Citation for this paper:
Akhmetshin, R.R., Amirkhanov, A.N., Anisenkov, A.V., Aulchenko, V.M., Banzarov,
V.Sh., Bashtovoy, N.S.,… Yudin, Yu.V. (2020).
Study of the process e
+e
−→
K
0SK
0Sπ
+π
−in the c.m. energy range 1.6–2.0 GeV with the CMD-3 detector
. Physics Letters B,
804, 135380.
https://doi.org/10.1016/j.physletb.2020.135380
UVicSPACE: Research & Learning Repository
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Study of the process e
+e
−→
K
0SK
0Sπ
+π
−in the c.m. energy range 1.6–2.0 GeV with the
CMD-3 detector
R.R. Akhmetshin, A.N. Amirkhanov, A.V. Anisenkov, V.M. Aulchenko, V.Sh.
Banzarov, N.S. Bashtovoy,D.E. Berkaev, A.E. Bondar, A.V. Bragin, S.I. Eidelman,
D.A. Epifanov, L.B. Epshteyn, A.L. Erofeev, G.V. Fedotovich, S.E. Gayazov, F.J.
Grancagnolo, A.A. Grebenuk, S.S. Gribanov… A.L. Sibidanov, E.P. Solodov, M.V.
Timoshenko, V.M. Titov, A.A. Talyshev, A.I. Vorobiov, I.M. Zemlyansky, Yu.V. Yudin
May 2020
© 2020 The Author(s.) Published by Elsevier B.V. This is an open access article
under the CC BY license ( http://creativecommons.org/licenses/by/4.0/ ).
This article was originally published at:
Contents lists available atScienceDirect
Physics
Letters
B
www.elsevier.com/locate/physletb
Study
of
the
process
e
+
e
−
→
K
0
S
K
0
S
π
+
π
−
in
the
c.m.
energy
range
1.6–2.0
GeV
with
the
CMD-3
detector
R.R. Akhmetshin
a,
b,
A.N. Amirkhanov
a,
b,
A.V. Anisenkov
a,
b,
V.M. Aulchenko
a,
b,
V.Sh. Banzarov
a,
N.S. Bashtovoy
a,
D.E. Berkaev
a,
b,
A.E. Bondar
a,
b,
A.V. Bragin
a,
S.I. Eidelman
a,
b,
e,
D.A. Epifanov
a,
b,
L.B. Epshteyn
a,
b,
c,
A.L. Erofeev
a,
b,
G.V. Fedotovich
a,
b,
S.E. Gayazov
a,
b,
F.J. Grancagnolo
f,
A.A. Grebenuk
a,
b,
S.S. Gribanov
a,
b,
D.N. Grigoriev
a,
b,
c,
F.V. Ignatov
a,
b,
V.L. Ivanov
a,
b,
S.V. Karpov
a,
A.S. Kasaev
a,
V.F. Kazanin
a,
b,
I.A. Koop
a,
b,
A.A. Korobov
a,
b,
A.N. Kozyrev
a,
c,
E.A. Kozyrev
a,
b,
P.P. Krokovny
a,
b,
A.E. Kuzmenko
a,
b,
A.S. Kuzmin
a,
b,
I.B. Logashenko
a,
b,
P.A. Lukin
a,
b,
A.P. Lysenko
a,
K.Yu. Mikhailov
a,
b,
V.S. Okhapkin
a,
E.A. Perevedentsev
a,
b,
Yu.N. Pestov
a,
A.S. Popov
a,
b,
G.P. Razuvaev
a,
b,
A.A. Ruban
a,
N.M. Ryskulov
a,
A.E. Ryzhenenkov
a,
b,
A.V. Semenov
a,
b,
Yu.M. Shatunov
a,
V.E. Shebalin
a,
b,
D.N. Shemyakin
a,
b,
B.A. Shwartz
a,
b,
D.B. Shwartz
a,
b,
A.L. Sibidanov
a,
d,
E.P. Solodov
a,
b,
∗
,
M.V. Timoshenko
a,
V.M. Titov
a,
A.A. Talyshev
a,
b,
A.I. Vorobiov
a,
I.M. Zemlyansky
a,
Yu.V. Yudin
a,
baBudker Institute of Nuclear Physics, SB RAS, Novosibirsk, 630090, Russia bNovosibirsk State University, Novosibirsk, 630090, Russia
cNovosibirsk State Technical University, Novosibirsk, 630092, Russia dUniversity of Victoria, Victoria, BC, V8W 3P6, Canada
eLebedev Physical Institute RAS, Moscow, 119333, Russia fInstituto Nazionale di Fisica Nucleare, Sezione di Lecce, Lecce, Italy
