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F. Ambrosino Euridice Midterm Meeting LNF 11/02/05 1 F.Ambrosino F.Ambrosino Università e Sezione INFN, Napoli Università e Sezione INFN, Napoli for the KLOE collaboration for the KLOE collaboration Study of Dalitz plot at KLOE •Motivations •Conclusions and outlook

F.Ambrosino Università e Sezione INFN, Napoli for the KLOE collaboration

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Study of h  ppp Dalitz plot at KLOE. F.Ambrosino Università e Sezione INFN, Napoli for the KLOE collaboration. Motivations h  p + p - p 0 h  p 0 p 0 p 0 Conclusions and outlook. h  3p in chiral theory. The decay h  3 p occours primarily on account of the d-u - PowerPoint PPT Presentation

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Page 1: F.Ambrosino Università e Sezione INFN, Napoli for the KLOE collaboration

F. Ambrosino Euridice Midterm Meeting LNF 11/02/05

1

F.AmbrosinoF.AmbrosinoUniversità e Sezione INFN, NapoliUniversità e Sezione INFN, Napoli

for the KLOE collaborationfor the KLOE collaboration

Study of Dalitz plot at KLOE

•Motivations•

•Conclusions and outlook

Page 2: F.Ambrosino Università e Sezione INFN, Napoli for the KLOE collaboration

F. Ambrosino Euridice Midterm Meeting LNF 11/02/05

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The decay occours primarily on account of the d-uquark mass differences and the result arising from lowest order chiral pertubation theory is well known:

222

2

2

2 33),,()(1),,(

FutsMmm

mm

QutsA K

K

With: 22

222 ˆ

ud

s

mmmm

Q

A good understanding of M(s,t,u) can in principle lead to a very accurate determination of Q:

42)3( QA

in chiral theory

22

243),,(

mmmsutsM

And, at l.o.

Page 3: F.Ambrosino Università e Sezione INFN, Napoli for the KLOE collaboration

F. Ambrosino Euridice Midterm Meeting LNF 11/02/05

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Still there are some intriguing questions for this decay :

•Why is it experimental width so large (270 eV) w.r.t theoretical calculation ? (Tree level: 66 eV (!!!); 1 loop : 160 eV ) Possible answers:

•Final state interaction•Scalar intermediate states •Violation of Dashen theorem

•Is the dynamics of the decay correctly described by theoretical calculations ?

…and its open questions

Page 4: F.Ambrosino Università e Sezione INFN, Napoli for the KLOE collaboration

F. Ambrosino Euridice Midterm Meeting LNF 11/02/05

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The usual expansion of square modulus of the decay amplitude about the center of the Dalitz plot is:

|A(s,t,u)|2 = 1 + aY + bY2 + cX + dX2 + eXY

Where: tu

QM

23

QTT3X -

12

313 200 smm

QmQTY

02 mmmQ

Dalitz plot expansion

Page 5: F.Ambrosino Università e Sezione INFN, Napoli for the KLOE collaboration

F. Ambrosino Euridice Midterm Meeting LNF 11/02/05

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Tabella sperimentale di Bijnens

Calculation a b dTreeOne-loop[1]Dispersive[2]Tree dispersiveAbsolute dispersive

-1.00 0.25 0.00-1.33 0.42 0.08-1.16 0.26 0.10-1.10 0.31 0.001-1.21 0.33 0.04

Measurement N a b dLayterGormley Crystal BarrelCrystal Barrel

808843000010773230

-1.08 0.14 0.034 0.027 0.046 0.031-1.17 0.02 0.21 0.03 0.06 0.04 -0.94 0.15 0.11 0.27-1.22 0.07 0.22 0.11 0.06 fixed

[1] Gasser,J. and Leutwyler, H., Nucl. Phys. B 250, 539 (1985) [2] Kambor, J., Wiesendanger, C. and Wyler, D., Nucl. Phys. B 465, 215 (1996)

Dalitz expansion: theory vs experiment

Page 6: F.Ambrosino Università e Sezione INFN, Napoli for the KLOE collaboration

F. Ambrosino Euridice Midterm Meeting LNF 11/02/05

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At KLOE is produced in the process .The final state for is thus , and the final state for is 7, both with almost no physical background.

at KLOE

Selection:• 2 track vertex+3 candidates• Kinematic fit

Page 7: F.Ambrosino Università e Sezione INFN, Napoli for the KLOE collaboration

F. Ambrosino Euridice Midterm Meeting LNF 11/02/05

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Resolutions and efficiency“core” X =

