Contents lists available atScienceDirect
Physics
Letters
B
www.elsevier.com/locate/physletb
First
observation
and
study
of
the
K
±
→
π
±
π
0
e
+
e
−
decay
The
NA48/2
Collaboration
J.R. Batley,
G. Kalmus,
C. Lazzeroni
1,
2,
D.J. Munday
1,
M.W. Slater
1,
S.A. Wotton
1 CavendishLaboratory,UniversityofCambridge,Cambridge,CB30HE,UK3R. Arcidiacono
4,
G. Bocquet,
N. Cabibbo
†,
A. Ceccucci,
D. Cundy
5,
V. Falaleev
6,
M. Fidecaro,
L. Gatignon,
A. Gonidec,
W. Kubischta,
A. Maier,
A. Norton
7,
M. Patel
8,
A. Peters
CERN,CH-1211Genève23,Switzerland
S. Balev
†,
P.L. Frabetti,
E. Gersabeck
9,
E. Goudzovski
1,
2,
10,
P. Hristov
11,
V. Kekelidze,
V. Kozhuharov
12,
13,
L. Litov
12,
D. Madigozhin,
M. Misheva
∗
,
14,
N. Molokanova,
I. Polenkevich,
Yu. Potrebenikov,
S. Stoynev
15,
A. Zinchenko
†JointInstituteforNuclearResearch,141980Dubna(MO),Russia
E. Monnier
16,
E. Swallow
†,
R. Winston
17 TheEnricoFermiInstitute,TheUniversityofChicago,Chicago,IL60126,USAP. Rubin
18,
A. Walker
DepartmentofPhysicsandAstronomy,UniversityofEdinburgh,Edinburgh,EH93JZ,UK
P. Dalpiaz,
C. Damiani,
M. Fiorini,
M. Martini,
F. Petrucci,
M. Savrié,
M. Scarpa,
H. Wahl
DipartimentodiFisicaeScienzedellaTerradell’UniversitàeSezionedell’INFNdiFerrara,I-44122Ferrara,ItalyW. Baldini,
A. Cotta Ramusino,
A. Gianoli
Sezionedell’INFNdiFerrara,I-44122Ferrara,ItalyM. Calvetti,
E. Celeghini,
E. Iacopini,
M. Lenti,
G. Ruggiero
19 DipartimentodiFisicadell’UniversitàeSezionedell’INFNdiFirenze,I-50125SestoFiorentino,ItalyA. Bizzeti
20,
M. Veltri
21Sezionedell’INFNdiFirenze,I-50019SestoFiorentino,Italy
M. Behler,
K. Eppard,
M. Hita-Hochgesand,
K. Kleinknecht,
P. Marouelli,
L. Masetti,
U. Moosbrugger,
C. Morales Morales,
B. Renk,
M. Wache,
R. Wanke,
A. Winhart
1 InstitutfürPhysik,UniversitätMainz,D-55099Mainz,Germany22https://doi.org/10.1016/j.physletb.2018.11.046
0370-2693/©2018TheAuthor(s).PublishedbyElsevierB.V.ThisisanopenaccessarticleundertheCCBYlicense(http://creativecommons.org/licenses/by/4.0/).Fundedby SCOAP3.
D. Coward
23,
A. Dabrowski
11,
T. Fonseca Martin,
M. Shieh,
M. Szleper
24,
M. Velasco,
M.D. Wood
23DepartmentofPhysicsandAstronomy,NorthwesternUniversity,Evanston,IL60208,USA
G. Anzivino,
E. Imbergamo,
A. Nappi
†,
M. Piccini,
M. Raggi
25,
M. Valdata-Nappi
DipartimentodiFisicadell’UniversitàeSezionedell’INFNdiPerugia,I-06100Perugia,ItalyP. Cenci,
M. Pepe,
M.C. Petrucci
Sezionedell’INFNdiPerugia,I-06100Perugia,ItalyF. Costantini,
N. Doble,
L. Fiorini
26,
S. Giudici,
G. Pierazzini
†,
M. Sozzi,
S. Venditti
DipartimentodiFisicadell’UniversitàeSezionedell’INFNdiPisa,I-56100Pisa,ItalyG. Collazuol
27,
L. DiLella
28,
G. Lamanna
28,
I. Mannelli,
A. Michetti
ScuolaNormaleSuperioreeSezionedell’INFNdiPisa,I-56100Pisa,ItalyC. Cerri,
R. Fantechi
Sezionedell’INFNdiPisa,I-56100Pisa,ItalyB. Bloch-Devaux
∗
,
29,
C. Cheshkov
30,
J.B. Chèze,
M. De Beer,
J. Derré,
G. Marel,
E. Mazzucato,
B. Peyaud,
B. Vallage
DSM/IRFU–CEASaclay,F-91191Gif-sur-Yvette,France
M. Holder,
M. Ziolkowski
FachbereichPhysik,UniversitätSiegen,D-57068Siegen,Germany31
S. Bifani
1,
M. Clemencic
11,
S. Goy Lopez
32 DipartimentodiFisicadell’UniversitàeSezionedell’INFNdiTorino,I-10125Torino,ItalyC. Biino,
N. Cartiglia,
F. Marchetto
Sezionedell’INFNdiTorino,I-10125Torino,Italy
H. Dibon,
M. Jeitler,
M. Markytan,
I. Mikulec,
G. Neuhofer,
L. Widhalm
† ÖsterreichischeAkademiederWissenschaften,InstitutfürHochenergiephysik,A-10560Wien,Austria33a
r
t
i
c
l
e
i
n
f
o
a
b
s
t
r
a
c
t
Articlehistory:
Received11September2018
Receivedinrevisedform23November2018 Accepted26November2018
Availableonline29November2018 Editor:W.-D.Schlatter
TheNA48/2 experimentatCERN reportsthefirstobservationofthe K±→
π
±π
0e+e− decayfromanexposureof1.7×1011chargedkaondecaysrecordedin2003–2004.Asampleof4919candidateswith 4.9%background contamination allowsthe determination ofthe branchingratioin thefull kinematic region,B R(K±→
π
±π
0e+e−)= (4.24±0.14)×10−6.Thestudyofthekinematicspaceshowsevidenceforastructuredependentcontributioninagreementwithpredictionsbasedonchiralperturbationtheory. SeveralP- andCP-violatingasymmetriesarealsoevaluated.
