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Physics Letters B
www.elsevier.com/locate/physletb
Investigation of the p– 0 interaction via femtoscopy in pp collisions
.ALICE Collaboration
a r t i c l e i n f o a b s t ra c t
Articlehistory:
Received16November2019
Receivedinrevisedform27March2020 Accepted6April2020
Availableonline9April2020 Editor: B.Blank
ThisLetterpresentsthefirstdirectinvestigationofthep–0interaction,usingthefemtoscopytechnique inhigh-multiplicityppcollisionsat√
s=13 TeVmeasuredbytheALICEdetector.The0isreconstructed viathedecaychanneltoγ,andthe subsequentdecayoftopπ−.Thephotonisdetectedviathe conversioninmaterialtoe+e−pairsexploitingthecapabilityoftheALICEdetectortomeasureelectrons atlowtransversemomenta.Themeasuredp–0correlationindicatesashallowstronginteraction.The comparison of the data to several theoretical predictions obtained employingthe CorrelationAnalysis ToolusingtheSchrödingerEquation(CATS)andtheLednický–Lyuboshitsapproachshowsthatthecurrent experimental precisiondoes not yetallow todiscriminate betweendifferentmodels,as it isthe case forthe availablescattering andhypernucleidata.Nevertheless, thep–0correlation functionisfound tobe sensitivetothe stronginteraction,and drivenby theinterplayofthedifferentspinand isospin channels.Thispioneeringstudydemonstratesthefeasibilityofafemtoscopicmeasurementinthep–0 channelandwiththeexpectedlargerdatasamplesinLHCRun3andRun4,thep–0interactionwill beconstrainedwithhighprecision.
©2020EuropeanOrganizationforNuclearResearch.PublishedbyElsevierB.V.Thisisanopenaccess articleundertheCCBYlicense(http://creativecommons.org/licenses/by/4.0/).FundedbySCOAP3.
1. Introduction
Aquantitative understanding of thehyperon–nucleon interac- tioninthestrangeness S= −1 sectorisfundamentaltopindown the role of strangeness within low energy quantum chromody- namics and to study the properties of baryonic matter at finite densities.Thepossiblepresenceoftheisoscalarandtheisovec- tor(+,0,−)hyperonstatesintheinnercoreofneutronstars (NS) is currently under debate due to the limited knowledge of theinteraction of such hyperons with nuclear matter. The inclu- sion ofhyperons in the description ofthe nuclear matter inside NS typically contains only states, and the on-average attrac- tive nucleon– (N–) interaction leads to rather soft Equations ofState(EoS)forNS.Thesearethenunabletoprovidestabilityfor starsofabouttwosolarmasses [1,2].Thehyperonsarerarelyin- cludedintheEoSforNS becauseofthe limitedknowledge about theN–stronginteraction.
Indeed,whiletheattractiveN–interactionisreasonablywell constrained from the available scattering and light hypernuclei data [3–5], the nature of the N– interaction lacks conclusive experimental measurements. One of the major complications for experimentalstudies isthefactthat thedecayofall statesin- volves neutral decay products [6], thus requiring high-resolution calorimeters.
E-mailaddress:alice-publications@cern.ch.
The mainsource ofexperimental constraintsonthe N– sys- tem comes from scattering measurements [7–9], analysis of − atoms [10–12],andhypernucleiproductiondata [13–16],although the latter are mainly dominated by large statistical uncertain- tiesandlarge kaondecaybackground.Latest hypernuclearresults obtained from different nuclear targets point towards an attrac- tive interaction in the isospin I=1/2 channel of the N– sys- tem [13,14],andrepulsioninthe I=3/2 channel [15,16].Hyper- nuclearmeasurements,however,areperformedatnuclear satura- tiondensityandhenceinthepresenceofmorethanonenucleon, resultingin asubstantial modeldependenceintheinterpretation oftheexperimentaldata [17].
Additionally, the hyperon–nucleon dynamics are strongly af- fected by the conversion process N– ↔ N–,occurring in the I=1/2 channel due to the close kinematic threshold between the two systems (about 80 MeV) [18–22]. This coupling is ex- pectedtoprovideanadditionalattractivecontributioninthetwo- body N– interaction in vacuum [21,22]. Indeed, depending on thestrength oftheN–↔N– couplingatthetwo-bodylevel, the correspondingin-medium hyperonpropertiesare very differ- ent.Forastrongcoupling,thisleads toarepulsivesingle-particle potential U at large densities [21,22]. For the hyperon, the in-mediumpropertiesaremostlydeterminedbytheoverallrepul- sioninthe I=3/2 component [21,22]. Arepulsivecomponentin thehyperon–nucleoninteractionscouldshifttheonsetforhyperon productiontolargerdensities,above2–3timesthenormalsatura-
https://doi.org/10.1016/j.physletb.2020.135419
0370-2693/©2020EuropeanOrganizationforNuclearResearch.PublishedbyElsevierB.V.ThisisanopenaccessarticleundertheCCBYlicense (http://creativecommons.org/licenses/by/4.0/).FundedbySCOAP3.
tiondensity,thusleadingtostifferEoSwhichareabletodescribe theexperimentalconstraintofNS.