0.018

“core” Y =

0.027

Efficiency almost flat, and 36%

Page 8: F.Ambrosino Università e Sezione INFN, Napoli for the KLOE collaboration

F. Ambrosino Euridice Midterm Meeting LNF 11/02/05

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Comparison Data-MC:

Page 9: F.Ambrosino Università e Sezione INFN, Napoli for the KLOE collaboration

F. Ambrosino Euridice Midterm Meeting LNF 11/02/05

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Comparison Data-MC:

Page 10: F.Ambrosino Università e Sezione INFN, Napoli for the KLOE collaboration

F. Ambrosino Euridice Midterm Meeting LNF 11/02/05

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SignalB/S 0.8%

Page 11: F.Ambrosino Università e Sezione INFN, Napoli for the KLOE collaboration

F. Ambrosino Euridice Midterm Meeting LNF 11/02/05

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The analysis has been applied on 450 pb–1 corresponding to:

N(+-0) = 1,425,131

events in the Dalitz plot, fitted with function:

• fit is stable…• …but the model seems not to fit adeguately data (BAD P

2).We have added the cubic terms:

|A(X,Y)|2 = 1+aY+bY2+cX+dX2+eXY+fY3+gX3+hX2Y+lXY2

|A(X,Y)|2 = 1+aY+bY2+cX+dX2+eXY

Fitting function

Page 12: F.Ambrosino Università e Sezione INFN, Napoli for the KLOE collaboration

F. Ambrosino Euridice Midterm Meeting LNF 11/02/05

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Fit stability

Page 13: F.Ambrosino Università e Sezione INFN, Napoli for the KLOE collaboration

F. Ambrosino Euridice Midterm Meeting LNF 11/02/05

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ndf P2

%

a b c d e f

147 60 -1.072 0.006-0.007 +0.005

0.117 0.006-0.006 +0.004

0.0001 0.0029-0.0021 +0.0003

0.047 0.006-0.005 +0.004

-0.006 0.008

-0. +0.013

0.13 0.01-0.01 +0.02

150 63 -1.072 0.005-0.008 +0.005

0.117 0.006-0.006 +0.004 ---

0.047 0.006-0.005 +0.004

0.13 0.01-0.01 +0.02

150 0.02 -1.055 0.004-0.007 +0.006

0.100 0.005-0.002 +0.004

--- --- ---0.12 0.01

-0.02 +0.02

150 0 -1.013 0.003-0.007 +0.004

0.120 0.005-0.023 +0. ---

0.043 0.006-0.003 +0.004

--- ---

Results

150 63 -1.072 0.005-0.008 +0.005

0.117 0.006-0.006 +0.004 ---

0.047 0.006-0.005 +0.004

0.13 0.01-0.01 +0.02

|A(X,Y)|2 = 1+aY+bY2+cX+dX2+eXY+fY3

Page 14: F.Ambrosino Università e Sezione INFN, Napoli for the KLOE collaboration

F. Ambrosino Euridice Midterm Meeting LNF 11/02/05

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Results (II)

|A(X,Y)|2 = 1-1.072 Y+0.117 Y2+0.047 X2+0.13Y3

Using preliminary KLOE results shown at ICHEP 04 B.V. Martemyanov and V.S. Sopov (hep-ph\0502023) have extracted:

Q = 22.8 ± 0.4 against Qdashen= 24.2 (as already argued for example in J. Bijnens and J. Prades, Nucl. Phys. B490, 239 (1997)

Page 15: F.Ambrosino Università e Sezione INFN, Napoli for the KLOE collaboration

F. Ambrosino Euridice Midterm Meeting LNF 11/02/05

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The dynamics of the decay can be studied analysing the Dalitz plot distribution. The Dalitz plot density ( |A|2 ) is specified by a single parameter:

|A|2 1 + 2zwith:

2max

22

3

1

)3

3(

32

0

i

i

mmmE

z

Ei = Energy of the i-th pion in the rest frame. = Distance to the center of Dalitz plot.max = Maximun value of .