a
r
t
i
c
l
e
i
n
f
o
a
b
s
t
r
a
c
t
Article history:
Received12December2019 Receivedinrevisedform3March2020 Accepted17March2020
Availableonline25March2020 Editor:L.Rolandi
Thecrosssectionoftheprocesse+e−→K0
SK0S
π
+π
−hasbeenmeasuredusingadatasampleof56.7pb−1 collectedwiththeCMD-3detector attheVEPP-2000e+e− collider.596±27 and 210±18 signal eventshavebeen selectedwithsixandfivedetectedtracks,respectively,inthecenter-of-massenergy range1.6–2.0GeV.Thetotalsystematicuncertaintyofthecrosssectionisabout10%.Thestudyofthe productiondynamicsconfirmsthedominanceoftheK∗(892)+K∗(892)−intermediatestate.
©2020TheAuthor(s).PublishedbyElsevierB.V.ThisisanopenaccessarticleundertheCCBYlicense (http://creativecommons.org/licenses/by/4.0/).FundedbySCOAP3.
1. Introduction
e+e− annihilationintohadronsbelow2GeVisrichforvarious multiparticlefinal states.Theirdetailedstudies are importantfor developmentofphenomenologicalmodelsdescribingstrong inter-actionsat low energies.One ofthe final states, K0SK0S
π
+π
−,has beenstudied beforeby the BaBarcollaboration [1], based onthe Initial-StateRadiation(ISR)method.Theiranalysisshowedthat be-lowthecenter-of-massenergy(Ec.m.)of2GeVtheprocessisdom-inatedby the K∗
(
892)
+K∗(
892)
− intermediatestatewithasmall*
Correspondingauthorat:BudkerInstituteofNuclearPhysics,SBRAS, Novosi-birsk,630090,Russia.E-mail address:solodov@inp.nsk.su(E.P. Solodov).
contribution of the K0SK0S
ρ
(
770)
reaction. As a part of the total hadronic crosssection, thecross section ofe+e−→
K0SK0Sπ
+π
−isinterestingforthecalculationsofthehadronicvacuum polariza-tion and, as a consequence, forthe hadronic contributionto the muon anomalous magnetic moment [2–4]. Until recently, of var-ious possible charge combinations of the KK
¯
π π
final state only two were measured (K+K−π
+π
− and K+K−π
0π
0).Contribu-tionsfromotherKK
¯
π π
finalstates(K±K0Sπ
∓π
0,K0 SK0 S
π
0
π
0etc.)were taken into account using isospin relations that resulted in largeuncertainties.Themeasurementsofotherexclusivereactions, see [5] andreferencestherein, helpeddecreasingsuch uncertain-tiesandchangedthecontributionofsuchfinalstatestothemuon anomalous magneticmoment from3
.
31±
0.
58 to2.
41±
0.
11 in unitsof 10−10 fortheenergyrange below2 GeV. Thedifferencehttps://doi.org/10.1016/j.physletb.2020.135380
0370-2693/©2020TheAuthor(s).PublishedbyElsevierB.V.ThisisanopenaccessarticleundertheCCBYlicense(http://creativecommons.org/licenses/by/4.0/).Fundedby SCOAP3.
2 R.R. Akhmetshin et al. / Physics Letters B 804 (2020) 135380
Table 1
Energyinterval,integratedluminosity,numberofsignal6-trackevents,numberof signal5-trackevents,detectionefficiency,and theobtainedcrosssectionforthe e+e−→K0SK
0
Sπ+π−reaction.Onlystatisticaluncertaintiesareshown.
