Upload
zuzela
View
27
Download
0
Tags:
Embed Size (px)
DESCRIPTION
Recent Charm Semileptonic Decay Results. Content I : Charm Semileptonic decay motivation II : Semileptonic BF results from CLEO-c III: Fully leptonic results from BaBar/CLEO-c IV : Form Factors for PseudoScalar l n from FOCUS, BaBar &CLEO-c - PowerPoint PPT Presentation
Citation preview
1
Jim WissUniversity of Illinois
FPCP06April 11,2006
Content
I: Charm Semileptonic decay motivation
II: Semileptonic BF results from CLEO-c
III: Fully leptonic results from BaBar/CLEO-c
IV: Form Factors for PseudoScalar l from FOCUS, BaBar &CLEO-c
V: Vector l Form Factors from CLEO-c
VI: Summary.
Recent Charm Semileptonic Decay Results
Representing:
2
K-D
c W l
q
scsV
Charm semileptonic decay as tests of LQCD
Charm SL decays provide a high quality lattice calibration, which is crucial in reducing systematic errors in the Unitarity Triangle. The techniques validated by charm decays can be applied to beauty decays. Improvement of CKM @ beauty sector.
The hadronic complications are contained in the form factors, which can be calculated via non-perturbative Lattice QCD,
BF provides a measurement of |VCq|2
3
Semileptonic reconstruction in Cleo-c
e
K e
0
0
0
0
(3770)
,
D
D
D
D K eK
K-
-
e+
K+
0Example: D e
CLEO BFRelative to PDG
(~117 events)
Ev
ents
/ 1
0 M
eV
U ( = Emiss – |Pmiss| )
4
Inclusive Semileptonic BF.
CLEO-c 281 pb-1
0
0 0
0.985 0.028 0.015SL SL
D D DSL SL
D D D
B
B
Inclusive BF vs sum of exclusive BF
Consistent with the known exclusive modes saturating the inclusive . Some room for new modes?
mode
D0Xe+ (6.46 ± 0.17 ± 0.13)%
i i (D0 Xe+ (6.1 ± 0.2 ± 0.2)%
D+ Xe+ (16.13 ± 0.20 ± 0.33)%
i i (D+ Xe+ (15.1 ± 0.5 ± 0.5)%
Consistent w/ SL isospin symmetry:
5
22
222
2 18
= great LQCD test( ) / DDF
cqD DD
mGB D M V
Mfmf
Fully leptonic decays: D+ +and DS +
/ 1.25 0.14
As expected from LQCD
s
BaBar CLEOD Df f
279 17 6 M19 eVsD
f
* at (4S)S sD D
0 09
2 8
41
4
0 2
3
4 40 0 66 10
201 3
222 6 1
17
6 7
Fnal/Mil
.
.
.
c
.
.
. .
MeV
. MeV
D
D
f
B
f
D
Tag D
Signal D+
0 D K
50 signal candidates
489 55 signal
m m m
6
D Pseudoscalar l form factors
22 3
2 3
22 2
2(
4( ) )
F cq P
lf q O mG V Pd D P
dq
What do we know about f+(q2) ?
This process can give a clean measurement of CKM angles and powerful tests of LQCD
2q 2q
22( )f q
Ra
te
P3
Unfortunately the rate vanishes at highest q2 where sensitivity to the form of f+(q2) is greatest. This is also the zero recoil limit where theory calculations are cleanest.
7
Pole Dominance in K*l
2 22 2
2 1
*
Im(
()
)
DDm K
f sds
s qm if q
q
R
22
2
2 2 2
2
2
22 2
2
0
1 1
eff *
* *
*
*
*
*
HQET&SCET
Becirevic & Kaidalov write as
effective pole with
( )
( )
integral
Res & Po
/
(/
le
)
D D
D
D
D D
D D
D
m m
f q
f
c c m
m q
m
f qq m q
m q
m
2Dm K Re s
Im s
2*Dm
Cauchy Theorem
0 5 0 04. .
(2004)
<Mpole> is 5.1 lower than Ds*
22 2
1
+Fits to f ( )pole
qm q
c Integral term is important
Ds*
BK expression is a good fit to recent lattice calculations
8
RS-WS
MC WS
12,840 K +
m K m K
m cut
FOCUS D0 K + analysis
0*
Select
decay chain
D D
Fixed Target Neutrino closure
• Jump to K rest frame
• The D and D* mass constraints the neutrino lies on a cone around the soft pion.
• Pick the that points the D closest to the primary vertex.
q2 re
con
st
q2 actual
Kframe
K
2min
2maxq
2minq
Lab frame
• A good muon candidate.