©2018TheAuthor(s).PublishedbyElsevierB.V.ThisisanopenaccessarticleundertheCCBYlicense (http://creativecommons.org/licenses/by/4.0/).FundedbySCOAP3.
*
Correspondingauthors.E-mailaddresses:milena.misheva@cern.ch(M. Misheva),brigitte.bloch-devaux@cern.ch(B. Bloch-Devaux). † Deceased.
1 Nowat:SchoolofPhysicsandAstronomy,UniversityofBirmingham,Birmingham,B152TT,UK. 2 SupportedbyaRoyalSocietyUniversityResearchFellowship(UF100308,UF0758946). 3 FundedbytheUKParticlePhysicsandAstronomyResearchCouncil,grantPPA/G/O/1999/00559. 4 Nowat:UniversitàdegliStudidelPiemonteOrientaleeSezionedell’INFNdiTorino,I-10125Torino,Italy. 5 Nowat:IstitutodiCosmogeofisicadelCNRdiTorino,I-10133Torino,Italy.
1. Introductionandtheoreticalframework
Kaondecayshaveplayedamajorroleinestablishingthequark mixingflavourstructureoftheStandardModel[1].Radiativekaon decaysareofparticularinterest intestingmodelsdescribing low-energyquantumchromodynamics(QCD)suchasthechiral pertur-bationtheory (ChPT),an effectivefield theoryvalidbelowascale
O
(1GeV).The radiative decay K±
→
π
±π
0e+e−, never observedso far,proceeds through virtual photon exchange followed by internal conversion into an electron-positron pair, i.e. K±
→
π
±π
0γ
∗→
π
±π
0e+e−. The virtualγ
∗ can be produced by two differentmechanisms: Inner Bremsstrahlung (IB)where the
γ
∗ isemitted byoneofthechargedmesonsintheinitial orfinal state,and Di-rectEmission(DE)wheretheγ
∗isradiatedoffattheweakvertex. Consequently, the differential decayrate consistsof three terms: the dominant long-distance IB contribution, the DE component (electricEandmagnetic Mparts), andtheir interference.The in-terferencetermINTincludesthedifferentcontributions,IB-E,IB-M andE-M.TheIB-MandE-MtermsareP-violatingandcancelupon angularintegrationinthetotalrate.There are few theoretical publications related to the K±
→
π
±π
0e+e−mode[2–4] andnoexperimentalobservation.Theau-thorsof[3] predicted,onthebasisoftheNA48/2measurementof
6 Nowat:JointInstituteforNuclearResearch,141980Dubna(MO),Russia. 7 Nowat:DipartimentodiFisicaeScienzedellaTerradell’UniversitàeSezione dell’INFNdiFerrara,I-44122Ferrara,Italy.
8 Nowat:DepartmentofPhysics,ImperialCollege,London,SW72BW,UK. 9 Nowat:SchoolofPhysicsandAstronomy,TheUniversityofManchester, Manch-ester,M139PL,UK.
10 SupportedbyERCStartingGrant336581. 11 Nowat:CERN,CH-1211Genève23,Switzerland.
12 Nowat:FacultyofPhysics,UniversityofSofia“St.Kl.Ohridski”,BG-1164Sofia, Bulgaria,fundedbytheBulgarianNationalScienceFundundercontractDID02-22.
13 Alsoat:LaboratoriNazionalidiFrascati,I-00044Frascati,Italy.
14 Nowat:InstituteofNuclearResearchandNuclearEnergyofBulgarianAcademy ofScience(INRNE-BAS),BG-1784Sofia,Bulgaria.
15 Nowat:FermiNationalAcceleratorLaboratory,Batavia,IL60510,USA. 16 Nowat:CentredePhysiquedesParticulesdeMarseille,IN2P3-CNRS,Université delaMéditerranée,F-13288Marseille,France.
17 Nowat:SchoolofNaturalSciences,UniversityofCalifornia,Merced,CA95343, USA.
18 Nowat:SchoolofPhysics,AstronomyandComputationalSciences,George Ma-sonUniversity,Fairfax,VA22030,USA.
19 Nowat:PhysicsDepartment,UniversityofLancaster,Lancaster,LA14YW,UK. 20 AlsoatDipartimentodiScienzeFisiche,InformaticheeMatematiche,Università diModenaeReggioEmilia,I-41125Modena,Italy.
21 AlsoatIstitutodiFisica,UniversitàdiUrbino,I-61029Urbino,Italy.
22 FundedbytheGermanFederalMinisterforEducationandresearchunder con-tract05HK1UM1/1.
23 Nowat:SLAC,StanfordUniversity,MenloPark,CA94025,USA. 24 Nowat:NationalCenterforNuclearResearch,P-05-400´Swierk,Poland. 25 Nowat:UniversitàdiRoma“LaSapienza”,I-00185Roma,Italy.
26 Nowat:InstitutodeFísicaCorpuscularIFIC,UniversitatdeValència,E-46071 València,Spain.
27 Nowat:DipartimentodiFisicadell’UniversitàeSezionedell’INFNdiPadova, I-35131Padova,Italy.
28 Now at: Dipartimento di Fisica dell’Università e Sezione dell’INFN di Pisa, I-56100Pisa,Italy.
29 Nowat:DipartimentodiFisicadell’UniversitàdiTorino,I-10125Torino,Italy. 30 Nowat:InstitutdePhysiqueNucléairedeLyon,IN2P3-CNRS,UniversitéLyonI, F-69622Villeurbanne,France.
31 Fundedbythe GermanFederalMinisterforResearchandTechnology(BMBF) undercontract056SI74.
32 Nowat:CentrodeInvestigacionesEnergeticasMedioambientalesyTecnologicas, E-28040Madrid,Spain.
33 FundedbytheAustrianMinistryforTrafficandResearchunderthecontractGZ 616.360/2-IVGZ616.363/2-VIII,andbytheFondsfürWissenschaftundForschung FWFNr. P08929-PHY.
themagneticandelectrictermsinvolvedintheK±
→
π
±π
0γ
de-cay [5],thebranchingratiosofIB,DE andINTcomponentsofthe
K±
→
π
±π
0e+e− decay andposted recently a revised work [6]where the interference term is re-evaluated using more realistic inputsbasedonadditionalexperimentalresultsandfewer theoret-icalassumptions.
