measurement of pp scattering lengths in kaon decays by na48/2
DESCRIPTION
Measurement of pp scattering lengths in Kaon decays by NA48/2. EPS-HEP 2007 Manchester 19-25 july 2007. Gianluca Lamanna (Università & INFN di Pisa) on behalf of NA48/2 collaboration. Outline. Introduction Ke4 (K ± → p + p - e ± n ) Form factors and pion scattering lengths - PowerPoint PPT PresentationTRANSCRIPT
1
Measurement of Measurement of scattering lengths in Kaon scattering lengths in Kaon
decays by NA48/2decays by NA48/2EPS-HEP 2007
Manchester 19-25 july 2007
Gianluca LamannaGianluca Lamanna (Università & INFN di Pisa)(Università & INFN di Pisa)
on behalf of NA48/2 collaborationon behalf of NA48/2 collaboration
2 Gianluca Lamanna – HEP07 19.07.2007
OutlineOutline Introduction
Ke4 (K±→ e±)
Form factors and pion scattering lengths
Data 2003: Preliminary results
Cusp (in K±→±)
A new method to extract pion scattering lengths through the strong rescattering process →
Data 2003+2004: Preliminary results
Conclusions
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Experimental setup:The BeamsExperimental setup:The Beams
K+
K−
BM
PK spectra, 603 GeV/c
54 60 66
Width ~ 5mm
K+/K- ~ 1mm
SPS protons @ 400 GeV
Simultaneus, unseparated, focused beams
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NA48/2 detectorNA48/2 detectorSpectrometer:Spectrometer:
σσpp/p = 1.0% + 0.044% p [p in /p = 1.0% + 0.044% p [p in GeV/GeV/cc]]
LKR calorimeter:LKR calorimeter:
σσEE/E = 3.2%/√E + 9%/E + 0.42% [E /E = 3.2%/√E + 9%/E + 0.42% [E in GeV]in GeV]
CHODCHOD, , HACHAC,,MUVMUV,, vetos vetos
KabesKabes
Beam MonitorBeam Monitor
Only the spectrometer and LKr are involved in the analysis.
The CHOD is used at the trigger level.
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NA48/2 data & resultsNA48/2 data & results
20032003 run: run: ~ 50 days~ 50 days
20042004 run: run: ~ 60 days~ 60 days
Total statisticsTotal statistics 2 years: 2 years:
KK±±→→±±0000: : ~1·10~1·1088
KK±±→→±±++--:: ~3·10~3·1099
Greatest amount ofGreatest amount of KK→3 →3 everever collectedcollected
u
v Beam Beam PipePipe
The main goal of NA48/2 was to measure the CP violationCP violation in charged kaon decays through the study of the asymmetry in three pion decays
The goal to reach a precision of 10-4 in the CP violation parameters Ag has been obtained after 2 years of data taking (2003 and 2004)
No signal of CP violation outside the SM at our level of precision
AAgg=(-=(-1.5+1.51.5+1.5statstat+0.9+0.9trigtrig+1.1+1.1systsyst))··1010-4-4
AAgg00=(1.8+1.7=(1.8+1.7statstat+0.5+0.5systsyst))··1010-4-4
AAgg=(-=(-1.5+1.51.5+1.5statstat+0.9+0.9trigtrig+1.1+1.1systsyst))··1010-4-4
AAgg00=(1.8+1.7=(1.8+1.7statstat+0.5+0.5systsyst))··1010-4-4Phys.Lett.B 634:474-Phys.Lett.B 634:474-
482,2006 Phys.Lett.B 482,2006 Phys.Lett.B 638:22-29,2006 638:22-29,2006 CERN-PH-EP-2007-021CERN-PH-EP-2007-021
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KKe4e4: formalism: formalism The Ke4 dynamics is fully described
by 5 (Cabibbo-Maksymovicz) variables: MM
22, M, Mee22, cos, cos, cos, cosee and and
In the partial wave expansion the amplitude can be written using 2 axial and 1 vector form factors (the axial form factor R is suppressed in Ke4 but accessible in K4):
F=Fseis+Fpeipcos
G=Gpeip
H=Hpeip
The form factors can be expansed as a function of M
2 and Me2:
F (Fp,Fs), G, H and =p-s will be used as fit parameters
Fs=fs+fs’q2+fs’’q4+fe’(Me2/4m
2)+...
Fp=fp+fp’q2+...
Gp=gp+gp’q2+...