Ec.m., MeV L, nb−1 N6π N5π σK0 SK0Sπ+π−, nb 2007.0±0.5 4259 45±7 19.0±5.0 0.048 0.341±0.047 1980±1 2368 29±6 13.5±4.1 0.053 0.366±0.063 1940–1962 5230 95±10 33.8±6.7 0.055 0.484±0.047 1890–1925 5497 72±9 25.8±5.9 0.059 0.329±0.037 1870–1884 16803 218±17 61.5±10.1 0.061 0.298±0.021 1800–1860 8287 79±11 37.2±7.0 0.064 0.238±0.026 1700–1780 8728 47±8 11.5±4.8 0.066 0.111±0.018 1600–1680 7299 11±4 7.8±3.7 0.068 0.041±0.011
isratherlargeandthedetailedstudy oftheproductiondynamics canfurtherimprovetheaccuracyofthesecalculationsand under-standingoftheenergydependenceofthecrosssection.
Inthispaperwereporttheanalysisofthedatasampleof56.7 pb−1 collected at the CMD-3 detector in the 1.6–2.0 GeV Ec.m.
range. Thesedata were collected during four energy scans, with a 5–10MeV c.m. energystep each, performedat the VEPP-2000
e+e−collider [6–9] inthe2011,2012and2017experimentalruns. In2017(abouthalfofintegratedluminosity)thebeamenergywas monitored by the back-scattering laser-lightsystem [10,11], pro-viding an absolutebeam-energy monitoring withbetter than 0.1 MeV uncertainty at every 10-20 minutes of data taking. In ear-lier runs the beam energy was determined using measurements ofchargedtrackmomentainthedetectormagneticfield withan about1MeVuncertainty.Sincethecrosssectionoftheprocessis small,we combineourscannedpoints intoeightenergyintervals asshowninTable1.
Thegeneral-purposedetectorCMD-3hasbeendescribedin de-tail elsewhere [12]. Its tracking system consists of a cylindrical drift chamber (DC) [13] and double-layer multiwire proportional Z-chamber, both also used for a charged track trigger, and both inside a thin (0.2 X0) superconducting solenoid with a field of
1.3 T.The trackingsystemprovides the98-99%trackingefficiency in about 70% of the solid angle. The liquid xenon (LXe) barrel calorimeterwith a 5.4 X0 thickness has fine electrode structure,
providing 1–2 mm spatial resolution for photons independently of their energy [14], and is located in the cryostat vacuum vol-umeoutsidethesolenoid.ThebarrelCsIcrystalcalorimeterwitha thicknessof8.1 X0 surroundstheLXecalorimeter,whilethe
end-capBGO calorimeterwithathickness of13.4 X0 is placedinside
thesolenoid [15].Altogether,thecalorimeterscover0.9ofthesolid angle and amplitude signals provide information for the neutral trigger.Chargedtriggerrequirespresenceofonlyonechargedtrack inDC,therefore ithas practically 100%efficiency forourstudied processwithfiveorsixdetected tracks.Arelatively largefraction ofthese events hassufficient energy deposition inthe calorime-terforthe independent neutraltrigger: theseevents are usedto controlthechargedtriggerefficiency.The luminosityismeasured usingtheBhabhascatteringeventsatlarge angleswithabout1% systematicuncertainty [16].
Tounderstandthedetectorresponse toprocesses understudy andto obtainthe detectionefficiency, we havedeveloped Monte Carlo(MC) simulationofour detectorbasedon theGEANT4 [17] package,inwhichallsimulatedeventspassthewhole reconstruc-tionandselectionprocedure.TheMCsimulationusesprimary gen-eratorswith the matrixelements forthe KS0K0S
π
+π
− final state withtheK∗(
892)
+K∗(
892)
−,K1(
1400)
K0S→
K∗(
892)
±π
∓KS0,andK1
(
1270)
K0S→
K0Sρ
(
770)
K0S intermediatestates.Theprimarygen-erator with the K0SK0S
π
+π
− in the phase-space model (PS) has beenalsodeveloped. Theprimary generator includesradiation of photonsbyan initialelectronorpositron,calculatedaccordingto Ref. [20].2. Selectionofe+e−
→
KS0K0Sπ
+π
−eventsTheanalysisprocedureissimilartoourstudyoftheproduction of sixcharged pions described in Ref. [19]. Candidate events are requiredtohavefiveorsixcharged-particletracks,eachhaving:
•
morethanfivehitsintheDC;•
atransversemomentumlargerthan40MeV/c;•
a minimum distance from a track to the beam axis in the transverseplane oflessthan6cm,thatallowsreconstruction ofadecaypointofK0S atlargedistances;•
aminimumdistancefromatracktothecenterofthe interac-tionregionalongthebeamaxisZoflessthan15cm. Reconstructed momenta andangles of thetracks forthe five-andsix-trackeventsareusedforfurtherselection.Inourreconstructionprocedurewecreatethelistofthe KS0
→
π
+π
− candidateswhichincludeseverypairofoppositelycharged tracks,assumingthemtobepions,withtheinvariantmasswithin±
80 MeV/c2 fromthe K0S mass [22] and acommon vertexpoint
within a spacialuncertainty of theDC. We calculate momentum andenergyforeach K0S candidatetakingthevalueoftheK0S mass fromRef. [22].