It is worth writing explicitly the various contributions to the squaredamplitudeofthedecay[3]:
spins|
M|
2=
2e 2 q4⎡
⎣
3 i=1|
Fi|
2Tii+
2Re 3 i<j(
Fi∗Fj)
Ti j⎤
⎦ ,
(1)where FiarecomplexformfactorsandTi j arekinematic
expres-sions(asdefinedin[3])whichdependonthefour-momentaofthe
e+e− systemandthe chargedandneutralpionsinthe kaonrest frame.Forconvenience,onealsowrites:
F1
=
F1I B+
F1D E,
F2=
F2I B+
F2D E,
F3=
F3D E.
(2)The form factors F1I B
,
F2I B include a strongphaseδ
02 correspond-ing to the S-waveand isospin 2 state of the dipion system. The complex formfactors F1D E,
F2D E correspond totheelectricpartof DE and make use of the ChPT counterterms NE(0,1,2) while FD E 3corresponds to the magnetic part of DE and makes use of the counterterm N(M0).Theseformfactorscarry astrongphase
δ
11 cor-respondingtotheP-waveandisospin1stateofthedipionsystem. Numericalvaluesofthecountertermswereestimated[6] using experimental measurements offormfactors intherelatedmodesK±
→
π
±γ
∗,KS→
π
0γ
∗andK±→
π
±π
0γ
.2. Kaonbeamlineanddetector
The NA48/2 experiment atthe CERN SPS was specifically
de-signed for charge asymmetry measurements in the K±
→
3π
decaymodes[7].Largesamplesofchargedkaondecayswere col-lected during the2003–2004 data takingperiod.The experiment beamline wasdesignedto deliversimultaneous narrow momen-tumband K+and K−beamsoriginatingfromprimary 400GeV/c protonsextractedfromtheCERNSPSandimpingingonaberyllium target. Secondary unseparated hadron beams with central
mo-menta of60 GeV/c anda momentumbandof
±
3.8%(rms) wereselected andbroughttoa commonbeamaxisby two systemsof dipole magnetswithzerototaldeflection(called“achromats”), fo-cusingquadrupoles,muonssweepersandcollimators.Thefraction of beamkaons decayingin the114 mlong cylindricalevacuated tankwas22%.
The momenta of chargeddecayproducts were measured in a magnetic spectrometer, housed in a tank filled with helium at nearly atmosphericpressure. The spectrometer was composed of pairs of drift chambers (DCH) on each side of a dipole magnet providing a momentum kick
p
=
120 MeV/c to charged parti-cles in the horizontalplane. The momentum resolution achieved wasσ
p/
p= (
1.
02⊕
0.
044·
p)
%(p inGeV/c).A hodoscope(HOD)consistingoftwo planesofplastic scintil-lators,eachsegmentedinto64strip-shapedcounters,followedthe spectrometer andprovided timemeasurements forcharged parti-cles with a resolution of150 ps. Grouping the counters of each plane ineight subsets, the HOD surface was logically subdivided into16exclusiveregionsproducingfastsignalsusedtotriggerthe detectorreadoutonchargedtracktopologies.
Further downstream was a liquid krypton electromagnetic
calorimeter (LKr), an almost homogeneous ionization chamber with an active volume of 7 m3, segmented transversally into
13248 projective 2
×
2 cm2 cells with no longitudinal segmenta-tion. The energies ofphotons andelectrons were measured withresolutions
σ
E/
E= (
3.
2/
√
E
⊕
9.
0/
E⊕
0.
42)
%.Thetransverse posi-tionsofisolatedshowersweremeasuredwithaspatialresolutionσ
x=
σ
y= (
0.
42/
√
E
⊕
0.
06)
cm, andtheshower time resolution was2.5ns/
√
E (E inGeV).Aniron/scintillatorhadronic calorime-terandmuondetectorswere locatedfurtherdownstream.Neither ofthemwasusedinthepresentanalysis.A dedicated two-level trigger was used to collect K± decays into three charged tracks with high efficiency: at the first level (L1),eventscontaining chargedtracks were selectedby requiring spaceandtime coincidencesofsignalsinthetwo HODplanesin atleasttwoofthe 16exclusiveregions;atthe secondlevel (L2), afarmofasynchronousmicroprocessorsperformedafasttrack re-constructionandranavertexfindingalgorithm.
Moredetails about thebeam lineand triggerimplementation canbefound in[7].Adetaileddescriptionofthedetectorcan be foundin[8].
3. Dataanalysis 3.1.Measurementmethod
The K±
→
π
±π
0e+e− decay rateis measured relative to thenormalizationdecay K±
→
π
±π
0 collectedconcurrently withthesame trigger logic. This method does not rely on an absolute kaonfluxmeasurement.Inthesignalsample, the
π
0 isidentifiedthroughthe
π
0→
γ γ
mode(
π
0γ γ
)
.Inthenormalizationsample,the
π
0 is identifiedthroughtheπ
0D
→
e+e−γ
Dalitz mode(
π
D0)
.Theratioofpartialrates(andbranchingratios)isobtainedas:
B R
(
K±→
π
±π
0e+e−)/
B R(
K±→
π
±π
0)
=
Ns−
Nbs Nn−
Nbn·
An×
ε
n As×
ε
s·
(
π
D0)
(
π
0 γ γ)
,
(3)whereNs
,
Nn arethenumbersofsignalandnormalizationcandi-dates;Nbs
,
Nbnarethenumbersofbackgroundeventsinthesignalandnormalizationsamples; Asand
ε
saretheacceptanceandthetriggerefficiencyforthesignalsample;Anand
ε
narethoseforthenormalizationsample.
The branching ratio of the normalization mode is B R
(
K±→
π
±π
0)
= (
20.
67±
0.
08)
% and the ratio ofπ
0 partial rates is(
π
0D
)/(
π
γ γ0)
= (
1.
188±
0.
035)
% [9]. Acceptances are obtainedfrom a detailed Monte Carlo (MC) simulation based on GEANT3 [10].The simulationincludesfull detectorgeometryandmaterial description,straymagneticfields,DCHlocalinefficienciesand mis-alignment,LKrlocalinefficiencies,accuratesimulationofthekaon beamlineandvariations oftheabovethroughoutthedata-taking period.