Tothisend,differenttheoreticalapproachesincludingchiralef- fectivefieldtheories(
χ
EFT) [20] andmeson-exchangemodelswith hadronic [23] and quark [24] degrees offreedom providea simi- lardescriptionoftheavailabledatabyassumingastrongrepulsion inthe spinsinglet S=0, I=1/2 andspin triplet S=1, I=3/2 andanoverallattractionintheremainingchannels.Recentabini- tio lattice calculations at quark physical masses show a similar dependenceon spin-isospin configurations for the central poten- tialterm [25]. The strength ofthe coupled-channel N–↔N–is strongly model dependent as well. Calculations based on chi- ral models [20,21] and meson-exchange models [18,26] predict a rather strong or much weaker coupling, respectively. A self- consistentdescriptionofthiscoupled-channeldemandsadetailed knowledgeofthestronginteractionintheN–system.
Recently, the study of two-particle correlations in momen- tum space measured in ultra-relativistic proton–proton (pp) and proton–nucleus collisions has proven to provide direct access to the interaction between particle pairs in vacuum [27–29]. The small size of the colliding systems of about 1 fm results in a pronouncedcorrelation signal fromstrong finalstate interactions, whichpermits thelatter to beprecisely constrained. These mea- surementsprovidedadditionaldatainthehyperonsectorwithan unprecedentedprecisioninthelowmomentumregime.InthisLet- ter,thesestudiesareextendedtothesector.Theelectromagnetic decayofthe0isexploitedforthefirstdirectmeasurementofthe p–0 interactioninppcollisions.Thisstudypavesthewayforex- tendingtheseinvestigationstothe charged states,inparticular inlightofthelargerdatasamplesexpectedfromtheLHCRuns3 and4.
2. Dataanalysis
ThisLetterpresentsresultsobtainedfromadatasampleofpp collisionsat√
s=13 TeVrecordedwiththeALICEdetector [30,31]
duringtheLHCRun2(2015–2018).Thesamplewascollectedem- ploying a high-multiplicity trigger with the V0 detectors, which consistoftwosmall-angleplasticscintillatorarrayslocatedonei- therside ofthecollision vertexatpseudorapidities2.8<
η
<5.1 and−3.7<η
<−1.7 [32].Thehigh-multiplicitytriggerisdefined bycoincidenthitsinbothV0detectorssynchronouswiththeLHC bunchcrossingandbyadditionallyrequiringthesumofthemea- sured signal amplitudes in the V0 to exceed a multiple of the averagevalueinminimumbiascollisions.Thiscorresponds,atthe analysis level, to the highest multiplicity interval containing the top0.17% ofallinelasticcollisions withatleastonechargedpar- ticlein |η
|<1 (referred to asINEL > 0). This data set presents asuitable environmenttostudycorrelationsduetotheenhanced production of strange particles in such collisions [33]. Addition- ally, the larger charged-particle multiplicity density withrespect tothe minimumbias sample significantly increasestheprobabil- ityto detect particle pairs. The V0 is alsoemployed to suppress backgroundevents,suchastheinteractionofbeamparticleswith mechanicalstructures ofthebeamline,orbeam-gas interactions.In-bunch pile-upevents withmore than one collision per bunch crossingarerejectedbyevaluatingthepresenceofadditionalevent vertices [31].Theremaining contaminationfrompile-upeventsis onthepercentlevelanddoesnotinfluencethefinalresults.
Charged-particletrackingwithintheALICEcentralbarreliscon- ducted with the Inner Tracking System (ITS) [30] and the Time Projection Chamber (TPC) [34]. The detectors are immersed in a homogeneous 0.5 Tsolenoidal magneticfield along thebeam di- rection.TheITSconsistsofsixcylindricallayers ofhighposition- resolutionsilicondetectorsplacedradiallybetween3.9 and43 cm aroundthebeampipe.Thetwoinnermostlayers areSiliconPixel
Detectors (SPD)andcoverthepseudorapidityrange|
η
|<2.0 and|
η
|<1.4,respectively. Thetwo intermediatelayers are composed ofSiliconDriftDetectors,andthetwooutermostlayers aremade ofdouble-sidedSiliconmicro-StripDetectors(SSD),covering|η
|<0.9 and |
η
|<1.0, respectively. The TPC consists of a 5 m long, cylindrical gaseous detector with full azimuthal coverage in the pseudorapidityrange|η
|<0.9.Particleidentification(PID)iscon- ductedviathemeasurementofthespecificionizationenergyloss (dE/dx)withup to159reconstructedspacepoints alongthepar- ticle trajectory. The Time-Of-Flight (TOF) [35] detector system is locatedataradialdistanceof3.7 mfromthenominalinteraction point andconsists ofMultigapResistive Plate Chambers covering thefullazimuthalanglein|η
|<0.9.PIDisaccomplishedbymea- suringtheparticle’svelocityβviathetimeofflightoftheparticles inconjunctionwiththeirtrajectory.Theeventcollisiontimeispro- videdasa combinationofthe measurementsin theTOF andthe T0 detector,two Cherenkovcounter arrays placed atforward ra- pidity [36].The primary eventvertex(PV)is reconstructedwiththecom- binedtrackinformationoftheITSandtheTPC,andindependently withSPDtracklets.Whenbothvertexreconstructionmethods are available, thedifference ofthecorresponding z coordinates isre- quired to be smallerthan 5 mm. Auniform detectorcoverage is assured byrestrictingthemaximaldeviationbetweenthe z coor- dinateof thereconstructedPV andthe nominalinteractionpoint to ±10 cm.Atotalof1.0×109 high-multiplicityeventsareused fortheanalysisaftereventselection.
