Measurement of spectral function in the decay τ − → π π ν − 0 τ
Yukiko Hirano
(Nara Women’s Uni. , High Energy Physics Lab.)
For the Belle collaboration
1. Motivation
~ Muon Anomalous Magnetic Moment ~
2. Event selection
3. mass spectrum (unfolding)
4. Evaluation of
5. result
2 g
µ−
ππ
0a
µππOutline
Motivation Motivation
~ ~ Muon Muon Anomalous Magnetic Moment ( ) ~ Anomalous Magnetic Moment ( ) ~ g µ − 2
Muon Anomalous Magnetic Moment : 2
a g 2
µ = µ −
¾ The prediction of Standard Model
γ
µ µ
Z ,
SM QED EW had had LBL
a µ = a µ + a µ + a µ + a µ γ
γ
µ µ
hadron
γ
µ µ
a µ had
hadron
γ
µ largest error from
Hadron vacuum polarization
and and τ → ππ ν 0 τ decay decay
a µ had
the contribution of hadrom Vacuum polarization ( )
obtained from Experimental Data.
γ
µ µ
ν
ττ
W
−π
π
0ρ e
e
π
+π
−a
µhaddifficult to obtain from first principle !
hadron e e
+ −→
Cross section of
τ Semi-Leptonic decay
Hadron system
Hadron system
decay is
useful to determine the term ,
0 τ
τ → ππ ν
a µ had
73% from system 2 π
and decay and decay
a µ ππ τ → ππ ν 0 τ
Hadron Vacuum polarization term from 2 system ( ) a
µππ0 2
2
4
(0) ( )
em ( )
M K s v
a ds
s s
π
ππ ππ µ
α π
= ∫ ∞ s = M
ππ2Spectral function
0 0
0 0
2 1
2 2 2
( ) 1 1 2
6
1
ud EW e
M s s dN
v s
M
B
N
V S M B d s
ππ ππ
ππ τ
τ τ
ππ
π
−= − +
ππ 0 mass square spectrum
π
K(s) is known function.
is measured in this experiment.
N
0ds
π 0
1 dN
ππ
π
Present status ;
Present status ; Muon Muon Anomalous Magnetic Moment ( ) Anomalous Magnetic Moment ( ) g
µ− 2
¾ Exp. ・・・ measured by BNL (g-2) experiment. ( 2002.9 )
¾ Theoretical prediction ・・・ new data (CMD-2) and data (ALEPH)
( 2003.1 )
exp 10
(11659203 8) 10 a
µ= ± ×
−+ −
e e + − τ
( )
10exp 10
11659193.6 5.9( ) 3.5( ) (9.4 10.5) 10
0.4 ( ) 10
SM
SM
had LBL QED EW
a
a a
µ
µ µ −
= ± ± ± +
−− = ×
×
± ⇒
• τ base
0.9 σ
agree within
( )
exp 1
10 0
11659169.3 7.0( ) 3.5( ) 0.4( ) 10
(33.7 11.2) 1 0
SM
SM
had LBL QED EW
a
a a
µ
µ µ
−
−
= ± ± ± +
− ×
×
± ⇒
=
• e e base
3.0 σ
difference by
・Hadron Vacuum Polarization. term is different between and base predictions.
・ Cross check is important !
e e
+ −τ
event selection event selection e e + − → τ τ + −
•Number of charged tracks : 2 or 4
•All charge ( ) = 0
•event vertex position :
•Separate the event into 2 hemisphere by the event axis.
