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1V.Patera CERN seminar 28 March 2006
[nb]
s [MeV]
Recent results of KLOE Recent results of KLOE at DAat DANENE
V.Patera Rome I University &
Laboratori Nazionali di Frascati (INFN)
V.Patera CERN seminar 28 March 2006
DaphneDaphne DANE(Greek , English laurel, Italian
alloro)daughter of the river god Peneios and
Gaea (goddess of the earth) flew the
courting of Apoll and was metamorphosed into
laurel by her mother; later on the name of
this plant was attributed to Apoll not to be confused with DaphnisDaphnis
– son of Hermes (Mercurius) and a Sicilian nymph
ChloeChloe KLOE – the greening, is a surname of
Demeter (Ceres) Daphnis and ChloeDaphnis and Chloe
– couple of lovers in the hononymous novel
of Logos (~300 a.C.)– made famous by Ravel symphonic
poem
DADANE & KLOE : the NE & KLOE : the originorigin
3V.Patera CERN seminar 28 March 2006
OutlineOutline
Physics @ peak DANE, the frascati
factory The KLOE detector KLOE recent results:
Kaon physics (mostly)Non Kaon physics
Future of KLOE & DANE Summary and conclusions
Recent results → 2005-2006
V.Patera CERN seminar 28 March 2006
Physics at a Physics at a -factory (I)-factory (I)Not only KAON physics
Vus , Medium-Rare KS,L decays, CPT
with Ks , KL charge asymmetries,
Quantum Interferometry, But
also: hadronic cross section ,
radiative decays. “Natural”
luminosity unit: fb-1
A factory is a collider e+e-
running at s = M= 1.02 GeV
(1020)
a0(980)
f0(980)
'
KK
0-
0- 1-
1-
0+
0+
BR 83%
BR
15%
BR 1.3%
decay Produced ev/fb-1
K+K- 1.5x109
KLKS 1.0x109
5x107
’ 2x105
5V.Patera CERN seminar 28 March 2006
KSKL and K+K- pairs are produced in a pure quantum state (JPC=1--) :
decay ~at rest. Detection of a KS (KL) guarantees the presence of a KL(KS) with known momentum and direction (the same for K+K)
Extensively study all the possible decay channels with a multipurpose detector
Physics at the Physics at the -factory (II)-factory (II)
Kaon physicsKaon physics
pppp ,,,,2
1SLSL KKKKi
# precision measurement of absolute BR’sprecision measurement of absolute BR’s#interference measurements in Kinterference measurements in KSS K KLL systemsystem
#unique feature is the production of pure unique feature is the production of pure and and quasi monochromatic Kquasi monochromatic KSS, K, KLL, K, K++ and K and K-- beamsbeams
BR( K +K ) = 49.2%
BR(K0K0) = 33.8%
6V.Patera CERN seminar 28 March 2006
Physics at the Physics at the -factory (III)-factory (III)
Radiative decays ( ) M to probe the quark structure of the meson M
Hadronic cross-section measurement using the Initial State Radiation to vary the energy: e+ e
ss
a0
f0
qqqq vs qq
s’
ISR
’ mixing angle
Non-kaon physics Non-kaon physics
For the theoretical estimate of the hadronic contribution (aa
hadrhadr) to the anomalous magnetic moment of the muon (a) down to the down to the threshold energy for threshold energy for production production
7V.Patera CERN seminar 28 March 2006
OutlineOutline
Physics @ peak DANE, the frascati
factory The KLOE detector KLOE recent results:
Kaon physics (mostly)Non Kaon physics
Future of KLOE & DANE Summary and conclusions
V.Patera CERN seminar 28 March 2006
DADANE: the Frascati NE: the Frascati -factory-factory
• ee collider @ s = M= 1019.4 MeV
• 2 interaction regions (KLOE – DEAR/FINUDA)• Separate e, e rings to minimize beam-
beam interactions
• Crossing angle: 12.5 mrad ( px12.5
MeV )
V.Patera CERN seminar 28 March 2006
DADANE: the Frascati NE: the Frascati -factory-factory
• 105+105 bunches
• 2.7 ns bunch
spacing
• I-peak ~ 2.4 A
• I+peak ~ 1.5 A
• Injection during
data taking
10V.Patera CERN seminar 28 March 2006
DANE 24h Performance (Dec. 05)
1.2e-32
8 pb-1
e-
e+ 1 A
2 A
11V.Patera CERN seminar 28 March 2006
s monitored to within 70 keV
Some variations in 2004
Stable (1019.3-1019.6) in 2005
DADANE: energy stabilityNE: energy stability
2004
2005
s (
MeV
)s
(M
eV
) Run number
Run number
IP position, spot
size and s
monitored on line
by bhabha and KK
events
V.Patera CERN seminar 28 March 2006
KLOE@DAKLOE@DANE: the data NE: the data samplesample
Data taking finished
march 2006
• Lpeak= 1.3 × 1032
cms
• Integrated L 2.5 fb-1
• 200 pb-1 off-peak
2001 170 pb-1
2002 280 pb-1
Analysis nearly
complete
2004 734 pb-1
2005 1256 pb-
1
analysis
ongoing
13V.Patera CERN seminar 28 March 2006
OutlineOutline
Physics @ peak DANE, the frascati
factory The KLOE detector KLOE recent results:
Kaon physics (mostly)Non Kaon physics
Future of KLOE & DANE Summary and conclusions
V.Patera CERN seminar 28 March 2006
Be beam pipe (spherical, 10 cm , 0.5 mm thick) + instrumented permanent magnet quadrupoles (32 PMT’s)
Drift chamber (4 m 3.75 m, CF frame) Gas mixture: 90% He + 10% C4H10
12582 stereo–stereo sense wires almost squared cells
Electromagnetic calorimeter lead/scintillating fibers (1 mm ), 15 X0
4880 PMT’s 98% solid angle coverage
Superconducting coil (B = 0.52 T)
The KLOE design was driven by the measurement of direct CP through the double
ratio:
R = (KL +) (KS 00) / (KS +)(KL00)
KLOE experiment
V.Patera CERN seminar 28 March 2006
The KLOE Calorimeter:The KLOE Calorimeter:
9
σ(E)/E = 5.7%/E(GeV)
σ(t) = 54 ps/E(GeV) 50 ps
ε 95% for 20 MeV photons
vtx() ~ 1.5 cm (from KL
)
Lead
• Pb-scintillating fibers matrix: <ρ> ~ 5 g/cm3, <X0>~ 1.6 cm• 4880 PMTs• 98% hermetic coverage
V.Patera CERN seminar 28 March 2006
The KLOE Drift Chamber:The KLOE Drift Chamber:
p/p = 0.4 % (tracks with > 45°)
xhit = 150 m (xy), 2 mm (z)
xvertex ~ 1 mm
(M) ~1 MeV (from KS→)
Drift ChamberDrift Chamber
• 90% He, 10% iC4H10 ( X0=900m )
• 12582 stereo sense wires
• structure in C-Fibre (<0.1 X0)
• Non saturated drift velocity
• 2x2 (inner) & 3x3 (outer) cm2
squared cell size
17V.Patera CERN seminar 28 March 2006
OutlineOutline
Physics @ peak DANE, the frascati
factory The KLOE detector KLOE recent results:
Kaon physics (mostly)Non Kaon physics
Future of KLOE & DANE Summary and conclusions
18V.Patera CERN seminar 28 March 2006
K physics at KLOE - taggingK physics at KLOE - tagging
pppp ,,,,2
1SLSL KKKK
Tagging: observation of KS,L signals presence of KL,S ; K+ signals K
pure JPC = 1state
KS, K KL, K BR decay mode
34.1%
KSKL
49.1%
KK
absolute branching ratio measurement: BR=(Nsig/Ntag)(1/εsig)
K+K = 0.245 p* = 127 MeV/c ±= 95 cm
KLKS = 0.22
p* = 110 MeV/cS = 6 mm; L = 3.4 m
The decay at rest provides monochromatic and pure beam of kaons
Clean , normalized K+,K-,KL and KS beams (KS unique!!)