The protoncandidates arereconstructedfollowingtheanalysis methods usedforminimumbiasppcollisions at√
s=7 TeV [27]
and 13 TeV [28,29], and are selected from the charged-particle tracks reconstructed with the TPC in the kinematic range 0.5<
pT<4.05 GeV/c and|
η
|<0.8. The TPCandTOF PIDcapabilities are employedtoselectprotoncandidatesby thedeviationnσ be- tween the signal hypothesis for a proton and the experimental measurement, normalized by the detector resolutionσ
.For can- didateswith p<0.75 GeV/c,PIDisperformedwiththeTPConly, requiring|nσ|<3.Forlargermomenta,thePIDinformationofTPC andTOF are combined.Secondary particles stemming fromweak decays or the interaction of primary particles with the detector materialcontaminatethesignal.Thecorrespondingfractionofpri- maryandsecondaryprotonsareextractedusingMonteCarlo(MC) templatefitstothemeasureddistributionoftheDistanceofClos- est Approach (DCA) of the track to theprimary vertex [27]. The MC templates are generated using PYTHIA 8.2 [37] and filtered throughtheALICEdetector [38] andreconstructionalgorithm [30].Theresultingpurityofprotonsisfoundtobe99%,withaprimary fractionof82%.
The 0 isreconstructedviathedecaychannel0→
γ
with a branching ratioof almost 100% [6]. The decay is characterized by a short life time rendering the decay products indistinguish- able fromprimary particles produced in theinitial collision. Due tothe smallmassdifference betweentheandthe0 ofabout 77 MeV/c2, theγ
has typically energies of only few hundreds of MeV. Therefore, it is reconstructed relying on conversions to e+e− pairs inthe detectormaterial ofthe centralbarrel exploit- ing the unique capability of the ALICE detector to identify elec- trons downto transverse momentaof 0.05 GeV/c. Fortransverse radii R<180 cmand|η
|<0.9 thematerial budget corresponds to (11.4±0.5)% of a radiation length X0, and accordingly to a conversion probability of (8.6±0.4)% [39]. Details ofthe photon conversionanalysisandthecorrespondingselectioncriteriaarede- scribed in [39,40]. The reconstruction relieson the identification of secondary vertices by forming so-called V0 decay candidates from two oppositely-charged tracks using a procedure described in detail in [41]. The products of the potentialγ
conversion are reconstructed with the TPC and the ITS in the kinematic rangeFig. 1.Invariantmassdistributionoftheγ andγ candidates,intwopTintervalsof1.5−2.0 GeV/cand6.5−7.0 GeV/c.ThesignalisdescribedbyasingleGaussian, andthebackgroundbyapolynomialofthirdorder.Thenumberof0candidatesisevaluatedwithinM0(pT)±3 MeV/c2.Onlystatisticaluncertaintiesareshown.
pT>0.05 GeV/c and|
η
|<0.9. Thecandidates forthe e+e− pair are identified by a broad PID selection in the TPC −6<nσ<7.The resulting
γ
candidate isobtained asthe combinationof the daughtertracks.OnlycandidateswithpT>0.02 GeV/c andwithin|
η
|<0.9 are accepted. Combinatorial background from primary e+e− pairs,orDalitzdecaysoftheπ
0 andη
mesonsis removed byrequiringthat theradialdistanceoftheconversionpoint,with respecttothedetectorcentre,rangesfrom5 cmto180 cm.Resid- ual contaminations from K0S and are removed by a selection in the Armenteros-Podolandski space [40,42]. Random combina- tionsofelectrons andpositrons are furthersuppressedbya two- dimensionalselectiononthe anglebetweentheplane definedby thee+e−pair,andthemagneticfield [43] incombinationwiththe reducedχ
2 ofa refitof thereconstructed V0 assuming that the particleoriginatesfromtheprimaryvertexandhasMV0=0 [40].The Cosine of the Pointing Angle (CPA) between the
γ
momen- tumand the vector pointingfrom the PVto the decay vertexis requiredtobeCPA>0.999.InadditiontothetightCPAselection, thecontributionofparticlesstemming fromout-of-bunchpile-up issuppressedbyrestrictingtheDCAofthephotontobealongthe beamdirection(DCAz<0.5 cm).Afterapplicationoftheselection criteria,about946×106γ
candidateswithapurityofabout95.4%areavailableforfurtherprocessing.