EfficienciesoftheL1andL2triggersaremeasuredfrom down-scaledcontrolsamples,recordedconcurrentlywiththethree-track trigger. The control trigger condition for the L1 efficiency mea-surementrequires atleast one coincidence of signalsin the two planesoftheHOD.ThecontroltriggersamplefortheL2efficiency measurementconsistsofL1triggersrecordedregardlessoftheL2 decision.Thetriggerdecisionisalsoavailableinthesimulationfor comparison.
3.2.Eventreconstructionandselection
ThestandardNA48/2softwarehasbeenusedincludingcharged track,LKrenergyclusterandthree-trackdecayvertex reconstruc-tion [7]. Fully reconstructed K±
→
π
±π
+π
− decays have been usedto monitorthe DCHalignment, the spectrometer field inte-gralandthe mean beampositionat each DCHplane throughout thedatataking.Signal and normalization candidates are reconstructed from threetracks: twosame-sign tracksandone opposite-chargetrack forming a commonvertex inthe fiducial decayvolume, the ver-tex charge being thereforeqvtx
= ±
1. The vertextime is definedas the average of the three HOD signal times associated to the tracks. The tracks are required to be in time within 5 ns of the vertextime.Theirimpactpointsarerequiredtobewithinthe ge-ometricalacceptanceofthedriftchambers.Inparticular,thetrack distancetothemonitoredbeampositioninDCH1planeisrequired tobelargerthan12cm.Thetrackmomentaarerequiredtobein therange(2–60)GeV
/
c andtrack-to-trackdistancesatDCH1tobe largerthan2 cmtosuppressphotonconversionstoe+e− pairsin theupstreammaterial.Configurationswherethethreeconsideredtracks,extrapolated totheHODfrontface,havetheirimpactpointsinasingle trigger region are rejected to avoidL1 inefficiencies of purely geometri-cal origin.Becauseofthedifferentkinematics,thisaffects2.3%of thesignalsampleandhasanegligibleeffectonthenormalization sample.
All vertices considered for further analysisare required to be reconstructedina98mlongfiducialvolume,starting 2m down-streamofthelastcollimatorexit,andwithin3 cmfromthebeam axis.
Photonclustersmatchingthevertextimewithin5 nsare con-sideredasphotoncandidatesiftheirenergyisintherange(3–60) GeV, their position is within the LKrgeometrical acceptanceand their distancetothenearestLKrinactivecell islargerthan2cm. Photon four-momenta are reconstructed assuming they originate fromthethree-trackvertex.Photontrajectoriesarerequiredto in-terceptthe DCH1plane ata radialposition largerthan 11cm to avoidpossibleinteractionswiththeDCHflangeresultingina de-gradedenergymeasurement.
Signal and normalization modes differ in their final state by one photon, whilesatisfyingsimilar kinematicconstraints onthe reconstructed
π
0 and kaon masses, although with differentres-olutions because of different numbers of participating particles.
The mass resolutions (Gaussian rms) obtained from the data
agreewiththose fromsimulationandare foundto be
σ
m(
π
D0)
1
.
7 MeV/
c2,
σ
m(
π
±π
D0)
4.
2 MeV/
c2andσ
m(
π
γ γ0)
2.
7 MeV/
c2,σ
m(
π
±π
γ γ ee0)
6.
1 MeV/
c2 for the normalization and signalmodes,respectively.
Very loose requirements are applied to the reconstructed masses, required to be within 15 MeV
/
c2 (45 MeV/
c2) from thenominal
π
0 (K±) mass[9], respectively, ensuring a minimalde-pendence of the selection on momentum or energy calibration effects,aswellasonanyresolutionmismatchesbetweendataand simulation.Acommonconstraint,takingintoaccount the correla-tionbetweenthereconstructedmπ0 andmK massesanddefined
as
|
mπ0−
0.
42·
mK+
72.
3| <
6(
all masses in MeV/
c2),
(4)contains more than 99% of the normalization events and about 96.5%ofthesignalevents.
In both modes, the single track with its charge opposite to
qvtxisconsideredtobeanelectron(positron).Theremaininge
/
π
ambiguity forthetwo same-sign tracks isthen solved by testing the two mass hypothesesagainst the full selection. When a par-ticular mass assignment is considered, an extra requirement on thedistanceofanyphoton cluster tothetrackimpactatthe LKr frontface isappliedtoguaranteephoton showerisolation, avoid-ing potential overlap with other showers: the distance between the photon position andthe electron and positron trackimpacts isrequiredtobelargerthan10cmandthedistancebetweenthe photonpositionandthepiontrackimpacttobelargerthan20cm.
ThisrequirementisenforcedonlyfortrackimpactswithintheLKr geometricalacceptance.
Noupperlimitonthenumberoftracksandclustersisset,all three-trackverticesbeingconsideredandcombinedwithany pho-tonclusterunderthetwopossiblee
/
π
masshypothesesuntilone combinationsatisfieseitherofthefollowingselections (normaliza-tionor signal)below, theeventbeingrejectedotherwise. Ifboth mass combinations are accepted, the one with the tighter con-straintofEq. (4) iskept.Normalizationselection The
π
0D candidateisreconstructed froma
pairofelectronandpositrontracksandaphotonoriginatingfrom the three-track vertex. The kaoncandidate is reconstructed from the
π
±π
0D system.
Theconsistencyofthefinal statewithakaondecayalongthe beamaxisischeckedfurtherby consideringtheenergy-weighted coordinates ofthe centreof gravity (COG)ofthe particles atthe LKrfront planecomputedfromthephotonpositionandthetrack extrapolations obtained from track parameters measured before the magnet (undeviated trajectories). The radial distance of the COGtothenominalbeampositionisrequiredtobesmallerthan 2 cm.Thepionmomentumisrequiredtobelargerthan10 GeV
/
cand the total momentum of the system to be in the beam
mo-mentum range (54–66) GeV
/
c. The e+e− massis required to be larger than 10 MeV/
c2 to ensure good agreement between dataandsimulation.Asampleof16316690candidatessatisfiesthe nor-malizationselectioncriteria.