Kaon momentum is measured with 1 MeV resolution (e.g. p(KL) = p()- p(KS))
19V.Patera CERN seminar 28 March 2006
Neutral KaonsNeutral Kaons KS semileptonic decays KS → decay
KL dominant BR’s KL lifetime KLe3 form factor slopes KL → -+ and ε
KL,KS and Bell-Steinberger KL,KS Quantun Interferometry
20V.Patera CERN seminar 28 March 2006
Tagging of KTagging of KS S KKLLbeamsbeams
ε ~ 70% (mainly geometrical)KL angular resolution: ~ 1°KL momentum resolution: ~ 1 MeV
KKSS
KKLL 2 2
ε ~ 30% (largely geometrical)KS angular resolution: ~ 1° (0.3 in )KS momentum resolution: ~ 1 MeV
KKLL “crash”“crash”=0.22 =0.22 (TOF)(TOF)
KKSS ee
KKLL tagged tagged by Kby KSS vertex at IP vertex at IP
KKSS tagged tagged by Kby KLL interaction in interaction in EmCEmC
21V.Patera CERN seminar 28 March 2006
Analysis of KAnalysis of KSS →→ee decays decays
e
Data MC fit e bad bad
other
50 5000
100
200
300
400
500
600
700
Emiss(e) pmiss (MeV)100150
Even
ts/M
eV
Fit distributions of 5 variables in data with various MC sources including e and processes
e
Event selection Event selection (410 pb(410 pb-1-1 ) )
Obtain number of signal Obtain number of signal events from a constrained events from a constrained likelihood fit of multiple data likelihood fit of multiple data distributionsdistributions
Normalize using Normalize using KKSS events in same data setevents in same data set
• KS tagged by KL crash
• 2 tracks from IP to EMC
• Kinematic cuts to reject
background from KS →
• Track-cluster association
• e/ ID from TOF
• Identify the charge of final state
22V.Patera CERN seminar 28 March 2006
KKSS ee decay – Results decay – Results
BR(KS e+) = (3.529 0.057 0.027) 10-4
BR(KS e-) = (3.518 0.051 0.029) 10-4
BR(BR(ee)) [KLOE ’02, Phys.Lett.B535, 17 pb1]:(6.91 0.34stat 0.15syst) 10-4
BR(KBR(KSS ee) = (7.048 ) = (7.048 0.076 0.076statstat 0.050 0.050systsyst))1010-4-4
Accepted by PLB
Accepted by PLB
Charge asymmetryCharge asymmetry
With 2.5 fb1: AS 3 103 2 Re
Linear form factor slope Linear form factor slope + = (33.8 4.1) 10-3
In good agreement with linear fit from KL semileptonic form factor [ ( 28.6 0.6)×10
AS=AL if CPT and S=QAS AL signals CPT in mixing and/or decay with SQAS-AL=4Re()if CPT holds in decays with SQ
AASSee = (1.5 = (1.5 9.6 9.6 2.9) 2.9)1010-3-3
→ε→ε→ε→ε
A=→ε→ε
A=
23V.Patera CERN seminar 28 March 2006
KKSS ee: CPT test: CPT test
AS = 2(Re ε Re Re y Re x)
AL = 2(Re ε Re Re y Re x)CPT indecay
CPT inmixing
CP S Q and CPT
Sensitivity to CPT violating effects through charge asymmetry
M11M22 i
mS mL iSL
1
2
(KS,L -e+) (KS,L +e-)
(KS,L -e+) (KS,L +e-)AS,L =
AS AL 0
violates CPT
AL = (3.322 0.058 0.047) 10-3 , KTeV 2002
14
1
LS
SL
eKBR
eKBRx
24V.Patera CERN seminar 28 March 2006
KKSS →→ee : results : results
Test of S = Q rule
(x+) = ( 0.4 3.1 1.8) × 10(x+) = ( 0.4 3.1 1.8) × 10
Factor 2 improvement w.r.t. current most precise measurement(CPLEAR, )
(KS) PDG
(KL) PDG + KLOE ’05 (avg.)BR(KL→e) KLOE
Test of CPT and S Q:
(x) = ( 0.2 2.4 0.7) × 10(x) = ( 0.2 2.4 0.7) × 10
Factor 5 improvement w.r.t. current most precise measurement (CPLEAR, )
AL KTeV
() CPLEAR
Test of S = Q rule
(KS) = 89.58 0.06 psPDG
(KL) = 51.01 0.20 nsPDG + KLOE ’05 (avg.)
BR(KLe3)
0.40
0.39
KTeV ’04
KLOE ’05
PDG ’04
KLOE KS assuming S = Q
Accepted by PLB
Accepted by PLB
25V.Patera CERN seminar 28 March 2006
KKSS : first observation: first observation
EmissPmiss (MeV)40-40 0 20-20
2002 Data
KS + +
• Measurement never done before
• More difficult than KSe3:
1) Lower BR: expect
2) Background events from
KS : same
PIDs of the signal• Event counting from the fit to Emiss()
Pmiss distribution:
3% stat error
• Efficiency estimate from KL early decays and from MC + data control samples.