Theparticlecandidatesarereconstructedviathesubsequent decay→p
π
−withabranchingratioof63.9% [6],followingthe procedures described in [27,28]. For the the charge conjugate decayisexploited,andthesameselectioncriteriaareapplied.The decayproductsarereconstructedwiththeTPCandtheITSwithin|
η
|<0.9.ThedaughtercandidatesareidentifiedbyabroadPIDse- lectionintheTPC|nσ|<5.Theresultingcandidateisobtained asthecombinationofthedaughtertracks.Thecontributionoffake candidatesis reduced by requesting a minimum pT>0.3 GeV/c.ThecoarsePIDselectionofthedaughtertracksintroducesaresid- ualK0Scontaminationinthesampleofthecandidates.Thiscon- taminationisremovedbya 1.5
σ
rejectiononthe invariantmass assumingadecayintoπ
+π
−,whereσ
correspondsto thewidth ofaGaussianfittedtotheK0S signal.Topologicalselectionsfurther enhancethepurityofthesample.Theradialdistanceofthede- cayvertexwithrespecttothedetectorcentrerangesfrom0.2 cm to100 cmandCPA>0.999.InadditiontothetightCPAselection, particles stemming from out-of-bunch pile-up are rejectedusing thetiming informationoftheSPDandSSD,andtheTOFdetector.One ofthe two daughter tracks isrequired to have a hit in one ofthesedetectors.Afterapplicationoftheselectioncriteria,about
188×106 (178×106) () candidates with a purity of 94.6%
(95.3%)areavailableforfurtherprocessing.
The 0 (0) candidatesare obtainedby combiningall () and
γ
candidatesfromthesameevent,wherethenominalparticle masses [6] are assumedforthe daughters. Inparticular the tim- ingselectiononthedaughtertracksoftheassuresthatthe0 candidatesstemfromtherightbunchcrossing.Incaseadaughter trackisusedtoconstructtwoγ
,,andcandidates,oracombi- nationthereof,theone withthesmallerCPAisremovedfromthe sample.Inordertofurtheroptimizetheyieldandthepurityofthe sample,only0candidateswithpT>1 GeV/c areused.The resulting invariant mass spectrum is shown in Fig. 1 for two pT intervals. In order to obtain the raw yield, the signal is fitted with a single Gaussian, and the background with a third- orderpolynomial. Dueto thedeterioratingmomentum resolution for low pT tracks, the meanvalue ofthe Gaussian M0 exhibits a slight pT dependence, which is well reproduced in MC simu- lations. The 0 (0) candidates for femtoscopy are selected as M0(pT)±3 MeV/c2.Thewidthoftheintervalischosenasacom- promisebetweenthe candidatecountsandpurity.In total,about 115×103 (110×103) 0 (0) candidates arefound at a purity of about 34.6%. Due to the enhanced combinatorial background at low pT, the purity increases from about20% at the lower pT thresholdtoitssaturationvalueofabout60%above5 GeV/c.Only one candidateper eventisused,andisrandomly selectedinthe very rare casein which more than one is available. In lessthan one permille ofthecaseswhenthe trackofa primary protonis alsoemployed asthe daughtertrackofthe
γ
orthe ,thecor- responding0 candidateisrejected.Sinceonly stronglydecaying resonancesfeedtothe0 [6],allcandidatesareconsideredtobe primaryparticles.3. Analysisofthecorrelationfunction
The experimental definition of the two-particle correlation function,forbothp–p andp–0pairs,isgivenby [44],
C
(
k∗) =
N×
Nsame(
k∗)
Nmixed(
k∗)
k∗→∞
−−−−→
1,
(1)withthesame(Nsame)andmixed(Nmixed)eventdistributionsofk∗ anda normalizationconstant N.The relative momentumof the pairk∗ isdefinedask∗=12× |p∗1−p∗2|,wherep∗1 andp∗2 are the momenta ofthe twoparticles in thepair restframe, denotedby the∗.Thenormalizationisevaluatedink∗∈ [240,340]MeV/c for
p–p andink∗∈ [250,400] MeV/c forp–0 pairs,whereeffectsof finalstate interactionsare absentandhencethecorrelationfunc- tionapproachesunity.
The trajectories of the p–p and p–p pairs at low k∗ are al- mostcollinear,andmightthereforebeaffectedbydetectoreffects liketracksplittingandmerging [45].Accordingly, thereconstruc- tionefficiencyforpairsinthesameandmixedeventmightdiffer.
To this end, a close-pair rejection criterion is employed remov- ingp–p andp–p pairsfulfilling
η
2+ϕ
∗2<0.01,wherethe azimuthalcoordinateϕ
∗considersthetrackcurvatureinthemag- neticfield.A total number of 1.7×106 (1.3×106) p–p (p–p ) and 587 (539)p–0 (p–0) pairs contribute to the respective correlation functionin theregionk∗<200 MeV/c.Toenhancethe statistical significance of the results, the correlation functions of baryon–
baryon andantibaryon–antibaryonpairs are combined.Therefore, inthefollowingp–0denotesthecombinationp–0⊕p–0,and correspondinglyforp–p.