•Event axis direction :
•Back Ground rejection (next slide)
•Physics trigger
∆ Q
2.5 cm , 0.5 cm
z r
V < V <
35
D< θ
*< 145
DVJGQVJGTJGOKURJGTG
QPGJGOKURJGTG
ǫ
ǫ
e e
+ −→ τ τ
+ −event selection criteria
(corresponding to production.) 4.0 10 ×
6τ τ
+ −Event selection Event selection
Data : accumulated from 2000.10 to 2000.12 at Belle. 4.43 fb − 1
event selection (Back ground rejection) event selection (Back ground rejection)
e e + − → τ τ + −
( )
22
track
e e
p p p
MM =
++
−− ∑ − ∑ p
γ
Missing mass and Missing angle cut ( plot)
Missing angle
Missing Mass(MM)
pe+
track
p
θmiss
track
p
pγ pγ
pe−
•Bhabha , and two photon rejection e e
+ −→ µ µ γ
+ −( )
•Hadron( ) rejection e e
+ −
Reject high-multiplicity event ( X
part≡ ( n
track+ n
γ)
one× ( n
track+ n
γ)
other≤ 25 )
V.S. mi s
s
MM θ
θ∗miss
MC
(degree)
Missing Mass (Gev)
0 2 4 6 8 10
0 25 50 75 100 125 150 175 200
Missing Mass ( G eV)
Missing Angle
MC ( τ τ
+ −)
Two photon BG
Bhabha BG
0 2 4 6 8 10
0 25 50 75 100 125 150 175 200 θ∗miss
Data
(degree)
Missing Mass (Gev)
Data
Missing Mass ( G eV)
Missing Angle
τ τ
+ −
→
+ −Event selection Event selection
0 τ
τ → ππ ν
π
0selection criteria
0 τ
τ → π π ν
•one charged track in hemisphere.
•one in the hemisphere.
gamma condition : gamma-like shower shape :
• veto the additional gamma
(with high momentum (more than 200 MeV/c))
π 0
0.08
GeVE
γ>
* We do analysis each hemispheres. τ → ππ ν
0 τsignal signal
π 0
(mγγ - mπ0)/σγγ
number of entries / 0.19
DATA MC(signal) MC(non-τ B.G.)
Normalization:
# of entries
0 5000 10000 15000 20000 25000
-8 -6 -4 -2 0 2 4 6 8
( m m
0) S
γγ γγ πσ
γγ≡ −
0 Mass0
: (134.98
MeV) m
ππ
:
: m
m
γγ
γγ γγ
γγ σ
invariant mass distribution resolution of
6 S
γγ5
− < <
Signal region
9 7
7 9
S S
γγ γγ
− < < −
< <
right:
left:
Side-band region
320,000 τ → ππ ν
0τ events.
Side-band region are used for
estimation of BG in signal region.
( ) 11
4
left right
si total
sig an l sig de side
N = N − N + N ×
π
010 102 103 104
0.5 1 1.5 2 2.5 3
(Mπ±π0)2 (GeV)2
number of entries
/0.05(GeV)2DATA MC(signal) τ-feed across (Kπ0) τ-feed across (others) non-tau B.G.
Normalization:
# of entries
mass spectraum mass spectraum ππ 0
B.G. fraction
Total
( ) ( ) Feed across B.G.
Two photon non- B.G.( )
B.G. fraction source
Clear peak of .
is dominant .
(770) ρ
τ → ρν
τpeak.
is also included . (1450)
ρ
τ → ρν ′
τee → qq 2.3 ± 0.06 % 0.14 ± 0.01 %
6.1 ± 0.10 % 1.74 ± 0.09 % 5.43 ± 0.08 % K π
02
0h ≥ π ν
τ
Unfolding Unfolding
Acceptance and bin-by-bin migration effects are corrected via Singular-Value-Decomposition method.
0 0.5 1 1.5 2 2.5 3
0 0.5 1 1.5 2 2.5 3
(Mππ0)2 (observe) (GeV)2
(M ππ0)2 (generate) (GeV)2
0 0
2 2
V.S.
