of High Energy Physics, Chinese Academy of Sciences, Beijing, China; ( b ) Department of Modern Physics, University of Science and Technology of China, Anhui,

University of Science and Technology of China Liu, Yang. MSRA, China