The systematic uncertainties of the experimental correlation functionareevaluatedbysimultaneouslyvaryingallproton,,
γ
, and0 single-particleselection criteriaby up to20% aroundthe nominalvalues.Onlyvariations thatmodifythepairyieldby less than10%(20%)forp–0 (p–p)withrespectto thedefaultchoice areconsidered, andthe 0 purityby lessthan 5%.Theimpact of statisticalfluctuationsisreducedbyevaluatingthesystematicun- certainties in intervalsof 100 MeV/c (20 MeV/c) in k∗ forp–0 (p–p). Theresulting systematicuncertainties are parametrizedby anexponentialfunctionandinterpolatedtoobtainthefinalpoint- by-pointuncertainties.Attherespectivelylowestk∗,thetotalsys- tematic uncertainties are of the order of 2.5% for both p–p and p–0.Using thefemtoscopy formalism [44], thecorrelation function can be relatedto the source function S(r∗) andthe two-particle wavefunction(r∗,k∗)incorporatingtheinteraction,
C
(
k∗) =
d3r∗S
(
r∗) | (
r∗,
k∗) |
2,
(2)where r∗ refers to the relative distance between the two parti- cles. As demonstrated in [27–29,46] the correlation function be- comes particularly sensitive to the strong interaction for small emissionsourcesformedinppandp–Pb collisions.Forthisstudy, asphericallysymmetricemittingsourceisassumed, withaGaus- sianshapedcoredensityprofileparametrizedbyaradiusr0,which isobtainedfromafittothep–p correlationfunction,similarlyas in [28,29].Followingthepremiseofacommonemissionsourcethe suchextractedradiusisthenusedasaninputtofitthep–0cor- relationfunction. Possiblemodifications ofthe sourceprofile due totheinfluenceofstronglydecayingresonances [47–49] arecon- sideredintheevaluationofthesystematicuncertaintiesassociated withthefittingprocedure.
The genuine p–p correlation function is modeled using the CorrelationAnalysisToolusingtheSchrödingerequation (CATS) [46], which allows one to useeither a localpotential V(r) or directly thetwo-particlewavefunction,andadditionallyanysourcedistri- bution asinput tocompute the correlation function.For thep–p correlation function thestrong Argonne v18 potential [50] inthe S,P,andDwavesisusedasaninputtoCATS.
The theoretical correlation function for p–0 is modeled em- ploying two different approaches. On the one hand, in CATSthe correlation function iscomputedfrom theisospin-averaged wave functions obtained within a coupled-channel formalism. On the other hand, the Lednický–Lyuboshits approach [51] relies on the effective-range expansion usingscatteringparameters asinput to evaluate the correlation function. The coupling ofthe n-+ sys- temto p–0 considering thedifferentthresholds isexplicitly in- cludedby meansofa coupled-channelapproach,whilethe effect
Table 1
Weightparametersfortheindividualcomponentsofthemeasuredcorrelationfunc- tion.Contributions fromfeed-downcontainthe motherparticle listedas asub- index.Non-flatcontributionsarelistedindividually.
p–p p–0
Pair λparameter
(%)
Pair λparameter
(%)
p–p 67.0 p–0 22.0
p–p 20.3 p–(γ) 73.1
Feed-down (flat) 11.6 Feed-down (flat) 4.7
Misidentification (flat) 1.1 Misidentification (flat) 0.2
ofthep–channelisincorporatedbycomplexscatteringparame- ters [52].Detailsoftheemployedmodelsaredescribedinthenext Section.
The experimental data are compared with the modeled cor- relation function considering the finite experimental momentum resolution [27].Inaddition tothe genuinecorrelation functionof interest, the measured correlation function also contains residual correlations due to protons coming from weak decays of other particles, such as and+ (feed-down), andmisidentifications.
Theseeffectsare includedbymodelingthetotalcorrelation func- tionasadecomposition,
Cmodel
(
k∗) =
1+
i
λ
i× (
Ci(
k∗) −
1),
(3)wherethesumrunsoverallcontributions.Theirrelativecontribu- tionisgivenbythe λparameterscomputedinadata-drivenway from single-particleproperties such asthepurity andfeed-down fractions [27],andaresummarizedinTable1.