V.Patera CERN seminar 28 March 2006
KKSS 000000 – test of CP and CPT – test of CP and CPT
KS 30 is purely CP violating
If CPT conserved, S = L |εε’000|2
BRSM(KS 30) = 1.9 × 109
Best previous result from direct search:
BR < 1.4 × 105 90% CL [SND ’99]
BR< 7.4 107 [interference, NA48, ‘04]
Signature (εpresel ~ 14%):
KL crash + 6 ’s, no tracks from IP
Background rejection:
KS + 2split/accidental clusters
• MC 3 (BR 105)• MC 2
Define signal box in 23 vs.2
2 plane:
3 cluster pairs with best0 mass estimates
2 best cluster pairs - 0 masses, E(KS), p(KS), angle between0’s
V.Patera CERN seminar 28 March 2006
Nbkg(MC) = 3.13 ± 0.82 ± 0.37
Nobs = 2
KLOE 450 pb1 ’01+’02 data
BR < 1.2 × 107 90% CL
Prospects for 2.5 fb1:
• 6.5 increase in statistics
(L efficiency)
• 1.5 decrease in background
Potential to reduce limit ~10
MC
Eff. Stat. =
5.3 data
450 pb1
’01+’02 data
KKSS 000000 (II) (II)
PLB 619
(2005)
350 pb-1
28V.Patera CERN seminar 28 March 2006
Dominant KDominant KLL branching ratios branching ratiosAbsolute BR measurements to 0.5-1%Absolute BR measurements to 0.5-1%from 328 pb-1 data sampleKL tagged by KS :
• 13106 for the measurement• 4106 used to evaluate
efficienciesBR’s to e, , and +-0:
• KL vertex reconstructed in DC
• PID using decay kinematics
• Fit with MC spectra including radiative processes and optimized
EmC response to //KL
BR to 000:
• Photon vertex reconstructed by
TOF using EmC (3 clusters)
• εrec = 99%, background < 1%
Lesser of pmissEmiss in or hyp. (MeV)
29V.Patera CERN seminar 28 March 2006
Dominant KDominant KLL BR’s and K BR’s and KLL lifetime lifetime Using the constraint BR(KL) = 1 we get:
BR(KBR(KLLee) = 0.4007 ) = 0.4007 0.00060.0006statstat
0.00140.0014systsyst
BR(KBR(KLL) = 0.2698 ) = 0.2698 0.00060.0006statstat
0.00140.0014systsyst
BR(KBR(KLL 3 3) = 0.1997 ) = 0.1997 0.00050.0005statstat 0.00190.0019systsyst
BR(KBR(KLL) = 0.1263 ) = 0.1263 0.00050.0005statstat
0.00110.0011systsyst
Lifetime indirect measurement:Lifetime indirect measurement: LL= 50.72 = 50.72
0.170.170.330.33nsns
L/c (ns)
6 - 24.8 ns40-165 cm
0.37 L
x102
Eve
nts/
0.3
ns
PK = 110 MeVExcellent lever arm
for lifetime measurement
Lifetime direct measurement Lifetime direct measurement [PLB 626 (2005)][PLB 626 (2005)] : : LL = 50.92 = 50.92 0.17 0.17 0.25 ns 0.25 ns
KKLL lifetime, KLOE average lifetime, KLOE average : LL = 50.84 = 50.84 0.23 ns 0.23 ns Vosburg, ’72: L = 51.54 ± 0.44 nsKKLL lifetime, KLOE average lifetime, KLOE average : LL = 50.84 = 50.84 0.23 ns 0.23 ns Vosburg, ’72: L = 51.54 ± 0.44 ns
LL direct measurement from direct measurement from KKLL 400 pb400 pb11))
•Require 3 ’s• ε(LK) ~ 99%, uniform in L•L() ~ 2.5 cm•Background ~ 1.3%Use KL π+π-π0 for: •EmC time scale
•Photon vertex efficiency
[PLB 632 (2006)]
30V.Patera CERN seminar 28 March 2006
KKLe3 Le3 form factor slopes form factor slopes(*) IS
TR
A+
m /m
0 correction
Phase space integral
Pole model versus Quadratic parameterization:• KLOE: 0.5 per mil difference• KTeV: 6 per mil difference.
103 103 2/dof
e 24.6 2.1 1.9 1.0 152/180e 26.4 2.1 1.0 1.0 173/180All 25.5 1.5 1.4 0.7 325/362
= (25.5 1.5 1.0) 103
= ( 1.4 0.7 0.4) 103
Correlation: (, ) = 0.95
Quadratic fit
Pole model MV = 870(7) MeV
• 328 pb1, 2 106 Ke3 decays
• Kinematic cuts + TOF PID to reduce background ( ~ 0.7% final contamination )• Separate measurement for each charge state (e, e) to check systematics• t measured from and KL momenta: t/m
2 0.3
103 2/dof
e 28.7 0.7 156/181e 28.5 0.6 174/181All 28.6 0.5 330/363
= (28.6 0.5 0.4) 103
Linear fit
Accepted by PLB
Accepted by PLB
V.Patera CERN seminar 28 March 2006
BR KBR KLL
Decay CP violating Related to
εK KL beam tagged by KS →
328 pb-1 ’01+’02 data
Selection
• KL vertex reconstructed in DC
• PID using decays kinematics
• Fit with MC spectra including
radiative processes
Normalize using KL
events
(MeV) )( 22missmiss pE BR(KL )= (1.963 0.012 0.017) 10-3
Submitted to PLB
Submitted to PLB
V.Patera CERN seminar 28 March 2006
• KLOE in agreement with KTeV
[PRD70 (2004),092006]
BR=(1.975 0.012)
• confirm the discrepancy
(4 standard deviations) with
PDG04
PDG2004
KTeV
KLOE preliminary
BR
(KL
)
10
-3
agreement with prediction from Unitarity Triangle (1.5)
Using BR(KS ) and L
from KLOE and S from PDG04 ε| = (2.216 0.013) 10-3
|ε| PDG04 = (2.280 0.013)10-3
BR KBR KLL and and llεε ll
33V.Patera CERN seminar 28 March 2006
Measurements of KS KL observables can be used for the
CPT test from unitarity :
f(1 + i tan SW) [Re εi Im ] A*(KS f ) A(KL f )
S
1ff
KS
00KS
KS
kl3 SL B(KLl3) ReεRe yi( ImIm
x)
SL B(KLl3) (AS+AL)/4 i( ImIm
x)SL
KL
SL KL
CPT test: Bell-Steinberger CPT test: Bell-Steinberger relationrelation
f = A(KL →f)/A(KS →f)
34V.Patera CERN seminar 28 March 2006
KSK
S
KS
KL
KLl
KS
KL
KS
SW= (0.759±0.001)
CPT test: inputs to the Bell-Steinberger CPT test: inputs to the Bell-Steinberger relationrelation
S 0.08958 ± 0.00006 ns
L= 50.84 ± 0.23ns
AL
AS
KL
KL
=0.757 ± 0.012= 0.763 ± 0.014Im x
+ = (0.8 ± 0.7) 10-2KLOE measurements
Im xfrom a combined fit of KLOE + CPLEAR data
35V.Patera CERN seminar 28 March 2006
Re ε Im
Re ε Im
CPLEAR: Re ε Im
KLOE preliminary:
Re ε
Im
CPT and Bell-Steinberger: CPT and Bell-Steinberger: resultresult
Im
- Uncertainty on Im is now dominated by and
- Semileptonic sector contributes by ~ 10%
V.Patera CERN seminar 28 March 2006
no simultaneous decays (t=0) in the samefinal state due to thedestructive quantum interference
t/S
I(t
) (a
.u)
mfrom here
cos2;, 2/ tmeeetI ttt LSSL