At the first stage ofsignal event selectionwe requireatleast two K0
S candidateswithfourindependenttracks plusone ortwo
additional charged tracks originating from the collision point. If there arestill more thantwo K0S candidates, twocandidate pairs withminimaldeviationsfromtheK0S massareretained. Addition-ally,werequirethedistancefromthebeamaxisforthetracksnot fromK0
S tobelessthan0.35cm.
Fig.1showsthescatter plotfortheinvariantmassofthefirst
K0S
→
π
+π
− candidate vs the second one for data (a) and MC simulation(b).Allenergyintervalsarecombinedforthepresented histogramsindata.Thelinesshowselectionsforthesignalevents in thecentral squareandforthe backgroundlevelestimate from theeventsinothereightsquares.Fig. 2(a) shows the scatter plot forthe invariant mass of the
K0
S
→
π
+π
−candidatesvstheradialdistanceofthereconstructedvertexfromthe beamaxis.Events associatedwith K0S areclearly seenaswellasthebackgroundevents.Reddots(inthecolor ver-sion)areforsimulation.Fig.2(b)showsaradialdistancefromthe beamaxisforthetracksnotassociatedwiththe K0
S decay.The
ad-ditional requirementfor thisdistance tobe lessthan 0.35cm is shownbytheline.
The central vertical andhorizontalbandsin Fig.1 correspond totheeventswithone wronglyreconstructed K0S,whichareseen inFig.1(b)alsoforsimulationduetoacombinatorialeffect,orif oneoftheK0S decaystoothermodes.Fordatatheseeventscanbe also due to a possible background, like e+e−
→
K0SK±π
∓π
+π
−witha misidentifiedormissingchargedkaon,whenonlyone K0S
ispresentinthefinalstate:theseeventscontributetotheselected datasampleinFig.1(a).
Whilewedonotusespecialorderingforthecalculationofthe firstandsecondm
(
K0S)
,thebackgroundcontributiontothevertical andhorizontalbandscanbe different,andwe usethe“nine tile” method to extract the numberof signal eventsand estimate the background contribution. In this procedure the two-dimensional plot isdivided intonine tiles withequalarea asshownin Fig.1 by lines.The tiles inFig.1 arenumbered fromleft torightfrom top to bottom. The central (signal) tile contains N5 events withtwowell-reconstructed K0S candidates,whiletheverticaland hor-izontal tiles, connectedto the central signal tile,are used foran estimate of thebackgroundcontribution to N5 fromthewrongly
Fig. 1. Scatterplotoftheinvariantmassofone
K
0Scandidatevsinvariantmassforthesecond
K
0Scandidatefordata(a)andMCsimulation(b).Thelinesshowselectionsforthesignaleventsandforthebackgroundlevelestimate.
Fig. 2. (a)Scatterplotoftheinvariantmassofthe
K
0Scandidatevstheradialdistanceofthedecayvertex(crosses):MCsimulationisshownby(redincolorversion)dots.
(b)Radialdistanceofthenot-from-kaonpionsfromthebeamaxis.Thelineshowsappliedselection.
to estimate the random background. The number of background eventsinthecentraltile,Nbkg,isthusdeterminedas
Nbkg
= (
N2+
N4+
N6+
N8)/2− (
N1+
N3+
N7+
N9)/4.