Apart fromthegenuine p–p correlation function, a significant contribution comes fromthe decayof particles feeding to the protonpair.Theresidual p–correlationfunctionismodeledus- ing either the Usmani potential [53], chiral effective field the- ory calculations at Leading (LO) [54], or Next-To-Leading order (NLO) [20]. The resultingcorrelation function istransformed into themomentumbasisofthep–p pairby applyingthecorrespond- ingdecaymatrices [55].Allothercontributionsareassumedtobe C(k∗)∼1.Duetothechallengingreconstructionofthe0,theex- perimentalpurityofthe0 sampleisratherlow,andadditionally exhibitsastrongdependenceonthetransversemomentum pT as demonstratedinFig.1.Theaverage pT ofthe0 candidatesused to constructthecorrelation functionatk∗<200 MeV/c,however, is lowerthan thepTofall inclusive0 candidates.Considering this effect, the 0 purity employed to compute the λ parame- ters is found to be 27.4%. Accordingly, the main contribution to thep–0 correlationfunctionstemsfromthecombinatorialback- groundappearing in theinvariant massspectrum around the 0 peak, whichinthefollowingisreferred toas(
γ
).Theshapeof the p–(γ
) correlation function is extractedfrom the sidebands oftheinvariant massselection,andisfoundtobeindependentof the choice of mass window. The non-flat behavior ismainly de- termined by residual p– correlationswhich are smeared by an uncorrelatedγ
, anddefines the baseline of the measurement of the p–0 correlation function. The shape is parametrizedwith a Gaussian distribution and weighted by its λ parameter. Allother contributions stemming frommisidentifiedprotons orfromfeed- downareassumedtobeC(k∗)∼1.The total correlation function includingall correctionsis then multipliedbyapolynomialbaselineCnon-femto(k∗),
C
(
k∗) =
Cnon-femto(
k∗) ×
Cmodel(
k∗),
(4) toaccountforthenormalizationandnon-femtoscopicbackground effects stemming e.g. from momentum and energy conserva- tion [27]. The p–p correlation function is fitted in the rangeFig. 2.Measuredcorrelationfunctionofp–p⊕p–p .Statistical(bars)andsystematic uncertainties(boxes)areshownseparately.Thewidthofthebandcorrespondsto onestandarddeviationofthesystematicuncertaintyofthefit.
k∗∈ [0,375] MeV/c todetermine simultaneously thefemtoscopic radius r0 and the parameters of the baseline. To assess the sys- tematic uncertainties on r0 related to the fitting procedure the upperlimitofthefitregionisvariedwithink∗∈ [350,400]MeV/c.
Thebaseline ismodeledasapolynomial ofzeroth,first,andsec- ond order. Additionally, as discussed above, all three models for the p– residual correlation function are employed, andthe in- putto the λ parameters is modified by ±20%while maintaining aconstant sum ofthe primary andsecondary fractions. The p–p correlation function is shown in Fig. 2, where the width of the bandscorrespondsto onestandard deviationofthetotalsystem- atic uncertainty of the fit. The inset shows a zoom of the p–p correlation function at intermediate k∗, where the effect of re- pulsionbecomes apparent. The femtoscopicfit yields a radius of r0=1.249±0.008(stat)+−00..024021(syst)fm.
Analysesof
π
–π
andK–Kcorrelationfunctionsatultrarelativis- ticenergies inelementary [56] andheavy-ioncollisions [57] indi- cateasource distributionsignificantly deviatingfroma Gaussian.Indeed,stronglydecaying resonancesareknownto introducesig- nificantexponential tailsto thesource distribution,especially for
π
–π
pairs [47–49].Thisbecomesevidentwhenstudyingthecor- responding resonance contributions obtained from the statistical hadronizationmodelwithinthecanonicalapproach [58].Themain resonancesfeedingtopions,ρ
andω
,aresignificantlylonger-lived thanthosefeedingto protons() and0 ((1405)).Hence,itis notsurprisingthatthesourcedistributionforπ
–π
deviates from aGaussian.Theseconclusionsareunderlinedwhenfittingthep–p correlationfunctionwithaLévy-stablesourcedistribution [59,60].Leavingboththefemtoscopicradiusandthestabilityparameter
α
forthe fittodetermine,the Gaussiansource shape(
α
=2) isre- covered.EmployingaCauchy-typesourcedistribution(α
=1),the datacannotbesatisfactorilydescribed.Therefore,thepremiseofa Gaussiansourceholdsforbaryon–baryonpairs.Accordingly, a Gaussian source with femtoscopic radius r0 is usedto fit the p–0 correlation function. The parameters ofthe linearbaseline are obtainedfromafit tothe p–(
γ
) correlation functionink∗∈ [250,600]MeV/c,whereitisconsistentandkine- matically comparable with p–0, howeverfeaturing significantly smalleruncertainties. Theexperimentalp–0 correlationfunction isthenfittedintherangek∗<550 MeV/c,andvaried duringthe fitting procedure within k∗∈ [500,600] MeV/c to determine the systematic uncertainty. Additionally, the input to the λ parame- ters is modified by ±20% while maintaining a constant sum of theprimaryandsecondaryfractions.Theparameters ofthe base-Fig. 3.Measuredcorrelationfunctionofp–0⊕p–0.Statistical(bars)andsystem- aticuncertainties(boxes)areshownseparately.Thegraybanddenotesthep–(γ) baseline.Thedataarecomparedwithdifferenttheoreticalmodels.Thecorrespond- ingcorrelationfunctionsarecomputedusingCATS [46] forχEFT [20],NSC97f [26]
andESC16 [23],andusingtheLednický–Lyuboshitsapproach [51,52] forfss2 [24].