Z [ 0 , 1 ]

Dalitz plot expansion

Page 16: F.Ambrosino Università e Sezione INFN, Napoli for the KLOE collaboration

F. Ambrosino Euridice Midterm Meeting LNF 11/02/05

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Alde (1984) -0.022 0.023Crystal Barrel (1998) -0.052 0.020Crystal Ball (2001) -0.031 0.004

Dalitz expansion: theory vs experiment

Calculation TreeOne-loop[1]Dispersive[2]Tree dispersiveAbsolute dispersive

0.000.0015-0.007 - -0.014-0.006-0.007

[1] Gasser,J. and Leutwyler, H., Nucl. Phys. B 250, 539 (1985) [2] Kambor, J., Wiesendanger, C. and Wyler, D., Nucl. Phys. B 465, 215 (1996)

Page 17: F.Ambrosino Università e Sezione INFN, Napoli for the KLOE collaboration

F. Ambrosino Euridice Midterm Meeting LNF 11/02/05

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Recoil is the most energetic cluster.In order to match every couple of photon to the right 0 we build a 2-like variable for each of the 15 combinations:

23

1

2

0

00

ij

m

j

j

Mmi

With:j

oi

m is the invariant mass of i

0 for j-th combination0

M = 134.98 MeVj

m 0 is obtained as function of photon energies

Photons pairing

Page 18: F.Ambrosino Università e Sezione INFN, Napoli for the KLOE collaboration

F. Ambrosino Euridice Midterm Meeting LNF 11/02/05

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Cutting on: Minimum 2 value 2 between “best” and “second” combination

One can obtain samples with different purity-efficiencyPurity= Fraction of events with all photons correctly matched to ‘s

Combination selection

Pur 85 % Eff 22 %

Pur 92 % Eff

14 %

Pur 98 % Eff 4.5 %

Page 19: F.Ambrosino Università e Sezione INFN, Napoli for the KLOE collaboration

F. Ambrosino Euridice Midterm Meeting LNF 11/02/05

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The problem of resolution

Phase spaceMC reconstructed

Resolution Efficiency

Page 20: F.Ambrosino Università e Sezione INFN, Napoli for the KLOE collaboration

F. Ambrosino Euridice Midterm Meeting LNF 11/02/05

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Results on MC

Page 21: F.Ambrosino Università e Sezione INFN, Napoli for the KLOE collaboration

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Results on MC

Page 22: F.Ambrosino Università e Sezione INFN, Napoli for the KLOE collaboration

F. Ambrosino Euridice Midterm Meeting LNF 11/02/05

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Results on MC

Page 23: F.Ambrosino Università e Sezione INFN, Napoli for the KLOE collaboration

F. Ambrosino Euridice Midterm Meeting LNF 11/02/05

23The agreement is good on all spectra

Comparison Data - MC

Page 24: F.Ambrosino Università e Sezione INFN, Napoli for the KLOE collaboration

F. Ambrosino Euridice Midterm Meeting LNF 11/02/05

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= -0.0ZZ 0.004̂

Low purity Medium purity High purity

= -0.0XX 0.002 ̂ = -0.0YY 0.002̂

Fitting Data

Systematics are at the same level of the statistical error

Page 25: F.Ambrosino Università e Sezione INFN, Napoli for the KLOE collaboration

F. Ambrosino Euridice Midterm Meeting LNF 11/02/05

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Conclusions

• KLOE is analyzing an unprecedented statistics of decays with negligible background

• For channel the analysis is almost completed and finds evidence for an unexpected large y3 term

• 3 analysis is much harder, we expect to provide soon a result at the same level of the Crystal Ball one.

Page 26: F.Ambrosino Università e Sezione INFN, Napoli for the KLOE collaboration

F. Ambrosino Euridice Midterm Meeting LNF 11/02/05

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SPARE SLIDES

Page 27: F.Ambrosino Università e Sezione INFN, Napoli for the KLOE collaboration

F. Ambrosino Euridice Midterm Meeting LNF 11/02/05

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Kinematic fit with no mass constrains

Page 28: F.Ambrosino Università e Sezione INFN, Napoli for the KLOE collaboration

F. Ambrosino Euridice Midterm Meeting LNF 11/02/05

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Tests of the fit procedure on MC

Generator slopes in MC rad-04:

a = -1.04b = 0.14c = 0.d = 0.06e = 0.

KLOE measure (100 pb-1)

Page 29: F.Ambrosino Università e Sezione INFN, Napoli for the KLOE collaboration

F. Ambrosino Euridice Midterm Meeting LNF 11/02/05

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Comparison Data-MC

data MC

A.U

.

Page 30: F.Ambrosino Università e Sezione INFN, Napoli for the KLOE collaboration

F. Ambrosino Euridice Midterm Meeting LNF 11/02/05

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Comparison Data-MC: Ych – Y0

Shift 1.33 MeV

Shift 0.03 MeV

NA48: 547.843 0.030st 0.041sys

Physica Scripta T99 140-142, 2002

Page 31: F.Ambrosino Università e Sezione INFN, Napoli for the KLOE collaboration

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• i is for each bin: the efficiency as a function of Dalitz-plot.• Ni is for each bin: the number of events of Dalitz-plot.• i is the statistical error on the ratio Ni / i •All the bins are included in the fit apart from the bins crossed by the Dalitz plot contour.