(1)Notethat therandom backgroundfora single tileis takentwice fromtheverticalandhorizontaltiles,sotheaveragerandom back-ground,estimatedfromthecornertiles,isusedforcompensation. Atthenextstageofeventselection,we calculatetheexpected distribution of any kinematic quantity by weighting the contri-bution of the eight tiles as in Eq. (1). This is compared to the distributionobservedinthesignalregion.
Fig.3shows thehistograms fortheradial distance ofthe de-cayvertexforthe K0
S
→
π
+π
− candidatesinthesignalregionofFig. 1 for data (a) and simulation at 1900 MeV (b). Points with errorsrepresentthecontributionofthebackground,estimatedby the“nine tile”methodofEq. (1).Thebackgroundfromthe beam-originatingeventsindataisseeninafewfirstbinsandiswell es-timatedbythemethod:itisnotdominating,sowedonotimpose anyrestrictions onthisdistance.Theprocedureis alsoappliedto the simulation, and Eq. (1) gives about 5% of the “background” events (Fig. 3(b)) due to only one correctly reconstructed K0S or due to small non-linearity of events in the bands, which is as-sumed to be linearfor the method.In our analysis theseevents aretreatedinthesamewayasfordata.Thesystematic uncertain-tiesofthemethodarediscussedbelow.
Forthe six- orfive-track K0
SK0S
π
+π
− candidates we calculatethetotalenergyoftwo K0S’sandtwopions:forthefive-track can-didatesthemissingmomentum isusedtocalculatetheenergyof thelostpion.Fig.4(a)showsthescatterplotofthedifference be-tween the total energyand c.m. energy, Etot
−
Ec.m., vs the totalmomentum of six- (a) or five-track (b) candidates, Ptot for data.
Events fromthecentraltileof Fig.1areshown. Aclearsignal of the e+e−
→
K0SKS0π
+π
− reaction is seen in Fig. 4(a) asa clus-terofcrossesnear zero,inagreementwith theexpectationfrom the simulation shownby (redin the colorversion) dots. We re-quire Ptotto belessthan180MeV/c2,thusreducing thenumberofeventswithhardradiativephotons.
Theexpectedsignaloffive-trackcandidateshastheEtot
−
Ec.m.valuenearzero,andthePtotvalueisdistributedupto500MeV/c,
as shown by the (red) dots from the signal MC simulation in Fig. 4(b). The (black) crosses show our data: signal events are clearlyseen.
Fig.5 showstheprojection plots ofFig.4, Etot
−
Ec.m., forthesix-track(a) withappliedselection, andthe five-track(b)events: the histograms present events from the signal tile, while dots with errors are our estimate ofthe background contribution us-ingEq. (1).Allenergyintervalsaresummed.
Toobtainthenumberofsignalevents,weusedistributions of Fig.5fortheEtot
−
Ec.m. difference,i.e.Nsig=
N5−
Nbkg.Wesix-4 R.R. Akhmetshin et al. / Physics Letters B 804 (2020) 135380
Fig. 3. Radialdistanceofthedecayvertexforthe K0
S→π+π− candidatesinthesignalregionofFig.1fordata(a)andsimulation(b).Dotswitherrorsrepresentthe
backgroundcontributionestimatedfromEq. (1).
Fig. 4. (a)Scatterplotofthedifferencebetweentheenergyof
K
0SK0Sπ+π−candidatesandc.m.energyvstotalmomentumforeventswithsixtracks.Thecrossesarefordata,
whilethesignalsimulationisshownbyred(incolorversion)dots;thelineshowstheappliedselection.(b)Scatterplotofthedifferencebetweentheenergyof
K
0SK
0
Sπ+π−
candidatesandc.m.energyvstotalmomentumforeventswithfivetracks.Thecrossesarefordata,whilethesignalsimulationisshownbyred(incolorversion)dots.
Fig. 5. (a)Thedifferencebetweentheenergyofthe
K
0SK0Sπ+π− candidatesandc.m.energyafterselectionbythelineinFig.4forsix-trackevents(a)andfive-track
Fig. 6. (a)Thedifferencebetweentheenergyofthe
K
0SKS0π+π−candidatesandc.m.energyafterbackgroundsubtractionforsix-track(a)andfive-trackevents(b)foreight
c.m.energyintervals(dots):lefttoright,toptobottomaccordingtoTable1.Histogramsshowexpectedsignalsfromsimulation,normalizedtothetotalnumberofevents ineachplot.