Kaon interferometry: KSKL
t2 t1
t=t1-t2
Perfect vertex reolution
V.Patera CERN seminar 28 March 2006
KSKL
• Analysed data: L=380 pb
• Fit including t resolution and efficiency effects + regeneration• S, L fixed from PDG
KL regeneration on beam pipe
Data
Fit result
KLOE PRELIMINARY
m = (5.34 0.34) 109 s1
At 2.5 fb-1 m 0.14 109 s1
PDG ’04: (5.290 0.016) 10 s1
Best (Ktev’03)(5.288 0.043) 10 s1
V.Patera CERN seminar 28 March 2006
tKKtKK
tKKtKKtI N
0000
200
200
2
,,2
,,;,
• Fit including t resolution and efficiency effects + regeneration• S, L m fixed from PDG
From CPLEAR data, Bertlmann et al. (PR D60 (1999) 114032) obtain:
KLOE preliminary result:with 2.5 fb-1 :
KSKL: test of quantum coherence
6SYSTSTAT00 102.00.24.2
7.04.000
6STAT 108.0
as CP viol. O(high sensitivity to
edecoherenc total 1
QM 0
00
00
Decoherence parameter:
001
39V.Patera CERN seminar 28 March 2006
Charged KaonsCharged Kaons
K ±
lifetime BR(K+
2 ) K± semileptonic decays
40V.Patera CERN seminar 28 March 2006
Tagging KTagging K++ K K--
Measurement of absolute BR’s: KMeasurement of absolute BR’s: K beam tagged from K beam tagged from K
pp**(MeV)(MeV)
Kinem. ID
180 200 220 240
1000
3000
2000
101022 Ev/0.5MeV Ev/0.5MeV
Data
— fit:
Two-body decays identified as peaks in the momentum spectrum of secondary tracks in the kaon rest frame: 6x106x1088 tags/fb tags/fb-1-1
Given the tag a dedicated reconstruction of K tracks is performed, correcting for dE/dx losses of charged kaons in the DC
K++ K––0
–
–
++
41V.Patera CERN seminar 28 March 2006
region
MC includes radiative process
P* [MeV]BR(KBR(K++ ++(()) = 0.6366 )) = 0.6366 0.0009 0.0009stat.stat. 0.0015 0.0015syst.syst. [PLB 632 (2006)][PLB 632 (2006)] BR(KBR(K++ ++(()) = 0.6366 )) = 0.6366 0.0009 0.0009stat.stat. 0.0015 0.0015syst.syst. [PLB 632 (2006)][PLB 632 (2006)]
• (K())/(()) |Vus|2/|Vud|2fK2/f2
• From lattice calculations: fK /f =1.198(3)(+165)
(MILC Coll. PoS (LAT 2005) 025,2005)
|Vus| / |Vud| =0.2294 0.0026|Vus| / |Vud| =0.2294 0.0026
Measurement of BR(KMeasurement of BR(K(())))
• Tag from K--.• 175 pb-1: 1/3 used for signal selection, 2/3 used as efficiency sample• Subtraction of 0 identified background.• Count events in (225,400) MeV window of the momentum distribution in K rest frame ( hypothesis)
Signal selection
• Selection efficiency measured on data• Radiated acceptance measured on MC
42V.Patera CERN seminar 28 March 2006
Measurement of the KMeasurement of the K lifetime lifetime • Tag events with K2 decay• Kaon decay vertex in the fiducial volume• Measure from PDG not in agreement
Measure the kaon decay length taking into account the energy loss: K = i Li/(iic)• Tracking efficiency and resolution functions measured on data by means of neutral vertex identification.• Fit of the K distribution.
= 12.367 = 12.367 0.044 0.044StatStat 0.065 0.065SystSyst ns nsKLOE preliminary
K (ns)
16-30 ns
PDG = (12.385±0.024)ns
200 pb-1
43V.Patera CERN seminar 28 March 2006
BR(KBR(Ke3e3) = ) =
(5.047 (5.047 0.019 0.019StatStat 0.039 0.039Syst-Stat Syst-Stat 0.004 0.004SysTagSysTag))××1010-2-2
BR(KBR(K33) = ) =
(3.310 (3.310 0.016 0.016StatStat 0.045 0.045Syst-StatSyst-Stat 0.003 0.003SysTagSysTag))××1010--
22
BR(KBR(Ke3e3) = ) =
(5.047 (5.047 0.019 0.019StatStat 0.039 0.039Syst-Stat Syst-Stat 0.004 0.004SysTagSysTag))××1010-2-2
BR(KBR(K33) = ) =
(3.310 (3.310 0.016 0.016StatStat 0.045 0.045Syst-StatSyst-Stat 0.003 0.003SysTagSysTag))××1010--
22
Measurement of BR(KMeasurement of BR(Kℓℓ3)3) 4 independent-tag samples: K+2, K+2, K2, and K2 keep under control the systematic effects due to the tag selection Kinematical cuts to reject non-semileptonic decays, residual background is about 1.5% of the selected Kl3 sample Constrained likelihood fit of m2 data distributions from ToF measurements count the number of signal events Selection efficiency from MC and correct for Data/MC differences.
KLOE preliminary
Perform the BR measurement on each tag sample, separately normalizing to tag counts in the same data set,and average accounting for correlations:
K nuc.intK00
K0
Ev/(14MeV)2
Ke3 K
3
44V.Patera CERN seminar 28 March 2006
All Kaons together!All Kaons together!
Test of CKM unitarity: the first row
45V.Patera CERN seminar 28 March 2006
Unitarity test of CKM matrix – VUnitarity test of CKM matrix – Vus us & & VVus us / V/ Vudud• Most precise test of unitarity possible at present comes from 1st row:
Can test if = 0 at 10-3 level: from super-allowed nuclear -decays: 2|Vud|Vud = 0.0005 from semileptonic kaon decays: 2|Vus|Vus = 0.0009
|Vud|2 + |Vus|2 + |Vub|2 ~ |Vud|2 + |Vus|2 1 –
• Extract |Vus| from Kl3 decays. EM effects must be included:
(K ℓ) |Vus f+K0-(0) |2 I(t) SEW(1 + + SU(2) )
|Vus|
|Vus|
t)
t) f+K0-(0)
f+K0-(0)
= 0.5 0.5 Relative uncertainty:
• Extract |Vus|/ |Vud| from (K())/(()) ratio. Dominated by the
theoretical uncertainity on the fK/f evaluation from lattice QCD
• KLOE can measure almost all experimental inputs for neutral and charged kaons: branching ratios, lifetimes, and form factors (but S).
46V.Patera CERN seminar 28 March 2006
VVusus from KLOE results (BR’s and from KLOE results (BR’s and LL))
12.384(24) ns89.58(6) ps50.84(23) ns
0.03310(40)0.05047(46)7.046(91)×10-40.2698(15)0.4007(15)BR
K 3K e3KS e3KL 3KL e3
2/dof = 1.9/4
• f+(0)=0.961(8) Leutwyler and Roos Z.
[Phys. C25, 91, 1984]
• Vud=0.97377(27) Marciano and Sirlin
[Phys.Rev.Lett.96 032002,2006]
From unitarity
Vus×f+(0) = 0.2187(22)
(Pole model: KLOE, KTeV, and NA48 ave.)