Hp=hp+hp’q2+...q2=(M
2/4m2)-1
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KKe4e4: selection & background: selection & backgroundSelection:Selection:
3 tracks
Missing energy and missing Pt
LKr/DCH energy to
electron PID 677500 decays
The background is studied using the electron “wrong” sign events (we assume Q=S and total charge ±1) and cross check with MC. The total bkg is at level of 0.5%.
Main background sources:Main background sources:
+ →e
with misidentified
or +(Dalitz) +e misidentified and s outside the LKr
e
K
Kaon momentum
GeV/c
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KKe4e4: Fitting procedure: Fitting procedure The form factors (F,G,H and ) are extracted minimizing a log-likehood estimator in
each of 10(M)x5(Me)x5(cose)x5(cos)x12()=15000 equi-populated bins. In each bin the correlation between the 4+1 parameters is taken into account.
Data MC
K+ evts 43565429
10.0 M667
Evts/bin
K- evts 24185616
5.6 M373
Evts/bin
The form factors structure is studied in 10 bins of M, assuming constant form factors in each bins
A 2D fit (M, Me) is used to study the Fs expansion
All the results are given wrt to Fs(q=0) constant term, due to the unspecified overall normalization (BR is not measured)
M
● Data
▬ MC
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KKe4e4: Fitting procedure and results: Fitting procedure and results
Fp(q
2)
Fs(q
2)
Gp
(q2)
Hp(q
2)
Fs is quadratic in q2 First measurement of Fp≠0
Linear in q2 No linear term (hp’)
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KKe4e4: form factors result: form factors result
f’s/fs = 0.165±0.011±0.006
f’’s/fs= -0.092±0.011±0.007
f’e/fs = 0.081±0.011±0.008
fp/fs = -0.048±0.004±0.004
gp/fs = 0.873±0.013±0.012
g’p/fs = 0.081±0.022±0.014
hp/fs = -0.411±0.019±0.007
f’s/fs = 0.165±0.011±0.006
f’’s/fs= -0.092±0.011±0.007
f’e/fs = 0.081±0.011±0.008
fp/fs = -0.048±0.004±0.004
gp/fs = 0.873±0.013±0.012
g’p/fs = 0.081±0.022±0.014
hp/fs = -0.411±0.019±0.007 All the Form factors are measured
relatively to fs
first evidence of fp≠0 and fe’≠0
The f.f. are measured at level of <5% of precision while the slopes at ~15% (factor 2 or 3 improvement wrt previous measurements)
Separately measured on K+ and K- and then combined (different statistical error)
Systematics checks:Systematics checks:
Acceptance
Background
PID
Radiative corrections
Evaluation of the sensitivity of the form factors on the Medependence of the normalization
Prelimina
ry (2003
data)
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KKe4e4:: dependence dependence The extraction of the pion scattering lengths from the =s-p phase shift needs
external theoretical and experimental data inputs .
The Roy equations, for instance, provide this relation between and a0,a2 near threshold, extrapolating from the M>0.8 GeV region. The precision of these data defines the width of the Universal Band in the (a0,a2) plane.
The fit of the experimental points using the Roy equations in the universal band allows to extract the a0 and a2 values
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KKe4e4: (a: (a00,a,a22) plane: result and comparison) plane: result and comparison
Minimizing the 2 in the 2D fit it’s possible to identify the favoured solution (and the corresponding ellipse)
The E865 and NA48/2 results agreement is marginal (manly due to the last point in E865) (work ongoing (see Gasser talk at Kaon07) )
The correlation between a0 and a2 is ~96% (similar for both experiment)
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KKe4e4: “neutral”: “neutral”Selection:Selection: one electron track in the DCH , 4 photons in the LKr, 0 mass constraints, missing Pt. 9642 events in 2003 (previous exp. 216 events) ~30000 events in 2004
Background:Background: with a misidentified , ke3+1 accidental ~ 3% in 2003 (276 events) ~ 2% in 2004
Due to the symmetry only the s-wave is present (fs’, fs’’)
f’e has been measured consistent with 0 within the present statistics
BR(Ke400)prel=
(2.587±0.026stat±0.019syst±0.029ext)·10-5
f’s/fs=0.129±0.036±0.020
f’’s/fs=-0.040±0.034±0.020
f’s/fs=0.129±0.036±0.020
f’’s/fs=-0.040±0.034±0.020
Preliminar
y
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Cusp: KCusp: K±±→→±± selection selection Offline selectionOffline selection: among all the possible pairings, the
couple for which is smallest is selected
The K-decay vertex is the average between the two decay vertices
After associating a charged track to the 2 0s the compatibility with the PDG kaon mass is requested to be ± 6 MeV.