Fig. 7. (a)Experimental K0
Sπ− vs K
0
Sπ+ invariant massdistribution(twoentriesperevent,crosses)fortheeventsfromthesignalregionofFig.1.Dots(redincolor
version)showthesimulateddistributionforthe
K
∗(892)+K∗(892)−intermediatestate.(b)Projectionplotof(a)(fourentriesperevent)withthefitfunction(solidcurve) todeterminethenumberofeventswiththeK
∗(892)signaloverthebackgrounddistribution(dottedcurve).Thehistogramshowsthecorrespondingnumberofsimulated eventsfortheK
∗(892)+K∗(892)−intermediatestate.and five-track events, and count remaining events in the
±
100 MeVregionforthesix-trackevents,andinthe±
200MeVregion for the five-track events. The obtained differences are shown in Fig.6 by dots for six- (a)and five-track (b) events: from left to right,fromtoptobottomaccordingtoenergyintervalsofTable1. Thehistogramsshowexpectedsignalsfromthesimulation.In to-tal,we obtain 596±
27 and210±
18for six- andfive-track signal events,respectively.Thenumbersofselectedeventsdeterminedin eachenergyintervalarelistedinTable1.3. Studyoftheproductiondynamics
First attempts to study the dynamics of the process e+e−
→
K0SK0S
π
+π
− were carried out by the BaBar Collaboration [1].Theyreportedtheobservationofthee+e−
→
K∗(
892)
+K∗(
892)
−,K∗
(
892)
±π
∓K0S, K0SK0Sρ
(
770)
processes, which contribute to theK0
SK0S
π
+π
− final state, with a dominant production of theK∗
(
892)
+K∗(
892)
− intermediate state for the c.m. energies be-low 2.5 GeV. In the model of the KK¯
π
+π
− production theK1
(
1400)
K0S intermediate state decays to K∗(
892)
±π
∓K0S, whileK1
(
1270)
KS0canbeobservedinthe K0SK0Sρ
(
770)
state.Fig. 7(a) shows the scatter plot of the K0S
π
− invariant mass vs K0Sπ
+ (two entries/event, all energy intervals are summed) for the K0SKS0π
+π
− six-track candidates. A clear signal of the correlated production of the pair of charged K∗(
892)
’s is seen (crosses),inagreementwiththeexpecteddistributionforthe sim-ulatede+e−→
K∗(
892)
+K∗(
892)
−reaction(dots).Fig.7(b)shows the projection plot of (a) (four entries per event) which we fit with the sum ofa double-Gaussian distribution for the K∗(
892)
signal and a polynomial function for the background. The back-groundincludes also wrongly assigned K0Sπ
combinations. Gaus-sian parameters are taken from the simulated histogram shown6 R.R. Akhmetshin et al. / Physics Letters B 804 (2020) 135380
Fig. 8. (a)Thebackground-subtractedπ+π−invariantmassdistribution(dots)incomparisonwiththesimulateddistribution(solidhistogram).(b)Thebackground-subtracted K0Sπ+π−(twoentriesperevent)invariantmassdistribution(dots)incomparisonwiththesimulatedone(asolidhistogram).Inbothplotsthesimulateddistributionincludes
the
K
∗(892)+K∗(892)−intermediatestateplus30%oftheK
1(1270)K0S,whichcontributionisshownbyadottedhistogram.Fig. 9. (a)Thebackground-subtractedexperimental(dots)polarangledistributionincomparisonwiththesimulateddistribution(histograms)forthemissingpion(a)andall detectedpions(b).