(KTeV and Istra+ ave.)
Slopes
47V.Patera CERN seminar 28 March 2006
VVusus around the world and Unitarity around the world and Unitarity
Vus f+(0)
plot: F
.Mescia cou
rtesy
<V<Vusus××ff++(0)>(0)>WORLD AV.WORLD AV. = 0.2164(4) = 0.2164(4)
• L = 50.99(20) ns, average KLOE-PDG
• Including all new measurements
for semileptonic kaon decays (KTeV, NA48, E865, and KLOE)
• f+(0)=0.961(8) Leutwyler and Roos
[Z.Phys. C25, 91, 1984]
• Vud=0.97377(27) Marciano and Sirlin
[Phys.Rev.Lett.96 032002,2006]
From unitarity
Vus×f+(0) = 0.2187(22)
PDG04PDG04
48V.Patera CERN seminar 28 March 2006
The VThe VususVVudud plane planeunitarity
VVusus = 0.2254 = 0.2254 0.0020 0.0020 Kl3 KLOE, using f+(0)=0.961(8)
VVudud = 0.97377 = 0.97377 0.00027 0.00027 Marciano and Sirlin Phys.Rev.Lett.96 032002,2006
VVusus/V/Vudud = 0.2294 = 0.2294 0.0026 0.0026 K2 KLOE (K())/(()) |Vus|2/|Vud|2fK
2/f2
Inputs:Inputs:
Fit resultsFit results, P(2) = 0.66:
Vus = 0.2246 0.0016 Vud = 0.97377 0.00027
Fit result assuming unitarity, P(2) = 0.23: Vus = 0.2264 0.0009
49V.Patera CERN seminar 28 March 2006
Non Kaons physicsNon Kaons physics(my personal selection)(my personal selection)
mass ((ee++ee→→)) off peak physics @ 1 GeVoff peak physics @ 1 GeV
V.Patera CERN seminar 28 March 2006
After the kinematic fit (p,Etot,cluster times) the mass measurement is almost independent from the energy of the clusters, it is dominated by the cluster positions. The momentum and the vertex position are precisely determined from Bhabha scattering at large angle e+e- → e+e . Absolute scale buy - line shape and mass
measurement:
cross checking:
measurement @ KLOEmeasurement @ KLOE
GEM: M = (547.311 ± 0.028 ± 0.032) MeV/c2 PLB 619 (2005) 281
NA48: M = (547.843 ± 0.030 ± 0.041) MeV/c2 PLB 533 (2002) 196
Large discrepancy between the two most precise measurements
E2E1
E3
measurement measurement methodmethod
51V.Patera CERN seminar 28 March 2006
measurement @ KLOEmeasurement @ KLOE• Kinematic fit applied on→ events and 0 selected by looking at different Dalitz plot regions
M (MeV)
<m> = ( 547.708 0.014 ) MeV = ( 2.143 0.012 ) MeV
<m = ( 134.956 0.018 ) MeV = ( 1.66 0.005 ) MeV
2/ndf = 304/257
0
2/ndf = 146/161E1<E2<E3
M (MeV)
M (MeV)
0
52V.Patera CERN seminar 28 March 2006
measurement @ KLOEmeasurement @ KLOE
Data set divided in 8 periods
M(0) = ( 134990 6stat 30syst ) keV
M(0)PDG = ( 134976.6 0.6 ) keV
Systematics mainly from √s and vertex position EMC linearity in
progress NA48 compatibility: 0.24
547.95
547.90
547.85
547.80
547.75
547.70
M (M
eV
)
M (M
eV
)
M() = ( 547822 5stat 69syst ) keVKLOE preliminaryKLOE preliminary
NA48
V.Patera CERN seminar 28 March 2006
μ μ and and ((ee++ee→→) @ KLOE) @ KLOE
Process e+e- +- @ s < 1 GeV contributes as much as 66% to ahad
So far, estimates of ahad from:
2) using the spectral function from (LEP, CESR data)
Dispersion integral relates had(vac-pol) to s(e+e- hadrons)
1) measuring (e+e ) vs s at an e+e- collider, varying the beam energy
54V.Patera CERN seminar 28 March 2006
((ee++ee→→) @ KLOE) @ KLOE
(s’ = s – 2 Es)
Luminosity from e+e() counts, 55 < e < 125, at 0.5% (th) 0.3%(exp)Radiator function H(M
), defined as:
d M
dM
MM
with inclusion of radiative effects, as FSR, from QED MC calculation (PHOKHARA, Karlsuhe Theory Group, Kühn et al.)
At the mass it is possible to measure e+e with high accuracy:
Exploit ISR to extract (e+e +) for s´ from 2m s
M2
FSR
55V.Patera CERN seminar 28 March 2006
((ee++ee→→) : data samples for ) : data samples for eventsevents
Photons at small angles( < 15o or > 165° )
Photon NOT DETECTED High Statistics for ISR Photons
Low relative contribution of FSR <0.5% in entire M– range
Small amount of other background
Photons at large angle
( 50o < < 130° ) Photon detection required High amount of FSR and background
Allows measurement at threshold
Allows measurement of charge asymmetry Test of FSR
56V.Patera CERN seminar 28 March 2006
(e+e- ) nb
0.4 0.5 0.6 0.7 0.8 0.90.3
200
400
600
800
1000
1200
1400
M2 (GeV2)
KLOE
2001 Data
140pb-1
Phys. Lett. B606 (2005) 12
((ee++ee→→) : small angle results) : small angle results
a [10-10 ]
KLOE (‘05)
SND (‘05),
CMD-2 EPS (‘05) preliminary
CMD-2 (‘04)
• fair agreement btw all 4 data sets CMD-2 and KLOE agree within 0.5 • disagreement btw KLOE and SND ca.1.5
2 contribution to ahadr
[0.3
7-0.
93 G
eV2 ]
V.Patera CERN seminar 28 March 2006
Changes of online andoffline reconstruction
The goals for the analysis of 2002 data: considerable reduction of errors
Total theoretical error 0.9%
*Goal : Error < 1%
0.5%Radiator Function0.3%FSR Corrections0.2%Vacuum Polarization
<<0.6%Luminosity *
Total experimental error 0.9%0.2%Unfolding Effects0.3%Background0.2%Trackmass Cut0.1%Particle ID
<< 0.6%Reconstruction Filter *<0.3%Vertex 0.3%Tracking
<0.3%Trigger *
0.3%Acceptance
New version ofBABAYAGAwith full NLO
dN
/dM
dN
/dM
22 (ev
ents
/GeV
(ev
ents
/GeV
22 ))
2002Data
Normalisation to Muons
MM22 (GeV (GeV22))
((ee++ee→→) : improvement at small ) : improvement at small angle angle
V.Patera CERN seminar 28 March 2006
the threshold region is accessible photon tagging is possible (4-momentum constraints) lower signal statistics large FSR contributions large backgroundirreducible bkg. from decays
PRO & CONTRA
50o<<130o
50o<<130o
L = 240 pb-1
preliminary
MC MC<
By means of dedicated selection cuts it is possible to fight the dominant background Analysis in very advanced state
Threshold region non-trivial due to irreducible FSR-effects,which have to be cut from MCusing phenomenol. Models(interference effects unknown)
ff
FSR f0
MM22 (GeV (GeV22))
((ee++ee→→) : large angle ) : large angle
59V.Patera CERN seminar 28 March 2006
((ee++ee→→) :) :Forward-backward asymmetry
Using the f0 amplitude from Kaon Loop model, good agreement data-MC* both around the f0 mass and at low masses.