2
0
1ijjiij dEE
mZ
++0000 invariant mass, GeV/c invariant mass, GeV/c22
Resolution: 0.9 MeV/c2
MKPDG ± 6 MeV/c2
cut
contribution
LKr
z
dij
i
jZ(i,j)Z(k,l)
Vertex
22
2
Km
K
z
mz
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Cusp: Dalitz plot distributionCusp: Dalitz plot distribution The high statistics and the good
resolution allow to see a “cusp” in the U (or M2
) distribution in the position of 2m
16.0 M events in 2003 + 43.6 M events in 2004 data taking
~65% of the whole statistics
M2
M2
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Cusp: one loop rescatteringCusp: one loop rescattering
M
K±
±
=M0
K±
±
+M1
K±
±
+-
24 ms ||)(|| 2
12
02 MMM
24 ms 10
21
20
2 2)()(|| MMMMM
The M1 contribution is real below and immaginary above threshold
M0 = A0(1+g0u/2+h’u2/2+k’v2/2)
1– ( )2M1 = –2/3(a0–a2)m+M+
M00
2m+
Below the threshold the (negative) interference term gives a “depletion” in the mass distribution
The cusp is proportional to (a0-a2)
Cabibbo Phys. Rev. Lett. 93, 121801 (2004)
threshold
13% of depletion
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Cusp: two loopsCusp: two loops
M
K± ±
=M0
K±±
+
M1
K±±
+
- K±
+ +...
Including 2-loops diagrams other terms appear in the amplitude
All the S-wave amplitudes (5 terms) can be expressed as linear combination of a0 and a2
The isosping breaking effect is taking in to account
The radiative correction (most relevant near threshold) are still missing
A deviation from the no rescattering amplitude behaviour appears also above threshold
Cabibbo,Isidori JHEP 0503 (2005) 21M2(00), (GeV/c2)2
0.074 0.076 0.078 0.080
Leading effect
Sub-Leading effect
No rescattering
Cusp
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Cusp: fit procedure & resultCusp: fit procedure & result The detector acceptance
correction is obtained with a full GEANT simulation
The 1-D fit is performed excluding 7 bins7 bins around the threshold position
The excess of events in this region is interpreted as pioniumpionium signature Pionium : R=(K+A2)/(K+–) =
(1.820.21)10–5.
Prediction: R=0.810–5 (Silagadze, 94)
(a0–a2)m+= 0.261 0.006stat. 0.003syst. 0.0013ext
.
a2m+= –0.037 0.013stat. 0.009syst. 0.0018ext.
(a0–a2)m+= 0.261 0.006stat. 0.003syst. 0.0013ext
.
a2m+= –0.037 0.013stat. 0.009syst. 0.0018ext.
Using ChPt constraints [Colangelo et al., PRL 86 (2001) 5008] a2 = –0.0444 + 0.236(a0–0.22) – 0.61(a0–0.22)2
– 9.9(a0–0.22)3 (a0–a2)m+= 0.263 0.003stat. 0.0014syst. 0.0013ext
Using ChPt constraints [Colangelo et al., PRL 86 (2001) 5008] a2 = –0.0444 + 0.236(a0–0.22) – 0.61(a0–0.22)2
– 9.9(a0–0.22)3 (a0–a2)m+= 0.263 0.003stat. 0.0014syst. 0.0013ext
This result is fully compatible with our previous measurement on partial sample ((Phys.Lett. Phys.Lett. B633:173-283,2006B633:173-283,2006))
Preliminar
y
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Cusp: systematics & “neutral” Cusp: systematics & “neutral” slopesslopesSystematic effectSystematic effect (a(a00––
aa22))101022
aa22101022 (a(a00–a–a22))
10102 2 ChPtChPtAnalysis technique ±0.10±0.10 ±0.20±0.20 ±0.08±0.08
Trigger inefficiency negl.negl. ±0.50±0.50 negl.negl.