gen obs
M
ππM
ππ0 0.05 0.1 0.15 0.2 0.25 0.3
0.5 1 1.5 2 2.5 3
(Mππ0)2
acceptance
(GeV)2
acceptance
Acceptance include both the
tau-pair and pipi0 selection. Mass square resolution : 0.03 GeV
2Unfolded mass spectrum Unfolded mass spectrum
1 10 10
210
310
410
50 0.5 1 1.5 2 2.5
(Mππ0)2 (GeV)2
mass spectrum (unfolded) Belle
number of entries /0.05(GeV)
2Data
G & S Fit
(ρ(770) + ρ(1450))
Red line :
Breit Wigner fitting function ( and are included. ) ρ ρ ′
ρ
ρ ′
Breit
Breit Wigner Wigner fitting form fitting form
( )
2
2 2
2 3
'
( )
( )
1 1 2
1 ( ) 12
( ) 1
1
i i
s s
M M
F s
F s BW e
dN v s d
B s
W v
e
s A τ τ
π π
π φ
φ ρ ρ
β
β
β
= − + ⋅
=
= + ⋅
+
0
0
2
2
;
( ) ; M s
s dN ds
v
M
ππ
=
ππmass distribution
Spectral function
, , , , , ,
A M ρ Γ ρ M ρ ′ Γ ρ ′ β φ
free parameter
2
(
2) ( ) ( )
GS
d
BW s f s i s
M M
M s
ρ ρ ρ
ρ ρ
ρ
+ ⋅ ⋅
= − + − ⋅
Γ
Γ
Gounaris and Sakurai (G&S) Model
GS model is known that it can fit wilder
mass region that the commonly used BW.
fit result and compare with previous Experiments fit result and compare with previous Experiments
Mρρ
Γ
βM
ρρ′′
Γ2
..
dof
χ
0.5 1.1
775.3 150.5
±
± 7 26
1365 356
±
±
0.108
− ± 0.007
26.8/24
(fixed)
180.0
≡
0.9 1.6
776.4 150.5
±
± 16
(fixed)
1400 310
±
≡
0.077
− ± 0.008
54/65
(fixed)
180.0
≡
ALEPH CLEO
Belle
Fit Parameter
M ρ Γ ρ
(MeV) (MeV)
M ρ
ρ
′
Γ ′
(MeV) (MeV)
0.4 0.7
773.9 152.4
±
± 21 40
1398 450
±
±
35.6/42
0.085 ± 0.010
181.0 ± 6.2
β
φ (degree)
2 d o f. .
χ
• parameters : good agreement with previous Exp.
• parameters : Belle results are most precise.
ρ
ρ ′
Evaluation of Evaluation of a ππ µ
0 0
0 0
2 1
2 2 2
1 1 2
6
( ) 1
ud EW e
s s B dN
M
M M B
V S s
s N
v d
ππ ππ
π
τ τ
π τ π
π
π
−= − +
0 2
2
4
(0) ( )
em ( )
M K s v
ds s
a s
π
ππ ππ µ
α π
= ∫ ∞
(tau mass)
(Electro-Weak correction factor) (element of CKM matrix)
(Br. of )
e
E ud
e e
W
M S V
B
τ ν ντ
→
Systematic error (
Systematic error ( Ⅰ Ⅰ ) )
External systematics ~Normalization factors~
total
value source
1.0199 0.0006 0.9734 0.0008
±
±
( )
( )
%
%
17.84 0.06 25.41 0.11
±
±
a ππ µ
∆
(10−10)
S
EWV
udB
eB
ππ00.32 0.42
±
±
1.82 2.30
±
±
± 2.98
Largest error from B
ππOSystematic error (
Systematic error ( Ⅱ Ⅱ ) )
Internal systematics 1.Non- BG.
・ estimated by B.G. MC.
・ control data sample are used for the calibration.
2. Feed-across
・ of measured Br.
3. Energy scale
・ uncertainty estimated from mass peak.
4. Selection
・ estimated from the uncertainty of side-band.