M (MeV) M (MeV)
• data MC: ISR+FSR MC: ISR+FSR+f0(KL)
Phys.Lett.B634 (06), 148
* G. Pancheri, O. Shekhovtsova, G. Venanzoni, hep-ph/0506332
+- system: A(ISR) C-odd while A(FSR) & A(scalar) C-even asymmetry in the variable:
-πθ π
θ
Pion polar angle [o]
90o
MC
V.Patera CERN seminar 28 March 2006
@ large angle: looking for f@ large angle: looking for f
The f0 signal is a deviation of M spectrum from the expected ISR + FSR shape. Scalar amplitude from models:
M() (MeV)
f0(980) region
M() (MeV)
Events/1.2 MeV
676000
events1. Kaon-loop KL (Achasov-Ivanchenko, NPB315
1989): for each scalar meson S there are three free parameters of the fit: gS, gSKK, MS
2. No-Structure NS (by G.Isidori and
L.Maiani): a modified BW + a polynomial continuum: gS, gS, gSKK, MS + pol. cont. parameters
SgKK
gSKK
gSPP
K
K
SV
gVS
gSe+
e-
V.Patera CERN seminar 28 March 2006
Fit to the m(Fit to the m() spectrum:) spectrum:
(491 bins, 1.2 MeV wide, m() = 420 to 1009 MeV)
Fit : ISR + FSR + + scalar ± interf(SCAL+ FSR)
Kaon-Loop and No-Structure fits:
Good description in both casesof signal and background
“negative” interference;
The introduction of a (600) doesn’t improve the fit.
KL fit NS fit
f0 signal
f0 signal
[PLB634 (2006) 148]
V.Patera CERN seminar 28 March 2006
• KLOE Integrated 200pb-1 at s = 1.00 GeV• In addition has been performed a -scan of 4 points, 10pb-1 each
• background-free Radiative Return 200pb-1 allow to be statistically com- petitive with VEPP-2000 at threshold
• a -scan allows to study the model- dependence in desciption of f0(980)
• background-free - program
s (
MeV
)
s = 1023s = 1023
s = s = 10301030
s = 1018s = 1018
s = 1010s = 1010
s = 1000s = 1000
Run-Nr.
Trackmass [MeV]
Nu
mb
er o
f E
ven
ts /
MeV
10pb-1 ONPEAK
OFFPEAK
First look into off-peak-data
very promising ..... !
- Large photon angle acceptance cuts- PID: both tracks identified as pions
Off resonance run @ 1 GeV Off resonance run @ 1 GeV
V.Patera CERN seminar 28 March 2006
KS PLB 538, 21 (02)KL PLB 566, 61 (03)
K+ +00 PLB 597, 49 (04)
KS e PLB 535, 37 (02)
KS 000 PLB 619, 61 (05)
KL main PLB 632, 43 (06)
KL lifetime PLB 626, 15 (05)
KLOE physics papers published to date
K+ +( ) PLB 632, 76 (06)
00 PLB 537, 21 (02)
0 PLB 536, 203 (02)
+0 PLB 561, 55 (03)
' PLB 541, 45 (02)
l+l PLB 608, 199 (05) + PLB 606, 12 (05)
PLB 591, 49 (04)
+ PLB 606, 12 (05)
+ PLB 634, 148 (06)
64V.Patera CERN seminar 28 March 2006
OutlineOutline
Physics @ peak DANE, the frascati
factory The KLOE detector KLOE recent results:
Kaon physics (mostly)Non Kaon physics
Future of KLOE & DANE Summary and conclusions
65V.Patera CERN seminar 28 March 2006
DADANE & KLOE NE & KLOE futurefuture
DANE upgrades physics programphysics program KLOE upgradesKLOE upgrades
V.Patera CERN seminar 28 March 2006
DADANE : near term future NE : near term future
2006 – Final KLOE run (up to 2 fb-1)
-shutdown for FINUDA installation
-FINUDA run
2007 – FINUDA run (up to 1 fb-1)
-shutdown for SIDDHARTA installation
-SIDDHARTA run
2008 – SIDDHARTA run (up to 1 fb-1)
-shutdown for FINUDA installation
-Final FINUDA run (up to 2 fb-1)
DAFNE scientific program
scheduled up to 2008.
Upgrades have been
proposed and submitted
to INFN. Explicitely
mentioned in the 3-years
“ROAD-MAP”
of INFN
Only e+e- collider in Europe
V.Patera CERN seminar 28 March 2006
DADANE Upgrade – short term (3 years)NE Upgrade – short term (3 years)
Starting from 1.5x1032, 2fb-1/year: Reduction of e- ring beam impedance (by a factor 2) :
Removal and shielding of the broken Ion-Cleaning-Electrodes
Higher positron current (up to 2 A), so far limited to 1.3 A: New injection kickers Ti-Coating against electron cloud
Feedback upgrades
Wigglers modifications to increase Lifetime (by a factor 2): New interaction region Transfer lines upgrade (continuous injection)
To be discussed: Crab cavities, waist modulation (RF quads) Expected a
factor > 3 in
Luminosity
V.Patera CERN seminar 28 March 2006
DADANE-2: Long term upgrade NE-2: Long term upgrade (2010(2010))
Change of machine layout, insertion of: Superconducting cavities
Superconducting wigglers Ramping Dipoles New vacuum chamber
Energy (GeV) 1.02 2.4
Integrated Luminosity per year (fbarn-1) >10
Total integrated luminosity (5 years, fbarn-1) >50 >3
Peak luminosity (cm-1sec-2) >8 1032 >1032
Machine can go higherMachine can go higher
in energy (up to 2.4 in energy (up to 2.4
GeV)GeV)TDR in preparation: necessary to submit the project
V.Patera CERN seminar 28 March 2006
The KLOE future: KLOE-2 The KLOE future: KLOE-2
An Espression of Interest for
the continuation of the KLOE
has been presented.
The physics program is focused
on KS physics , ’ physics and
quantum interferometry
studies.