Thewidthofthebandscorrespondstoonestandard deviationofthesystematic uncertaintyofthefit.Theabsolutecorrelateduncertaintyduetothemodelingof thep–(γ)baselineisshownseparatelyasthehatchedareaatthebottomofthe figure.
lineare varied within 1
σ
oftheir uncertainties considering their correlation, includingthe caseofa constant baseline. Finally,the femtoscopicradiusisvariedaccordingtoitsuncertainties.Possible variations ofthe p–0 sourceduetocontributions ofmT scaling andstrongdecaysare incorporatedbydecreasingr0 by 15%,sim- ilarly asin [28,29]. The correspondingresonance yieldsare taken fromthestatisticalhadronization modelwithinthe canonicalap- proach [58].All correlation functions resulting from the above mentioned variationsoftheselectioncriteriaarefittedduring theprocedure, additionallyconsideringvariations ofthemasswindowtoextract thep–(
γ
)baseline.ThewidthofthebandsinFig.3corresponds toonestandarddeviationofthetotalsystematicuncertaintyofthe fit.Theabsolutecorrelateduncertaintyduetothemodelingofthe p–(γ
) baseline correlation function is shown separately atthe bottomofthefigure.4. Results
Theexperimental p–0 ⊕p–0 correlation functionisshown inFig.3.Thek∗ valueofthedatapointsischosenaccordingtothe k∗ ofthe sameevent distribution Nsame(k∗)in the correspond- ing interval. Therefore, due to the low number of counts in the first bin,thedata pointis shiftedwithrespect tothe bincentre.
Sincetheuncertaintiesofthedataaresizable,adirectdetermina- tion ofscatteringparametersvia afemtoscopicfit isnot feasible.
Instead,thedataaredirectlycomparedwiththevariousmodelsof the interaction.These include, onthe one hand,meson-exchange models,such asfss2 [24] andtwoversionsofsoft-core Nijmegen models(ESC16 [23],NSC97f [61]),andontheotherhandresultsof
χ
EFTatNext-to-LeadingOrder(NLO) [20].Thecorrelationfunction ismodeledusingtheLednický–Lyuboshitsapproach [51] consider- ingthecouplingsofthep–0 systemtop–andn-+[52] with scatteringparametersextractedfromthefss2 model.Forthecase ofESC16,NSC97fandχ
EFT,thewavefunctionofthep–0system, includingthecouplings,isusedasaninputtoCATStocomputethe correlationfunction.Thedegreeofconsistencyofthedatawiththe discussed models isexpressed by thenumber ofstandard devia- tionsnσ,computedintherangek∗<150 MeV/c fromthep-valueTable 2
Degreeofconsistencyofthedifferentmodels withthe experimentalcorrelation function.
Model p–(γ)
baseline
fss2 χEFT NSC97f ESC16
nσ (k∗<150 MeV/c) 0.2−0.8 0.2−0.9 0.3−1.0 0.2−0.6 0.1−0.5
of the theoretical curves. The range of nσ shown in Table 2 is computedasonestandarddeviationofthecorrespondingdistribu- tion.Thedataare within (0.2−0.8)
σ
consistentwiththep–(γ
) baseline,indicating thepresence ofan overallshallowstrongpo- tentialinthep–0channel.Themainsourceofuncertaintyofthe modelingofthecorrelationfunctionistheparametrizationofthe p–(γ
) baseline due the sizeable statistical uncertainties of the latter.All employed models for the N– interaction potential suc- ceedinreproducing thescatteringdatainthe S= −1 sector [7].
Duetotheavailableexperimental constraints,theoveralldescrip- tionofthep–interactionyields aconsistentdescription.Onthe other hand, the corresponding p–0 correlation functions differ significantlyamongeachother.Thisdemonstratesthatfemtoscopic measurements candiscriminate andconstrain models,andthere- forerepresenta uniqueprobeto studythe N– interaction.Both fss2 and
χ
EFT exhibit an overall repulsionin N– atintermedi- atek∗,whichmainlyoccursinthespinsinglet S=0,I=1/2 and spintriplet S=1,I=3/2 components [20,24].Inthelowmomen- tumregion,belowroughly50 MeV/c,bothmodelsyieldattraction, which is reflected in the profile of the correlation function. The Nijmegenmodels,ontheotherhand,arecharacterizedbyarather constantattractionoverthewholerangeofk∗.Inparticularatlow relativemomenta,however,thebehaviorofthetwomodelsdevi- atessignificantly.Theshapeofthecorrelationfunctionofthemost recentNijmegenmodel,ESC16,differssignificantlyfromthatofthe other calculations. This ismainly due tothe fact that the occur- rence ofboundstates inthestrangenesssector (S= −1,−2,−3) is not allowed in the model [23]. This leads to a repulsive core inall theN–channels, whichcan wellbe observedin Fig.3as thenon-monotonicbehavioratsmallrelativemomenta.Incontrast toallotherdiscussedmodels,NSC97fyieldsattractioninthespin triplet S=1,I=3/2 channel [61].Accordingly,thecorresponding correlation function demonstrates the strongest attractionat low momenta.The ratherlarge differencesamong themodeled p–0 correlation functions demonstrate that the shape ofthe latteris verysensitivetodetailsofthestronginteraction,anddrivenbythe interplayofthedifferentspinandisospinchannels.Thisshowsthe strength of femtoscopic measurements, in particular in the N–channel.