Signalselection The
π
0γ γ candidateisreconstructedfromtwo
pho-tonsoriginatingfromthethree-trackvertex.Thekaoncandidateis reconstructedfromthe
π
±π
0e+e− system. The twophotonclus-tersarerequiredto beseparatedby morethan10 cm attheLKr front plane to avoid shower overlap. The event COG coordinates arethenobtainedincludingthetwophotonsandthethreecharged tracks,andsubjectedtothesamerequirementasabove.Thetotal momentumofthesystemisrequiredtobe inthebeam momen-tumrange(54–66) GeV
/
c.Thee+e− massisrequiredtobelarger than3 MeV/
c2.Twomainsourcesofbackgroundcontribute tothesignal final state: K±
→
π
±π
0γ γ
π
D0 (K3πD)where oneof thephotonsislost(ormergedwithanotherparticle),andK±
→
π
±π
0D
(
γ
)
(K2πDγ ),wheretheradiative photonandthe Dalitzdecayphoton mimica
π
0→
γ γ
decay. Suppression of the K3πD background eventsis
achieved by requiring the squaredmass of the
π
+π
0 systemtobe greaterthan 0.12
(
GeV/
c2)
2,exploitingthe largerphase spaceavailableinthesignalmode.Thiscutalonerejects94%oftheK3πD
simulated eventsand
∼
1% ofthe IB signal. To reject the K2πDγbackground,each ofthetwo possiblemassesmeeγ isrequiredto
bemore than7 MeV
/
c2 away fromthe nominalπ
0 mass(corre-spondingto about4
σ
ofthe massresolution). Asample of 4919 candidatessatisfiesthesignalselectioncriteria.3.3. Backgroundevaluation
The background processes contributing to the normalization mode (K2πD) are semi-leptonic decays followed by a Dalitz
de-cay ofthe
π
0: K±→
μ
±νπ
0D (Kμ3D) and K±
→
e±νπ
0 D (Ke3D),collectivelydenoted Kl3D,wherethe
π
D0 decayiscorrectlyrecon-structedbutthelepton(
μ
±,
e±)iserroneouslyattributedtheπ
+ mass.Theacceptances ofsuchprocesses inthenormalization se-lectionareO
(10−4)andobtainedfromlargesimulatedsamples.Foreachbackgroundprocess,thenumberofeventsNbn is
esti-matedrelativetothenumberofobservedeventsinthe normaliza-tionmodeNn usingtheacceptancesinthenormalizationselection
andtheworldaveragebranchingratios[9]:
Kl3D
:
Nbn/
Nn= (
AKl3D/
An)
·
B R(
Kl3D)/
B R(
K2πD)
(5)wherethetriggerefficienciescanceltofirstorderduetothe simi-lartopologies.
The number of backgroundevents in the signal selection Nbs
isestimatedrelativetothenumberofobservedeventsinthe nor-malization selection Nn and is obtained as in Eq. (5), using the
acceptancesinthesignalselection,both
O
(10−6):K3πD
:
Nbs/
Nn=
2× (
AK3πD/
An)
·
B R(
K3πD)
×
B R(
π
0→
γ γ
)/
B R(
K2πD),
(6)K2πDγ
:
Nbs/
Nn=
AK2πDγ/
An.
(7)Note the factor of two in Eq. (6) due to the two
π
0 mesons inthe K3πD mode.Anorderofmagnitudesmallercontributionfrom Ke3D isalsoconsidered.Inall contributionsbothbackgroundand
normalizationbranchingratiosincludethe
π
0Dalitzdecaypartialratewhosevalueanduncertaintycancelintheestimation.
4. Branchingratiomeasurement
Candidatesandbackground Samplesof16
.
3×
106K2πD candidates
and 4919 signal candidates have been selected froma subset of a 1
.
7×
1011kaondecayexposurein2003–2004. Thebackground estimatesfromsimulationamount to(10437±
119) Kμ3D eventsand(6851
±
106) Ke3D events inthe normalizationmode,corre-sponding to a total relative backgroundcontribution of 0.11%. In the signal mode, they amount to (132
±
8) events from K3πD,(102
±
19) events from K2πDγ and (7±
3) from Ke3D, addingup to arelative backgroundcontribution of(4.9
±
0.4)%.The re-constructedγ
e+e−(
γ γ
)
andπ
±π
0D (
π
±π
0e+e−) massdistribu-tionsaredisplayed inFig.1(Fig.2) fortheselectednormalization (signal)candidates.Backgroundandnormalization(signal) simula-tions, scaled tothenumber ofobservedcandidates,show a good agreementwiththedatadistributions.
Acceptances Because the selection acceptance is not uniform acrossthephasespace,itsoverallvaluedependsonthedynamics oftheconsideredprocess.TheacceptanceAn (3.981%)iscomputed
using the simulation of K±
→
π
±π
0 accordingto [11] followedby
π
0D decayaccordingtothemostrecent“Prague”radiativedecay
calculation[12].
TheMCsamplesforthedifferentK±
→
π
±π
0e+e−signalcon-tributionsIB,DEandINThavebeengeneratedseparatelyaccording to the theoretical description givenin [3,6]: the DE contribution consistsmainlyofthemagneticMterm,withtheEtermexpected to befifteentimeslower; theINT termincludes onlytheelectric interferenceIB-E,astheotherinterferencetermsIB-MandE-Mdo notcontributetothetotalrateinthelimitoffullangular integra-tion(Section1).Particularcarehasbeentakeninthegenerationof theIB-Etermwhichcontributesconstructivelyordestructively to thedifferentialratedependingonthekinematicspaceregion con-sidered. Thispropertyis illustratedinFig.3-left. Radiativeeffects areimplementedusingthe
PHOTOS
package[13].Global acceptances are obtained for each of the three main componentsofthesignalprocess:IB
(
0.
645±
0.
001)
%,M(
1.
723±
0.
003)
% and IB-E(
0.
288±
0.
001)
%. The signal acceptance As isthen obtained from a weighted average of the single-component acceptances,usingasweights,w,theirrelativecontributionstothe totalratewithrespecttoIBcomputedin[3,6]:
As
=
AIB
+
AM·
wM+
AIB-E·
wIB-E1
+
wM+
wIB-EFig. 1. Normalizationcandidates.Left:reconstructedγe+e−mass.Right:reconstructedπ±π0
D mass.Fulldotscorrespondtodatacandidates;stackedhistogramsare,from
bottomtotop,theexpectedKμ3D(green)andKe3D(blue)backgroundsmultipliedbyafactorof50tobevisible.Thenormalizationsimulation(red)includesradiativeeffects
inbothkaonandπ0
Ddecaysthatreproducetheasymmetrictailsofbothdistributions.