Time schedule and luminosity
foreseen are 30fb-1 on tape
within 2014 11 institution x 7 nations involved
V.Patera CERN seminar 28 March 2006
KLOE2: perspectives for Kaon physicsKLOE2: perspectives for Kaon physics
KS 0 0 0 CP,CPT < 1.2 10-7 < 5 10-9 seenKS e CPT, S= Q (7.09 0.10)10-4 0.2 10-5 0.1 10-5
As CPT (1.5 11) 10-3 2 10-3 1 10-3KS + - 0 pt (3 1)10-7 0.4 10-7 0.3 10-7 KS e+e- < 1.4 10-7 < 2 10-8 < 9 10-9
KS 0 e+e- KL CP (6 3)10-9 seen 2 10-9 KS pt (2.78 0.07)10-6 0.03 10-6 0.02 10-6
Assuming/extrapolating present KLOE efficiencies/systematics
Present @20fb-1 @50 fb-1
Competitive on rare KS decays, CPT and S= Q violating parameters, interesting for CHPT
Lint= 20-50 fb-1
BR(K±e2)/BR(K±
2) SM test (2.4160.053)10-5 <% rel. err few ‰ rel err
V.Patera CERN seminar 28 March 2006
ChPT, study of spectrum expected 3000 events
’ l+l-,lll(‘)l(‘) (Dalitz & double dalitz decays) with high statistics
e+e test of CP violation beyond SM
’ sensitive toexpected
200.000 events
KLOE-2: perspectives for KLOE-2: perspectives for & scalars & scalars physicsphysics
With 20 fb-1 f0 , fK+K- (KK) (expected BR ~ 10-6(-8) ) well measured (105 K+K- and 103 KK), direct measure of the gfKK coupling
-factory = ed ’ factory
BR( ) = 1.3 ×10-2 N(20 fb-1) ~ 9 × 108
BR( ’) = 6.2 ×10-5 N’(20 fb-1) ~ 5 × 106
Monochromatic prompt photon: clear signature
V.Patera CERN seminar 28 March 2006
KLOE2: Kaon interferometry: main KLOE2: Kaon interferometry: main observablesobservables
measured quantity parameters
εε
εε
mode
0;,0;,
0;,0;,0000
0000
tItI
tItItA
00 LS KK
LS KK
a
dK
a
cK
LS KK teIteI
teIteItA
;,;,
;,;,
tI ;, LS KK L Sm
adab
A KKL
ε2
0;,0;,
0;,0;,
teeIteeI
teeIteeItACPT
V.Patera CERN seminar 28 March 2006
Use of a lower magnetic field. This can increase acceptance for several of the above mentioned channels and ease pattern recognition (.5T→.3T →x 2 gain in acceptance on KSl3)
Insertion of a vertex chamber. At present, first tracking layer is at 30 cm (i.e. 50 S) from the I.P. Increase the KS, K± geometrical acceptance
Increase calorimeter’s readout granularity. Can improve photon counting, as well as particle identification (e//).
A small angle tagger for physics
KLOE2: detector KLOE2: detector upgradesupgrades
The KLOE efficiency/systematics can be improved, increasing
quadratically the collected events both via the tag and via
the signal emisphere. The KLOE experience suggest as
upgrades of the detector
74V.Patera CERN seminar 28 March 2006
OutlineOutline
Physics @ peak DANE, the frascati
factory The KLOE detector KLOE recent results:
Kaon physics (mostly)Non Kaon physics
Future of KLOE & DANE Summary and conclusions
V.Patera CERN seminar 28 March 2006
ConclusionsConclusions
KLOE has integrated 2.5fb-1 during its data taken at
DANE
During 2005-2006 published results leading to
substantial improvement to VUS, TCPV, hadr
Analysis of approx. 2/3 of the data set on-going
An EoI for the continuation of the KLOE physics
program at an improved DANE has been presented
76V.Patera CERN seminar 28 March 2006
SPARESSPARES
V.Patera CERN seminar 28 March 2006
Magnetic field value dramatically affects signal acceptance. Can improve up to a factor ~ 2
Proper balancing with consequent loss in momentum resolution yet to be studied
B (kG)
ε (KLCrash + Ks DC selection)
Present analysis, MC with detailed field map400 pb MC with LSF=0.5, with uniform axial B field
0.1
0.2
3 540
0.15
0.05
T. Spadaro
Bfield & reconstruction eff:Bfield & reconstruction eff: KKSS ee decaysdecays
V.Patera CERN seminar 28 March 2006
KS 30 decays
Background mostly due to photon clusters double splittings
Preliminary studies show that there is room for “algorithmic” improvements in background rejection without big losses in
signal efficiency
Study of the entire KLOE data set crucial for a better assessment of the real potentialities of the analysis
Ideally, with 20 fb1 one can reach a limit ~ 5x109
With With 50 fb50 fb11 one could hope to observe a few events! one could hope to observe a few events!
V.Patera CERN seminar 28 March 2006
KS + 0 : a test for ChPT
ChPT predicts B(Ks +0) = (2.4 ± 0.7)x107
The present experimental value (3.3 +1.1 0.9 ) x107 is the average of three different measurement each individually precise at ~ 40%
A preliminary KLOE analysis obtains εsig ~ 1.3%, S/B ~ 2
Assuming
Error on BR @ 2 fb1 (%)
Error on BR @ 20 fb1 (%)
Error on BR @ 50 fb1 (%)
No further effort made to reduce background
~ 60% ~ 20% ~ 12%
Further efforts completely remove background
~ 40% ~ 12% ~ 8%
V.Patera CERN seminar 28 March 2006
KS + 0 as a pedagogical example
This is the typical case where analysis would greatly benefit from simple detector upgrades
At least one of the two tracks has low momentum: 65% of signal lost lost only due to acceptanceonly due to acceptance
Acceptance can be increased by the use of a lower B fieldlower B field. Also the use of a vertex chambera vertex chamber could definitely help
Both can be useful also for the rejection of the background due to patological charged kaon events
V.Patera CERN seminar 28 March 2006
KS 0 e+e decays
Fundamental to assess indirect CPV contribution to parent KL decay
Measured by NA48 on the basis of 7 events (plus 6 +)
Theoreticians’ dream: measurement at 15% accuracy
BR = (5.8 ± 3) x 10-9
What efficiency can reasonably be expected for KLOE?