5. minimum energy
1 σ
π
0π
0γ τ
efficiency
B.G. fraction B.G. estimation
total
Use side-band
non- BG
80MeV – 200MeV
Minimum energy Energy scale
Feed across BG
2 photon hadron
non- BG
comment
source
K
−π
02
0h ≥ π ν
π
0γ τ
a ππ µ
∆
(10−10)
2.3
± 0.06% 0.14
±0.01%
1.74
±0.09% 5.43
± 0.08%
0.05 0.4
±
± 0.3 1.2
±
±
± 0.1
1.8 0.8
±
±
± 2.36
π0
/ 0.2% ( 0)
E E π
∆ = ±
result result
Result of is … a
ππµ( 541.3 2.0 ( stat .) 2.36 ( sys .) 2.98 ( sys ext . .) ) 10 10
a µ ππ = ± ± ± × −
2 2 2
Integrated mass sqr. region : 4 m
πto (1.8 )
GeVpreli mina ry
cf. ALEPH
( 533.86 3.57( ) 2.36( ) ) 10
10a
ππµ= ± stat ± sys ×
−( base) τ
2 2 2
Integrated mass sqr. region : 4 m
πto (1.8 )
GeV( )
2 2
7.4 1.6 4.7
ALEPH
Belle ALEP Be e
H
a
µ lla
µσ σ
− = =
− excluding common error
Consistent within error
Backup slide
Analysis Analysis
Flow of this analysis Flow of this analysis
Data from Belle
Unfolding (reject detector contribution)
Spectral function measurement
Calculation of the term hadron vacuum polarization event selection
0 τ
τ → ππ ν
event selection e e
+ −→ τ τ
+ −mass spectrum of Data
ππ
0decide mass spectrum ππ
02.Event selection 2.Event selection
Exp. Data
Monte Carlo simulation
Belle detector
Data taking system Raw Data
Simulator of event production
Detector simulation
Data reconstruction event selection
τ τ
+ −event selection
0 τ
τ ππ ν →
event
0 τ
τ → ππ ν
event τ τ
+ −τ τ
+ −Used Data
data accumulated from 2000.10 to 2000.12 at Belle
data :
4.44 fb − 1
4.0 10 ×
6event selection event selection e e + − → τ τ + −
• There are few charged tracks in the event.
e
+τ
+e
−τ
−e
+τ
+e
−τ
−decay to 1 charged track : about 85%
decay to 3 charged tracks : about 15%
τ τ
72% 13%
• There are missing of momentum and mass because of neutrino ( ) . ν
decay
τ
ντ
τ
W−
π
π0
ρ
missing
event selection (Back ground rejection) event selection (Back ground rejection)
e e + − → τ τ + −
•Bhabha , and two photon rejection e e
+ −→ µ µ γ
+ −( )
clean Bhabha and mumu event rejection : ∑ P ≤ 9.0
GeV/c, ∑ E ≤ 9.0
GeV( )
22
track
e e
p p p
MM =
++
−− ∑ − ∑ p
γ0 2 4 6 8 10
0 25 50 75 100 125 150 175 200 θ∗miss
Data
(degree)
Missing Mass (Gev)
θ∗miss
MC
(degree)
Missing Mass (Gev)
0 2 4 6 8 10
0 25 50 75 100 125 150 175 200
Missing mass and Missing angle cut
Missing angle
Missing Mass(MM) pe+
track
p
θ
misstrack
p
pγ
pγ
pe−
•Hadron( ) rejection e e
+ −( ) ( ) 25
part track one track other
X ≡ n + n γ × n + n γ ≤
Low-multiplicity event :
Then ,we obtained about 1,300,000 event of . e e
+ −→ τ τ
+ −Missing mass VS. Missing angle Missing mass VS. Missing angle
0 2 4 6 8 10
0 50 100 150 200 0 2 4 6 8 10
0 50 100 150 200
0 2 4 6 8 10
0 50 100 150 200 0 2 4 6 8 10
0 50 100 150 200
θ∗miss (degree) (1)Data
Missing Mass (Gev)
θ∗miss (degree) (2)MC(τsample)
Missing Mass (Gev)
θ∗miss (degree) (3)MC(Bhabha,mumu)
Missing Mass (Gev)
θ∗miss (degree) (4)MC(2photon)
Missing Mass (Gev)
Data MC(tau)
MC(Bhabha) MC(2photon)
Time dependence
10 cm
BELLE
0.246 0.248 0.25 0.252 0.254 0.256 0.258 0.26 0.262 0.264
8 9 10 11 12 13 14 15 16 17 18 19 20
∆R/Rave= ± 0.5 %
average=0.2568
2000 2001 2002
Exp. Number R = N
hπ0/ N
ττdata at Belle detector
τ
Time dependence of event ππ
0is stable within 0.5%.
N
0N
ππ ττ
Time dependence
0.246 0.248 0.25 0.252 0.254 0.256 0.258 0.26 0.262 0.264
8 9 10 11 12 13 14 15 16 17 18 19 20
∆R/Rave= ± 0.5 %
average=0.2568
2000 2001 2002
Exp. Number R = N
hπ0/ N
ττTime dependence of event ππ
0is stable within 0.5%.