Fig. 2. Signalcandidates.Left:reconstructedγ γmass.Right:reconstructedπ±π0e+e−mass.Fulldotscorrespondtodatacandidates;stackedhistogramsare,frombottom
totop,theexpectedK3πD(green),K2πDγ (lightblue)andKe3D (darkblue)backgroundsandIBsignal(red)estimatedfromsimulation.Allquotederrorsarestatistical.
where wM and wIB-E are equalto 1/71and
−
1/
253 respectively.Theresulting signal acceptanceisobtainedas As
=
0.
9900 AIB+
0
.
0139 AM−
0.
0039 AIB-E= (
0.
662±
0.
001)
%.Both normalization and signal acceptances are obtained with respecttothefullmee kinematicrange.
Triggerefficiencies Trigger efficiencies are measured from control data samples for the normalization mode (L1:
(
99.
75±
0.
01)
%, L2:(
97.
66±
0.
04)
%)andcross-checkedagainst thesimulated es-timations (L1:(
99.
767±
0.
003)
%, L2:(
98.
495±
0.
006)
%) which providealso an accurate description oftheir time variations due tolocalandtemporary inefficienciesoftheHODorDCHs.Dueto thelow statistics ofthe signal candidate sample, it is not possi-bletoobtain thetriggerefficiencies fromthedownscaled control samples. Trigger efficiencies for the signal candidates are there-foreestimatedfromthesimulatedsamples(L1:(
99.
729±
0.
009)
%, L2:(
98.
604±
0.
021)
%)andnot affectedbyotherwiselargestatis-tical uncertainties. The full trigger efficiency in each selection is obtainedastheproductofL1andL2efficienciesthatarebasedon differentdetectorsandthereforeuncorrelated.
Systematicuncertainties Thestatisticaluncertaintiesonacceptance andtriggerefficiencyvaluesare accountedaspartofthe system-aticuncertainties.
Thecontrolofthegeometricalacceptancesisevaluatedby con-sideringthreeexclusiveregionsofthedecaylongitudinalposition (showninFig.3-right)withdifferentacceptancesandbackground conditionsforbothsignal andnormalizationchannels. The differ-ence betweenthe statisticalcombination ofthe three B R values
andtheglobalvalueisquotedassystematicuncertainty.
Thecontroloftheacceptancedependencewithtimeandkaon charge is quantified by considering four exclusive B R
quot-Fig. 3. AcceptancesoftheIB,MandIB-Ecomponentsprojectedalongthemee andthelongitudinal vertexposition Zvertex variables(the Z axisoriginislocated18m
downstreamofthelastcollimatorexit).FortheIB-Ecomponent,theacceptanceisformallyplottedwithanegative(positive)valuewhentheinterferenceisdestructive (constructive).Thearrowscorrespondtothethreeexclusiveregionsconsidered.
ingassystematicuncertaintythedifferencebetweenthestatistical combinationofthefourB R valuesandtheglobalvalue.
An evaluation of the background control level is obtained by tightening the constraintof Eq. (4) to reduce the background to signalcontributionfrom4.9%to3%whiledecreasingthesignal ac-ceptancebyarelativefractionof8%.Thequoteduncertaintycovers alsotheeffectoftheresidualdisagreementbetweendataand sim-ulatedreconstructedmasses.
Trigger efficiencies obtained from simulation are used in the
B R calculation.The difference betweenthe measured and simu-latedefficienciesofthenormalizationcandidatesisconsidered as asystematicuncertainty.
Themodeldependenceofthesignalacceptanceisinvestigated by varying in turn each input (N(M0)
,
N(E0,1,2)) within its theoreti-caluncertaintyestimate.Theresultingvariationsinacceptanceare addedinquadraturetoobtaintheoverall contributionto system-atics.Accordingtotheauthorsofthe
PHOTOS
package[14],the un-certainty on the photon emission implementation cannot exceed 10%ofthefulleffect(here4.
9×
10−2relativeinthesignalmode), which is quoted as systematic uncertainty. In the normalization mode,intheabsenceofanyprescriptionfromtheauthorsofthe “Prague”π
0D decayimplementation,10%ofthe0
.
53×
10−2relativedifference between the
PHOTOS
and“Prague” K2πD acceptancesis conservativelyassigned asa systematicuncertainty andadded quadratically to the signal
PHOTOS
uncertainty. The agreement betweendata andsimulationcan be judgedfrom themeedistri-butionsofFig.4.
Externalerrorsstemfromrelative errorson B R(K±
→
π
±π
0)andon
(
π
0D
)
/(
π
γ γ0)
.Table1summarizestheconsideredsourcesofuncertainty.
Result Thefinalresultisobtainedas:
B R
(
K±→
π
±π
0e+e−)
= (
4.
237±
0.
063stat±
0.
033syst±
0.
126ext)
×
10−6,
(9)wherethestatisticalerrorisdominatedbythesignalstatistics,the systematicerrorbytheradiative effectsandtheexternalerrorby the
π
0D branchingratiouncertainty.
This value can be compared to the predictions from [3,6]:
B R
(
K±→
π
±π
0e+e−)
=
4.
183×
10−6 for IB only, B R(
K±→
Table 1
Statistical, systematic and external uncertainties to the K±→
π±π0e+e− branchingratiomeasurement.The uncertainties
re-latedtothemodeldependenceandtoradiativeeffectscanalso beconsideredasexternalerrorsasbeingunrelatedtoourdata.
Source δB R/B R×102 Ns 1.426 Nbs 0.416 Nn 0.025 Nbn negl. Total statistical 1.486 As(MC statistics) 0.171 An(MC statistics) 0.051 ε(L1s×L2s) (MC statistics) 0.023 ε(L1n×L2n) (MC statistics) 0.007
Acceptance geometry control 0.083 Acceptance time variation control 0.064 Background control 0.280 Trigger efficiency (systematics) 0.400
Model dependence 0.285 Radiative effects 0.490 Total systematic 0.777 B R(K2π) 0.387 (π0 D)/(πγ γ0 ) 2.946 Total external 2.971
π
±π
0e+e−)
=
4.