Description of resolution ±0.06±0.06 ±0.11±0.11 ±0.06±0.06LKr non-linearity ±0.06±0.06 ±0.26±0.26 ±0.05±0.05Geometric acceptance ±0.02±0.02 ±0.01±0.01 ±0.02±0.02
MC sample ±0.03±0.03 ±0.21±0.21 ±0.06±0.06
Simulation of LKr showers ±0.17±0.17 ±0.50±0.50 ±0.04±0.04V-dependence of amplitude
±0.17±0.17 ±0.38±0.38 ±0.02±0.02
Total ±0.28±0.28 ±0.90±0.90 ±0.14±0.14
The external error comes from A00/A+-= 1.9750.015
A theoretical error of 0.013 (in a0-a2) have to applied to take in to account the still missed radiative correction and the high order terms
Standard expansion is not enough to describe the K→3dynamics
The slopes has been remeasured as (slightly different definition wrt to the PDG definition):
g = (64.9 0.3stat. 0.4syst. )% h’ = (–4.7 0.7stat 0.5syst.)%k’ = (0.970.03stat.0.08syst.)%
g = (64.9 0.3stat. 0.4syst. )% h’ = (–4.7 0.7stat 0.5syst.)%k’ = (0.970.03stat.0.08syst.)%
First evidence of k≠0
Preliminary
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ConclusionsConclusions
NA48/2NA48/2 exploited two different procedure to measure the scattering lengths.
Ke4Ke4: the phase shift can be related to the a0 and a2 using theoretical input (e.g. Roy equations)
K→K→: the scattering lengths are extracted from the study of rescattering contribution in the m mass distribution (the error is dominated by the theoretical error)
Applying the isosping breaking corrections the two results are fully compatible
The results are compatible with the DIRAC experiment results
NA48/2 Ke4NA48/2 Cusp
DIRAC band (prel. 2007)
Isospin breaking corrections applied both in Cusp and in Ke4 (work ongoing (see Gasser talk at Kaon07) )
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SparesSpares
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MeMe slope: 2D fit slope: 2D fit
Fs=fs+fs’q2+fs’’q4+fe’(Me2/4m
2)+...
f’’s f’s
f’s -0.96 0.03
f’’s -0.06 In the 1D fit a residual variation is observed with respect to Me
2D in (M, Me
) performed
Linear depence with Me
f’e/fs = 0.081±0.011±0.008
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Ke4: isospin breaking correctionKe4: isospin breaking correction
See Gasser’s talk @ Kaon 2007Kaon 2007
Thanks to the indipendent bin analysis the correction can be applied also to old data coming from previous experiment
The results become compatible with the cusp’s results
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Fit resultsFit results
K-
K+
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Cusp fit (in 2003)Cusp fit (in 2003)
420/148420/148
155/146155/146
149/145149/145
145/139145/139
One loop
Two loops
Pionium
Excluding 7 bins
Standard Dalitz plot parameterization
=(data-fit)/data
|M(u,v)|2 ~1+gu+hu2+kv2+...
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Dirac experimentDirac experiment The |a0-a2| quantity can be extracted from the
measurement of the lifetime of pionic atoms in a model independent way
The ionized exotic atoms are produced in a fixed target
Lifetime in the order of 3 fs
ChPt predicts with high accuracy this lifetime
p is the 0 momentum and corrections
Physics Letters B 619 (2005) 50
|a0-a2|=0.264+0.033-0.020
expected error in 2007: +7.4%, -4.2%
)1(||9
21 220
3
aap
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Spectrometer alignmentSpectrometer alignment
P = P0∙(1+β)∙(1+qbP0)
B signKaon sign
Raw momentum
Eq. Sensitivity (on DCH4):
M/x 1.5 keV/m
The kaon mass depends from the time variation of the spectrometer alignment
The mis-alignment gives a mis-measurement of the charged pion momentum
The reconstructed invariant K mass is used to fine tune the spectrometer by imposing (correction ) : MK+ =MK-
The non-perfect field alternation is tuned by imposing ( correction): MK+-=MKpdg
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Beam movementsBeam movements
DCH1DCH1(upstream magnet)(upstream magnet)
K+ K
X, cm
Large time scale movement: the beam positions change every run
Acceptance largely defined by central beam hole edge (~10 cm radius)
The cut is defined around the actual beam position obtained with the c.o.g. measured run by run, for both charges as a function of the K momentum (“virtual pipe” cut)
Short time scale movement: the beam moves during the SPS spill
Monitored with an high resolution beam monitor on the beams
The 2 beam movement is “coherent”
No effect in the 4-uple ratio
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““blue field”blue field”
The Earth field (Blue Field) was directly measured and used at the vertex recostruction level. The residual
systematics is ΔΔ<10<10-5-5
P kick(stray field)P kick(spectrometer) 1010
-4-4