in Fig. 7(b). The fit yields 788
±
73±
95 events: a second uncer-tainty is from a variation of the fit functions. Each event from the K∗(
892)
+K∗(
892)
− reaction contributes twice, so a half of thisvalue should be compared to 596±
27, thetotal number of thesix-tracksignalevents.Theobtainednumberindicatesthatthe contributionoftheK∗(
892)
+K∗(
892)
−intermediatestatedoesnot exceed66±
11%.With our data we cannot quantitatively extract a contribu-tionfromproductionofa single K∗
(
892)
orfromeventswithoutK∗
(
892)
’s.Wecalculatethebackground-subtractedinvariantmassforthe twopionsinthesix-tracksample,notoriginatingfromK0S,shown inFig.8(a),andforthe KS0
π
+π
− invariantmass(twoentriesper event), shown in Fig. 8(b). These distributions indicate that theρ
(
770)
resonanceintheπ
+π
− invariantmass,andthe K1(
1270)
resonancein the K0S
π
+π
− invariant massdistribution cannot be excluded. The solid histograms show the simulated distributions of the K∗(
892)
+K∗(
892)
− intermediate state summed with the 30%contributionfromtheK1(
1270)
K0S→
K0SK0Sρ
(
770)
intermedi-atestate.Thelattercontributionisshownbythedottedhistogram.
Withthecurrentdatasamplewecannotquantitativelyextractthis contribution.
4. Detectionefficiency
Inourexperiment, theacceptanceoftheDCforchargedtracks is not100%, andthe detectionefficiencydependsonthe produc-tiondynamicsofthereactionaswellasonthetrackreconstruction efficiencyintheDC.
To obtain the detection efficiency, we simulate K0SK0S
π
+π
−productionin theprimary generators,50000 eventsforeach c.m. energyintervalforeachmodel,passsimulatedeventsthroughthe CMD-3 detectorusing theGEANT4 [17] package, andreconstruct them withthesamesoftware asexperimentaldata.We calculate the detection efficiencyfrom theMC-simulated events asa ratio of events afterthe selectionsdescribed inSecs. 2,3 to the total numberofgeneratedevents.
Our selection ofsix- and five-track signal eventsallows us to estimate a differencein thetrackingefficiencyindata and simu-lation.Fig.9showsbydotsthebackground-subtractedpolarangle foramissingpion(a)andforalldetectedpions(b).Thehistogram
Fig. 10. (a)The ratioof the numberof five- to six-track eventsfor data (dots) and simulation for the different intermediatestates: phasespace model(squares), K∗(892)+K∗(892)− intermediatestate(opensquares),
K
1(1400)KS0(triangles),and K1(1270)K0S intermediatestate(open circles).(b)DetectionefficiencyobtainedfromtheMCsimulationforthe
e
+e−→K0SK
0
Sπ+π−reactionforthedifferentintermediatestates(symbolslegendisthesameasfor(a)).
represents the simulated distribution forthe K∗
(
892)
+K∗(
892)
− intermediatestate.Weobservereasonableagreementfordataand simulation inthese distributions as well as inthe calculated ra-tioofthenumberoffive- tosix-trackeventsateach c.m.energy interval,shownin Fig.10 (a)by open squares. Thevalues ofthe ratioforthephase-spacemodel(squares), K1(
1400)
K0S (triangles),andK1
(
1270)
K0S intermediatestate (opencircles) arealsoshowninFig.10(a)andtheyarelesscompatiblewithdata.
Wecalculatethedetectionefficiencyforthesumofeventswith sixandfivedetectedtracks.Fig.10(b)showsthedetection efficien-cies obtained for the e+e−
→
K0SK0S
π
+π
− reaction fordifferentintermediate states:markers are thesame asforFig. 10(a). The detectionefficiencies fordifferentmodesare relatively close, and the efficiencies calculated for the K∗
(
892)
+K∗(
892)
− intermedi-ate state only and calculated with a 30% contribution from theK1
(
1270)
K0S reactiondifferbylessorabout5%.5. Crosssectioncalculation
Ineachenergyintervalthecrosssectioniscalculatedas
σ
=
N6π+
N5πL
·
· (
1+ δ)
,
where N6π , N5π are the background-subtracted numbers of
sig-naleventswithsixandfivetracks,L istheintegratedluminosity forthisenergyinterval,
is thedetection efficiency,and
(
1+ δ)
is the radiative correction calculated according to Ref. [20,21]. To calculate the radiative correction, we use BaBar data for thee+e−
→
K0SK0Sπ
+π
−reaction[1] asafirstapproximation,and ob-tain(
1+ δ)
=
0.