229×
10−6 whenincludingallDEandINTterms.Theobtainedvalueiscompatiblewithbothpredictionswithinthe experimental errors.However itshouldbenotedthat noneofthe abovepredictionsincludesanyradiativeorisospinbreakingeffects.
5. Kinematicspacestudy
The current data statistics does not allow a precise enough measurementtoquantifythecontributionoftheDEmagneticterm Mtothetotaldecayrate(expectedtobeabout1%).However,the authorsof[3,6] havepointedoutthatthecontributionsofIB, mag-neticM,andinterferenceIB-Etermshavedifferentdistributionsin the Dalitz plot (T∗π ,Eγ )∗ for different ranges ofq2 values, where T∗π , E∗γ and q2 are the charged pion kinetic energy and the vir-tual photon energy in the kaon rest frame, and the e+e− mass squared, respectively. The differences remain relevant even after the analysis selection acceptanceis applied. A method based on
Fig. 4. Reconstructede+e− massdistributionfor thenormalization(left)andsignal(right)candidateswith thelowercutsof10and3 MeV/c2,respectively.Simulated backgroundandnormalization(signal)contributionsarealsodisplayed.
the population of 3d-boxes in the kinematic space (q2, T∗
π , E∗γ )
isusedtodeterminetherelativefractionofeachcomponentthat wouldadd upto reproducethedatasample population.Thedata 3d-spaceis first split into N1 slices along q2, then each slice is splitintoN2slicesalong T∗π andthenintoN3E∗γ slices, all with equalpopulations.TheresultisagridofN1
×
N2×
N3exclusive 3d-boxesofvariablesizebutidenticalpopulation.Thebackground contributionsandthevarioussimulatedsignalcomponentsare dis-tributedaccordingto thedata griddefinition,each resulting ina setof3d-boxes ofunequal population. Toaccount forthe poten-tially different sizes of the simulation samples, scale factorsρ
Mand
ρ
IB-EaredefinedastheratiosoftheIBtotheMandIBtotheIB-Esimulatedsamplesizes.
To obtain the fractions (M)/IB and (IB-E)/IB reproducing the data,a
χ
2estimatorisminimized:χ
2=
N1×
N2×N3 i=1
(
Ni−
Mi)
2/(δ
N2i+ δ
M2i),
(10)where Ni
(δ
Ni)
is the data population (error)and Mi(δ
Mi)
theexpectedpopulation(error)inboxi.Thedenominatorofeachterm isdominatedbythenumberofdataevents
δ
N2i
=
Ni,thesameineachbox.Theexpectednumberofeventsinboxi iscomputedas:
Mi
=
N× (
NiIB+
a·
NMi+
b·
NIB-Ei)
+
N Bkgi
,
(11)whereN is aglobalscalefactortoguaranteethat thesumofthe simulated events andbackground contributions is normalized to thetotalnumberofdatacandidates.Attheendofthe minimiza-tion,theobtainedvaluesofa andb canberelatedtotherelative contributions(M)/IBand(IB-E)/IBby:
(
M)/IB= (
a± δ
a)/
ρ
M,
(IB-E)/IB= (
b± δ
b)/
ρ
IB-E.
(12)Themethodhasnosizeabledependenceontheprecisegrid struc-tureaslong asthe granularityensures sensitivity to the popula-tionvariation within theresolution(at least3q2 slicesand5or
6 slices along the two other variables) and large enough statis-tics per box to consider Gaussian errors. The grid configuration 3
×
5×
6 has been employed and the resultsare obtainedwith aχ
2 probability of 19% for a value of 98.2/87 degrees offree-dom anda correlation C
(
a,
b)
=
0.
06.The obtainedvalue (M)/IB =0.
0114±
0.
0043stat isconsistent withthe predictedvalue from[3], 1
/
71=
0.
0141±
0.
0014ext, obtained using the experimentalmeasurementof N(M0).The (IB-E)/IBvalue of
−
0.
0014±
0.
0036statshows that there is no sensitivity to this contribution within the current data statistics and agrees with the value from [6],
−
1/
253= −
0.
0039±
0.
0028ext, obtained using experimentalin-putstoN(E0,1,2)values.Theexternalerrorsonthepredictedvalues stemfromtheuncertaintiesofthemeasurementsusedasinputin theevaluations.
6. Asymmetryinvestigations
Electroweak (or beyond Standard Model) phases change sign underchargeconjugationwhenswitchingfrom K+ to K−,unlike the strongphase
δ
= δ
20− δ
11 that governsthe final state interac-tionofthepionsystem.Thesephasescanbeinvestigatedthrough asymmetriesbetweenK+andK−partialrates.ThesimplestCP-violatingasymmetry isthecharge asymmetry betweenK+andK−partialratesintegratedoverthewholephase space:
AC P
=
(
K+→
π
+π
0e+e−)
− (
K−→
π
−π
0e+e−)
(
K+→
π
+π
0e+e−)
+ (
K−→
π
−π
0e+e−)
.
(13)Thevalueof AC P canberelatedtotheinterferenceIB-Etermand
isproportionaltosin
δ
sinE,where
E isapossibleCP-violating
phaseappearingintheformfactorsF1D E,F2D Einaddition (subtrac-tion)tothestrongphase
δ
11(Section1).Theasymmetryisobtained from the statistically independent measurements of K+ and K−branching ratios,that takeinto accountthepossible biases intro-ducedbythedetectoracceptances.Thevalues
B R
(
K+)
= (
4.
151±
0.
078stat)
×
10−6,
B R
(
K−)
= (
4.
394±
0.
108stat)
×
10−6 (14)leadto AC P
= −
0.
0284±
0.
0155,wheretheerrorisstatisticalonly,asthesystematicandexternalerrorscancelintheratio.Thisvalue isconsistentwithzeroandistranslatedtoasingle-sidedlimit:
Other asymmetries are defined in [3] using the so-called Cabibbo-Maksymowicz[15] variables34 to describe the kinematic spaceofthe decayandselecting particularintegration regions of the
φ
angularvariable:AφC P∗
=
2π 0 d(K+−K−) d
φ
dφ
∗ 2π 0 d(K++K−) d
φ
dφ
,
where 2π 0 dφ
∗≡
⎡
⎢
⎣
π/2 0−
π π/2+
3π/2 π
−
2π 3π/2⎤
⎥
⎦
dφ,
(16) AC P˜φ=
2π 0 d(K+−K−) d
φ
d˜φ
2π 0 d(K++K−) d
φ
dφ
,
where 2π 0 d˜φ ≡
⎡
⎢
⎣
π/2 0+
π π/2−
3π/2 π
−
2π 3π/2⎤
⎥
⎦
dφ.