The underlying two-body N– interaction obtained within these models, however,translates into significantly differentval- uesforthein-mediumsingle-particlepotentialUwhenincluded inmany-bodycalculations. Boththefss2quark-model,along with
χ
EFT, deliver similar results at nuclear saturation density, lead- ing to an overall repulsive U of around 10–17 MeV [20,21,24].This is in agreement with evidence from relativistic mean field calculations fittingexperimental data of − atoms [12] and the experimental absence of bound states in hypernuclei [16]. On the contrary, both Nijmegen models yield a slightly attractive single-particle potential, ranging from≈ −16 MeV for NSC97fto
≈ −3 MeV forESC16. As alreadymentioned, however,the inter- pretation of hypernuclear measurements introduces a significant model dependence.This concerns not only the extraction of the experimental results, relying for instance on the framework of the distorted-wave impulse approximation [17], but also the ex- trapolationoftheoreticalcalculationstofinitedensityvia e.g. the G-matrixapproach [62,63].
5. Summary
ThisLetterpresentsthefirstdirectinvestigationofthep–0in- teraction inhigh-multiplicitypp collisions at√
s=13 TeV, hence proving the feasibility of femtoscopic studies in the N– sector.
Thep–0correlationfunctionisconsistentwiththep–(
γ
)base- line, andthereforethemeasurementindicates thepresence ofan overallshallowstrongpotential.Thedataarecomparedwithstate- of-the-artdescriptionsoftheinteraction,includingchiraleffective field theory and meson-exchange models. Due to the scarce ex- perimentalconstraintsintheN–sector,themodeled correlation functions differsignificantly among each other.The shape of the modeled correlationfunctionsappears tobevery sensitiveto de- tailsofthestronginteraction,andisdrivenbytheinterplayofthe different spin andisospin channels. This proves that femtoscopic measurements inhigh-energyppcollisions provideadirectstudy of the genuine two-body N– strong interaction. The presented femtoscopic data cannot discriminate between different models, which is also the case forthe available scattering and hypernu- cleidata.Further femtoscopic studies enabled by the abouttwo orders ofmagnitudelargerpp datasamplesof6 pb−1 inminimumbias collisions at √
s=5.5 TeV and of 200 pb−1 in high-multiplicity at √
s=14 TeV,foreseen to be collected inthe LHC Runs 3and 4 [64], will therefore shed light on the N– sector and provide constraintsonthemodelsdescribingtheinteraction.
Declarationofcompetinginterest
Theauthorsdeclarethattheyhavenoknowncompetingfinan- cialinterestsorpersonalrelationshipsthatcouldhaveappearedto influencetheworkreportedinthispaper.
Acknowledgements
TheALICECollaborationisgratefultoJ. HaidenbauerandT. Ri- jkenforvaluablediscussions andforprovidingthe theoreticalre- sultsforthep–0interaction.
The ALICECollaboration would like to thank all its engineers andtechniciansfortheirinvaluablecontributionstotheconstruc- tion of the experiment and the CERN accelerator teams for the outstanding performance of the LHC complex. The ALICE Collab- oration gratefully acknowledges the resources and support pro- videdbyallGridcentresandtheWorldwideLHCComputingGrid (WLCG) collaboration. The ALICE Collaboration acknowledges the following fundingagenciesfortheir supportin buildingandrun- ningtheALICEdetector:A.I.AlikhanyanNationalScienceLabora- tory(YerevanPhysicsInstitute)Foundation (ANSL),State Commit- 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 Nacional de Desenvolvimento Científico e Tecnológico(CNPq), Fi- nanciadora de Estudose Projetos (Finep),Fundação de Amparo à Pesquisa do Estado de São Paulo(FAPESP) andUniversidadeFed- eraldoRioGrandedoSul(UFRGS),Brazil;MinistryofEducationof China (MOEC), MinistryofScience &Technology ofChina (MSTC) and NationalNatural Science Foundation of China (NSFC), China;
Ministry of Science and Education and Croatian Science Founda- tion,Croatia;CentrodeAplicacionesTecnológicasyDesarrolloNu- clear (CEADEN), Cubaenergía, Cuba;Ministry of Education, Youth and Sports of the Czech Republic, Czech Republic; The Danish Council for Independent Research | Natural Sciences, the Villum Fonden and Danish National Research Foundation (DNRF), Den- mark; HelsinkiInstitute ofPhysics(HIP), Finland;Commissariatà