92 withveryweakenergydependence.Wecalculatethecrosssectionsforthee+e−
→
KS0K0Sπ
+π
− re-actions usingthe efficiency shownby open squaresin Fig. 10(b) for the K∗(
892)
+K∗(
892)
− intermediate state. The cross section isshownin Fig.11. Wealso calculatethe crosssection by using onlyeventswithsixdetected tracks: a lessthan5% difference is observed.Theenergy interval,integratedluminosity, thenumberof six-andfive-trackevents,efficiency,andtheobtainedcrosssectionfor eachenergyintervalarelistedinTable1.
Fig. 11. The
e
+e−→K0SK
0
Sπ+π−crosssectionmeasuredwiththeCMD-3detector
atVEPP-2000(circles).TheresultsoftheBaBarmeasurement [1] areshownbyopen circles.
6. Systematicuncertainties
The following sources of systematic uncertainties are consid-ered.
•
The tracking efficiencywas studied in detail inour previous papers [18,19],andthecorrectionforthetrackreconstruction efficiency compared to the MC simulation is about1.0±
1.0% per track.Sincewe add events withonemissingtrack (from the twonot from K0S),the MC-simulated detectionefficiency iscorrectedby(–5±
3)%:theuncertaintyistakenasthe corre-spondingsystematicuncertainty.•
The model dependence of the acceptance is determined by comparing efficiencies calculatedfor thedifferent production dynamics.The maximumdifference ofthe detection efficien-cies of the dominant K∗(
892)
+K∗(
892)
− intermediate state andthoseforother statesis about15%. apossibleadmixture (ofabout30%)ofother stateschangestheefficiencybyabout 5%,whatistakenasthesystematicuncertaintyestimate.•
Sinceonlyonechargedtrackissufficientforatrigger(98–99% single track efficiency),and usinga cross check withthe in-dependentneutraltrigger,weconcludethatforthemultitrack8 R.R. Akhmetshin et al. / Physics Letters B 804 (2020) 135380
eventsthe trigger inefficiency givesa negligible contribution tothesystematicuncertainty.
•
The systematic uncertainty due to the selection criteria is studied by varying the requirements described above and doesn’texceed5%.•
The uncertainty on the determination of the integrated lu-minositycomes fromthe selection criteriaofBhabha events, radiativecorrectionsandcalibrations ofDCandCsI anddoes notexceed1% [16].•
The uncertainty in the background subtraction is studied by the variation of the tile dimensions (20×
20, 25×
25, and 30×
30MeV/c2 dimensionstested),andby thecomparisonof thecrosssectioncalculatedusingonlysix-trackevents.Aless than5%differenceisobserved.•
Theradiativecorrection uncertaintyisestimatedasabout2%, mainlydue tothe uncertaintyon themaximum allowed en-ergyoftheemittedphoton,aswellasfromtheuncertaintyon thecrosssection.Theabovesystematicuncertaintiessummedinquadraturegive anoverallsystematicerrorofabout10%.
7. Conclusion
Thetotalcrosssectionoftheprocess e+e−
→
K0SK0Sπ
+π
− has beenmeasuredusing56.7pb−1 ofintegratedluminositycollectedby the CMD-3 detector at the VEPP-2000 e+e− collider in the 1.6–2.0GeVc.m.energyrange.Thesystematicuncertaintyisabout 10%.Fromourstudywecanconcludethattheobservedcross sec-tioncanbedescribedbythee+e−
→
K∗(
892)
+K∗(
892)
−reaction, but an about 30–35% contribution of the K1(
1270)
K0Sinterme-diate state is not excluded. The measured cross section for the
e+e−
→
K0SK0Sπ
+π
− reactionagreeswiththeonlyavailable mea-surementbyBaBar [1].Declarationofcompetinginterest
Theauthorsdeclarethattheyhavenoknowncompeting finan-cialinterestsorpersonalrelationshipsthatcouldhaveappearedto influencetheworkreportedinthispaper.
Acknowledgements
The authorsare gratefultoA.I. Milsteinforhis helpwith the-oretical interpretation anddevelopmentof themodels.We thank theVEPP-2000teamforexcellent machineoperation.Theworkis partially supported by the Russian Foundation forBasic Research grant17-02-00897.
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