(17)These asymmetriescan be obtainedby combiningthe branching ratios measured in various parts of the
φ
variable space. Defin-ing sectors of theφ
space between 0 and 2π
as1
(
0,
π
/
2)
,2
(
π
/
2,
π
)
,3
(
π
,
3π
/
2)
and4
(
3π
/
2,
2π
)
, and combin-ing them as statistically independent sector sums (13
=
1+
3
,
24
=
2+
4)and(12
=
1+
2,
34
=
3+
4)one canobtaintheaboveasymmetries.The
φ
∗ integralhastheinteresting propertyofsubtractingthe contribution of sector sum24 from the contribution of sector sum
13. The interference termIB-M (Section 1) equally popu-lates sectors
1 and
3 when positive anddepopulates sectors
2 and
4 when negative. The AφC P∗ asymmetry is then related tothe interferenceIB-Mtermandisproportional tocos
δ
sinM,
where
M isapossibleCP-violatingphaseappearing intheform
factor F3D E (Section1). The interference IB-M termhas not been generatedinthesimulationasitisnotexpectedtocontribute sig-nificantlytothe totalrate. Howeverithasbeen checkedthatthe wholerangeof the
φ
variableisalways considered inthe accep-tancecalculation,apart fortheregionq2<
3 (MeV/c2)
2 excluded fromthesignalselection. TheCPasymmetries definedinEq. (16,17)aremeasured,althoughtoalimitedprecisiongiventhecurrent datastatistics,as:
AφC P∗
=
0.
0119±
0.
0150stat and AC P˜φ=
0.
0058±
0.
0150stat.
(18)
Allasymmetriesareconsistentwithzero,single-sidedupperlimits canbesetas
|
AφC P∗| <
3.
11×
10−2,
|
AC P˜φ| <
2.
50×
10−2at 90% CL.
(19)34 For K± decays,the variables arethe squaredinvariant dipion and dilepton
masses,theangleoftheπ±(e±)inthedipion(dilepton)restframewithrespect totheflightdirectionofthedipion(dilepton)inthe K± restframe,theangleφ betweenthedipionanddileptonplanesinthekaonrestframe.
Following another prescriptionof [3], a long-distance P-violating
asymmetrydefinedas A(PL)
=
2π 0 dd
φ
dφ
∗ 2π 0 dd
φ
dφ
=
(
13)
− (
24)
(20)
can be obtainedfrom the asymmetry between sector sums
13 and
24 when considering K+ or K− alone, and combined if found consistent. The A(PL) asymmetry isproportional to N(M0) [3] andsin
δ
.Aprecise A(PL) measurementwouldallowacheckofthe signofN(M0)andameasurementofsinδ
.Ourdataleadto A(PL)
(
K+)
=
0.
0059±
0.
0180stat andA(PL)(
K−)
=
−
0.
0166±
0.
0237stat, both consistent with zero. The combinedvalueis A(PL)
(
K±)
= −
0.
0023±
0.
0144stat.Theerrorsarestatisticalonly as both systematic and external uncertainties cancel in the ratios.Thisvaluecanbetranslatedintoasingle-sidedupperlimit:
|
A(PL)| <
2.
07×
10−2at 90% CL.
(21) 7. ResultsandconclusionThe data sample recorded by the NA48/2 experiment in
2003–2004 has been analyzed, searching for the unobserved
K±
→
π
±π
0e+e− decaymode inan exposureof1.
7×
1011kaondecays.Asample of4919decaycandidateswith4.9%background has been identified, resulting in the first observation of this de-cay mode.The branchingratiohasbeenmeasured relativeto the
K±
→
π
±π
0 modefollowed byaDalitz decayπ
0D
→
e+e−γ
andfound to be
(
4.
237±
0.
063stat±
0.
033syst±
0.
126ext)
×
10−6, inagreementwithpredictionsfromChPT.
Despitethelimitedstatisticsavailable,astudyofthekinematic spaceofthedecayhasbeenperformedtoextract informationon thefractionofmagnetic(M)andinterference(IB-E) contributions with respect to inner bremsstrahlung (IB). The relative contribu-tion,(M)/IB
= (
1.
14±
0.
43stat)
×
10−2,isfoundconsistentwiththetheoreticalexpectationof
(
1.
41±
0.
14ext)
×
10−2.TherelativeIB-Econtribution,(IB-E)/IB
= (−
0.
14±
0.
36stat)
×
10−2,isalsoinagree-ment with the prediction of
(
−
0.
39±
0.
28ext)
×
10−2 but withlimited significancedue to the lackof data statistics inthe high
mee region.
Several CP-violating asymmetries and a long-distance P-vio-latingasymmetryhavebeenevaluatedandfoundtobe consistent with zero, leading to upper limits
|
AC P|
<
4.
8×
10−2,
|
Aφ∗ C P
|
<
3.
1×
10−2,
|
A˜φ C P|
<
2.
5×
10−2,
|
A (L) P|
<
2.
1×
10−2at90%CL.If larger data statistics becomes available (for example at the NA62 experiment),more detailed studies of the kinematic space willallowforanimprovedevaluationoftheDEtermcontribution. A studyofthe P-violatingasymmetrycould bring informationon the signofthe DE magnetictermand onthe strongphase
δ
in-volvedinthefinalstateinteractionofthetwopions.Acknowledgements
WegratefullyacknowledgetheCERNSPSacceleratorandbeam linestafffortheexcellent performanceofthebeamandthe tech-nical staff of the participating institutes for their efforts in the maintenance andoperation of the detector, anddata processing. We thank M. Koval for making the “Prague” radiative
π
0 Dalitzdecay code available in the NA48/2 simulation software. Discus-sions with G. D’Ambrosio and O. Catà were most stimulating in clarifyingtheimpactofinterferencetermsonourmeasurement.
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