The fit is done using a binned 2 approach

21

22

2

)),((

i

Nbin

i bini

i dXdYYXAN

Fit procedure

Page 32: F.Ambrosino Università e Sezione INFN, Napoli for the KLOE collaboration

F. Ambrosino Euridice Midterm Meeting LNF 11/02/05

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Comparison Data-MC: X & Y

Page 33: F.Ambrosino Università e Sezione INFN, Napoli for the KLOE collaboration

F. Ambrosino Euridice Midterm Meeting LNF 11/02/05

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Comparison between efficiency corrected data and fitted function as function of the bin number.The structure observed is due to the Y distribution for X slices

P(2 02) 60%

Goodness of fit

Page 34: F.Ambrosino Università e Sezione INFN, Napoli for the KLOE collaboration

F. Ambrosino Euridice Midterm Meeting LNF 11/02/05

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A = (-0.009 0.093) 10-

2

NNNNA

4321

4231

NNNNNNNNAq

Aq = (-0.02 0.09) 10-2

654321

642531

NNNNNNNNNNNNAs

As = (0.07 0.09) 10-2

Asymmetries

Page 35: F.Ambrosino Università e Sezione INFN, Napoli for the KLOE collaboration

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We have tested the effect of radiative corrections to the Dalitz plot density.

The ratio of the two plots has been fitted with the usual expansion: corrections to parameters are compatible with zero

Page 36: F.Ambrosino Università e Sezione INFN, Napoli for the KLOE collaboration

F. Ambrosino Euridice Midterm Meeting LNF 11/02/05

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time stabilityTo check stability wrt data taking conditions we fit the integrated Dalitz plot in samples of 4 pb-1 each

Page 37: F.Ambrosino Università e Sezione INFN, Napoli for the KLOE collaboration

F. Ambrosino Euridice Midterm Meeting LNF 11/02/05

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Check on cubic term

No cubic dependence in |A(X,Y)|2

|A(X,Y)|2 = 1 + aY + bY2 + dX2 with a -1.

Can evaluate such as to mimic the cubic term.

Fitted function is actually :

Real (X,Y)MC(X,Y)

|A(X,Y)|2

Assume:

Real (X,Y)MC(X,Y)

1+Y+X2

Page 38: F.Ambrosino Università e Sezione INFN, Napoli for the KLOE collaboration

F. Ambrosino Euridice Midterm Meeting LNF 11/02/05

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MCMC weighted

MCMC weighted

Page 39: F.Ambrosino Università e Sezione INFN, Napoli for the KLOE collaboration

F. Ambrosino Euridice Midterm Meeting LNF 11/02/05

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The cuts used to select: are :

7 and only 7 prompt neutral clusters with 21° < < 159°

and E > 10 MeV opening angle between each couple of photons >

18° Kinematic Fit with no mass constraint 320 MeV < Erad < 400 MeV P(2) > 0.01

Sample selection

Page 40: F.Ambrosino Università e Sezione INFN, Napoli for the KLOE collaboration

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Page 41: F.Ambrosino Università e Sezione INFN, Napoli for the KLOE collaboration

F. Ambrosino Euridice Midterm Meeting LNF 11/02/05

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Once a combination has been selected, one can do a second kinematic fit imposing 0 mass for each couple of photons.

Second kinematic fit

Page 42: F.Ambrosino Università e Sezione INFN, Napoli for the KLOE collaboration

F. Ambrosino Euridice Midterm Meeting LNF 11/02/05

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i

iin log

But now:

ni = recostructed eventsi = from each single MC recostructed event weighted with the theoretical function

Still we minimize:

Doing it the hard way..

Page 43: F.Ambrosino Università e Sezione INFN, Napoli for the KLOE collaboration

F. Ambrosino Euridice Midterm Meeting LNF 11/02/05

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The center of Dalitz plot correspond to 3 pions with the same energy (Ei = M/3 = 182.4 MeV). A good check of the MC performance in evaluating the energy resolution of 0 comes from the distribution of E0 - Ei for z = 0

Comparison Data – MC (II)

Page 44: F.Ambrosino Università e Sezione INFN, Napoli for the KLOE collaboration

F. Ambrosino Euridice Midterm Meeting LNF 11/02/05

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E*1 - E*2

Vs.

E

Comparison Data – MC (II)