N
0N
ππ ττ
Momentum of and
Momentum of and π 0 π ±
0 1000 2000 3000 4000 5000 6000 7000 8000 9000
0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1
Ph±(CM) / EBeam (GeV)
number of entries / 0.01
DATA MC(signal) non-tau B.G.
Normalization:
number of entries
π ±
0 2000 4000 6000 8000 10000
0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1 Pπ0 (CM) / EBeam (GeV)
number of entries / 0.01
DATA MC(signal) non-tau B.G.
Normalization:
number of entries
π 0
Good agreement between Data and MC .
Fitting result of Breit Wigner model Fitting result of Breit Wigner model
1 10 102 103 104 105
0 0.5 1 1.5 2 2.5
(Mππ0)2 (GeV)2
mass spectrum (unfolded) Belle
number of entries /0.05(GeV)2
Data
G&S Fit(ρ(770))
G&S Fit(ρ(770) + ρ(1450))
1 10 102 103 104 105
0 0.5 1 1.5 2 2.5
(Mππ0)2 (GeV)2
mass spectrum (unfolded) Belle
number of entries /0.05(GeV)2
Data
K&S Fit(ρ(770))
K&S Fit(ρ(770) + ρ(1450))
G&S model
K&S model
Fitting result Fitting result
G&S G&S
K&S K&S
0.39 0.68 18.9 41.5 0.020
9.05 38.8/ 42
773.07 150.76 1421.7 542.28 0.14 188.4
0.93
±
±
±
±
±
±
=
'
( is real)
ρ ρ β + ρ ρ β φ +
'( , used) ρ ρ β +
'( is real) ρ ρ β φ +
'( , used)
'
'
2 do f . .
M
M
ρ ρ
ρ ρ
β φ
χ
Γ Γ
0.36 0.66 6.6
29.6 0.005
40.9/ 43
773.25 150.58 1397.8 514.77
0.120
0.93
±
±
±
±
±
=
−
0.35 0.69 6.3 28.5
0.004
35.6/ 43
773.94 152.37 1395.0
445.9 0.084
0.83
±
±
±
±
±
=
−
0.37 0.71
20.9 39.9 0.010 6.17 35.6/ 42
773.9 152.4 1398.2
450.4 0.085 180.0
0.85
±
±
±
±
±
±
=
Unfolding of invariant mass Unfolding of invariant mass
The observed distribution includes contribution of detector acceptance ,and smeared .
We can obtain true distribution by using Unfolding.
About Unfolding
Detector
unfolding
initial distribution obserbed distribution
Unfolding is carried out by
Singular Value Decomposition (SVD) method.
method a la ALEPH , A.Hocker, V.Karvelishvili,N.I.M. 372(1996)469
Spectral function Spectral function
10
-310
-210
-11
0 0.5 1 1.5 2 2.5
(Mππ0)2 (GeV)2
Belle
v
(M2 )Belle CLEO
Systematic detail 1 Systematic detail 1
(1) BG estimation (two photon )
Data MC (two photon)
Two photon B.G. estimated by Data using control sample.
(2) BG estimation (hadron)
Hadron BG contribution also estimated by Data using control sample.
( ) ( ) 25 for selection
part track one track other
X ≡ n + n
γ× n + n
γ≤ τ
for hadron selecti
( ) ( ) 2 5 o n
part track one track other
X ≡ n + n
γ× n + n
γ>
Systematic detail2 Systematic detail2
(3) Energy scale
2% uncertainty of mass spectrum is assumed. π
0(4) Gamma energy threshold
(5) side-band subtraction π
0Uncertainty of as gamma-threshold function. B h ( π
0)
24.6 24.8 25 25.2 25.4 25.6 25.8 26 26.2 26.4
0.05 0.1 0.15 0.2 0.25 0.3 0.35 0.4 0.45 0.5 0.55
∆B/B= 1.0 %
gamma theshold energy B(hπ0 )
(%)
(GeV)
Use control sample of side-band . π
0Hadron Vacuum polarization and
Hadron Vacuum polarization and e e + − Data Data
e e
+ −→ hadron
The term of hadron vacuum polarization
e
+γ
e
−q
q
γ e
+