V.Patera CERN seminar 28 March 2006
KS 0 e+e decays
Further selection based on cuts on 5 independent variables
e+e inv. mass 2 kinem. fit
MC MC
DATA 400 pb1 DATA 400 pb1
signal
signal
V.Patera CERN seminar 28 March 2006
KS 0 e+e decays
Cuts tuned on MC: 0 events retained < 4.8 ev / fb1 @ 90% CL
Detailed studies of problematic topologies:
single dalitz : 880 pb1 : 0 events < 2.6 ev / fb1
double dalitz: 4200 pb1 : 0 events < 0.55 ev / fb1
K+K : 880 pb1 : 0 events < 2.6 ev / fb1
Overall efficiency on signal: 4.3%
Check on data (~ 400 pb1) : 0 observed (0.12 expected)
Optimistically (no further bkg) ~ 5 events observed in 20 fb1
V.Patera CERN seminar 28 March 2006
Mode Parameter Best measurement
or PDG-04 fit
KLOE-2
L=100 fb-1
m 5.288 ± 0.043 109 s-1
± 0.02STAT
109 s-1
Reε’ε (1.67 ± 0.26) 10-3 ± 0.2STAT 10-3
Imε’ε 0.0012± 0.0023 ± 0.0022STAT
e AL (3322± 58 ± 47 ) 10-6 ± 18STAT 10-6
e e Re() (0.29 ± 0.27) 10-3 ± 0.2STAT 10-3
e e Im() (0.24 ± 0.50) 10-4 ± 20STAT 10-4
Prospectives for InterferometryProspectives for Interferometry
V.Patera CERN seminar 28 March 2006
-factory = ed ’ factoryBR( ) = 1.3 ×10-2 N(20 fb-1) ~ 9 × 108
BR( ’) = 6.2 ×10-5 N’(20 fb-1) ~ 5 × 106
Monochromatic prompt photon: clear signature
Mixing – ’: Uncertainty dominated by systematics;improvement can come by measuring main ’ BR’s
decays: (test ChPT; major improvements expected with 20 fb-1)Dalitz decays: e+e-, , e+e-e+e- Transition FF e+e- (Test of CP violation, analogous to KL e+e- )Improvements on forbidden/rare decays
’ decays:Dalitz plot of ’+- scalar amplitude ’ first observation / isospin violation
Perspectives forPerspectives for’ at DA’ at DANE-2NE-2
86V.Patera CERN seminar 28 March 2006
KKSS ee: CPT test: CPT test
AS = 2(Re ε Re Re y Re x)
AL = 2(Re ε Re Re y Re x)CPT indecay
CPT inmixing
CP S Q and CPT
• Sensitivity to CPT violating effects through charge asymmetry
eHWK = a b
eHWK = a* b*
eHWK = c d
eHWK = c* d*
b=d=0 if CPT holdsc=d=0 if S=Q holds
KS eamplitudes
Re y = Re b/aRe x = Re d*/a
M11M22 i
mS mL iSL
1
2
87V.Patera CERN seminar 28 March 2006
dcKbaK
dcKbaK
00
00
S=QCPTTCP
=0=0=0=0d=0=0=0c
=0=0=0b=0=0a
Semileptonic decay amplitudes: definitions
a
cx
a
dx
a
by CPT violation:
S=Q violation:
CPT violation & S=Q violation :
88V.Patera CERN seminar 28 March 2006
Number of KL from fit of Number di KL from fit of
KL CP violation
22 )( missmiss pE
(MeV) 22missmiss pE
)hyp. (missmiss Ep
(MeV) missmiss Ep
89V.Patera CERN seminar 28 March 2006
We get the following accuracies on each term of the sum:
KS
00KS
KS
SL B(KLl3) AS+AL)/4iIm x
SL KL
SL KL
10-4
Im
Re
CPT test: accuracy on CPT test: accuracy on ii
90V.Patera CERN seminar 28 March 2006
CPT test: m(K)-m(K)CPT test: m(K)-m(K)
m(K)-m(K)
(K
)-(K
)
(K
)-(K
)
m(K)-m(K)
GeV
GeV GeV
GeV
(m) ~ 210 GeV
() ~ 410 GeV
CPLEAR KLOE
M11M22 i
mS mL iSL
1
2
91V.Patera CERN seminar 28 March 2006
a [10-10 ]
KLOE (‘05)
SND (‘05),
CMD-2 EPS (‘05) preliminary
CMD-2 (‘04)
MM22 (GeV (GeV22))
/ K
LO
E -
1
• CMD-2 (‘04) and KLOE agree @ high M
• some disagreement btw. KLOE and
CMD-2/SND on the peak
• fair agreement btw all 4 data sets
CMD-2 and KLOE agree within 0.5
• disagreement btw KLOE and SND ca.1.5
interpolation of 60KLOE data points from 0.35
to 0.95 GeV2
Comparison with recent e+e DataComparison of e+e- experiments 2 contribution to a
hadr
[0.3
7-0
.93
GeV
2]JETP, Vol. 101, No 6 (2005) 1053
PLB 578 (2004) 285
92V.Patera CERN seminar 28 March 2006
mass measurement : the mass measurement : the methodmethod
E1
E2
E3Using the decays:
Px,Py,Pz,Etott-r/c of clusters
A kinematic fit is performed imposing:
conservationcompatible with light velocity
As a consequence of the kinematic fit the mass measurement is almost independent from the energy of the clusters, it is dominated by the cluster positions.
The momentum and the vertex position are precisely determined run by run from the study of the Bhabha scattering at large angle e+e- e+e – (90000 events for each run). Absolute scale determined buy line shape and mass
cross checking purpose
93V.Patera CERN seminar 28 March 2006
Prospects for small angle analysisProspects for small angle analysis
Many systematics cancel out on
the theory side:
Luminosity, VP , radiatoror reduce to small corrections on
the experimental side
tracking , vtx efficiencies
and trigger veto
Differently from the old analsyis
statistics is an issue, due to the
small cross section in some S bins
′′′′
′′
)(/
/)( s
sdd
sdds Born
obs
obsBorn
Analysis of the new data (2 fb): take advantage of larger statistics!Change strategy normalizing to
Improvements also on Filter/ECL strategies
V.Patera CERN seminar 28 March 2006
Neutral kaons tagging: KNeutral kaons tagging: KSS “beam” “beam”
Kinematic closure of the
event
(pS=p-pL):
KS angular resolution: ~ 1° (0.3
in )
KS momentum resolution: ~ 1
MeV/c
*
Clean KS tagging by time-of-flight
identification of KL interactions
in the calorimeter :
tof(KL) ~30 ns tof
(~6 ns)
KL velocity in the rest frame 0.218
Tagging efficiency εtag,total~ 30% 1.4
108 tagged KS
Clean KS tagging by time-of-flight
identification of KL interactions
in the calorimeter :
tof(KL) ~30 ns tof
(~6 ns)
KL velocity in the rest frame 0.218
Tagging efficiency εtag,total~ 30% 1.4
108 tagged KS
KS KL “crash”
95V.Patera CERN seminar 28 March 2006
@ large angle (@ large angle (50o<<130o, E>50MeV ))
10 times more statistics on tape!The spectrum extends down to the 2-pions threshold
dN
/dM
2 Both the particles not
identified as electrons Cut on 2
in the hyp.
Cut on TrackMass vs. M
2
Cut on angle
L = 240 pb-1
M2 [GeV2]
M2 [GeV2]
KLOE preliminary
KLOE preliminary
missp
γp
– MC
– MC
- MC
M2 [GeV2]
Mtr
k [M
eV
]
m
m
m
V.Patera CERN seminar 28 March 2006
Forward-backward asymmetry +- system: A(ISR) C-odd A(FSR) C-even an asymmetry is expected in the variable:
-πθ π
θ
Pion polar angle [o]
90o
MCtest of sQED via comparison data/MC
Issue: to distinguish the effect of the interference (described in our MC by sQED ) and the effect of f0(980).
Czyż, Grzelińska, Kühn, Phys.Lett.B 611(116)2006
M [GeV]
20o<<160o
45o<<135o
f0 kk model f0 ‘no str’ f0 ‘no str’ /2 no f0
A(f0) C-even
V.Patera CERN seminar 28 March 2006
The Particle Data Group measures are not in agreement
: experimental picture: experimental picture
= (12.385±0.024)ns