• Cerenkov ID for K/ candidates.
• L/ > 5 between two good vertices.
• D* tag required, and wrong sign soft subtraction
9
Correcting for charm backgrounds inD0 K +
The background only affects the highest q2 bins.
0
0.5
1
1.5
2
2.5
0 0.5 1 1.5 2
after subtraction pole=1.9 before subtraction
2f q
2 2 4 (GeV / )q c
After subtracting known charm backgrounds, f+(q2) is an excellent match to a pole form withmpole= 1.91 0.04 0.05 GeV/c2 or = 0.32 (CL 87%, 82%).
10
Comparing to Lattice Gauge & prelim BaBar
2q (GeV )D 2
~100K
13K
Nearly identical q2 resolution!
11
Preliminary untagged DK/ e from CLEO-c
Slightly lower than previous measurements
Neutrinos are closed by energy-momentum balance but no recoil D tag
q2 resolution still about 10x better than FOCUS/BaBar
q2
CKM info Modified pole
12
DVector l Decay
H0(q2), H+(q2), H-(q2) are helicity-basis form factors computable by LQCD A new factor h0 (q2) is needed to describe s-wave interference piece.
2 22 2
2 22 2
22 222 20
2 2 20
2
(1 cos )sin ( )
(1 cos )sin ( )
1A 2sin cos ( )
8 sin cos ( ) ( ) e8
R
( )
l V
l V
l V
V
o
l
iH q h q
H q BW
H q BW
d q H q B
O
W
A
Ae BW
Korner+Schuler form from 1990
S-wave interfere asymmetry
cosV
Present in K* l nu
13
KS / GS model for H and H0
2V 2
1 1
Only 2 shape parameters needed
in spectroscopic pole
A (0)V(0) R = R =
A (0
dominance
) A
fit
(0)
2.1 2.5V A1 A2M GeV M M GeV
Spectroscopic pole dominance
22
2
2
*
* * "2
*
(1 )
(1 )(1 )
(1 )
1 '
'(1 ) 2 (1 ')
(1 ' )(1 '' )
2H'
H'1
H2
Ds*
Fajfer & Kamenik (
c qV where x
c A w
2005
here
)
cA
D
D K
D K K H
D K
aq
x ax m
a mq
b x m m
m m a m c aq
m m b x b x
B&K style “effective” poles
•V(q2) essentially same as B&K with one physical and one effective 1- poles.
•A1(q2) forced to one effective 1+ pole
•A2(q2) has two effective 1+ poles
Versus
This is traditional method
But S-pole dominance should work poorly at low q2 Need for alternative…
14
E6
87
E7
91
FO
CU
S
BE
AT
E6
91
E6
53
0.0
0.5
1.0
1.5
2.0
2.5
3.0 1.66 0.060
0.827 0.055R2
Spectroscopic pole dominance DVl fits
Ds D+ K
2V 2
1 1
A (0)V(0)R = R =
A (0) A (0)
The latest (FOCUS) data on Dsis consistent with D+ K
theory
theory
RV
R2
RV
15
A non-parametric approach
7 8 9
4 5 6
1 2 3
cosV
cosL
D: M+ M- M0
m vectors (angular bin)��������������
0
0
0 0 0 00
The projection weights can be computed directly
from the MC bin populations using linear algebra
I
I
I
P m m m m m m
P m m
m m
m m m m
m m m m m mP
m m
P
0
0
0
1
I
II I I I I
m m
m m m m m m m
m
m m
m
m
Disentangle helicity form factors based on their different angular bin populations.
Each Kπe candidate is given four weights based on its decay angles.
These weights project
Re
o
s
ut
ults appear as just 4 weighted histogram
H (q ) , H (q ) , H (q ) & H h (q )
s.
-+
n
´2 2 2 2 2 2 20 00
16
CL = 40%CL = 24%
CL = 59%CL = 0.2%
Preliminary CLEO D+ Kefrom 281/pb
20 0( )H h q
2 2( )H q
2 2( )H q
2 2( )oH q
FOCUS model
2 2 2 2
The CL are to the Focus model
Normalized so that
as 0 , ( ) 1 oq q H q
2 2q (GeV )
Low q2 peaking of Ho and ho is very apparent. Apart from interference term the CL are rather good.
17
Intensity contributions q2 H2(q2)
2 2q (GeV )
2 2 2( )q H q
2 2 2( )q H q
2 2 2
0( )q H q
2 20 0( )q H h q
H+ contribution vanishes at 0.
H- contribution vanishes at 0.
Subtle deviation of H0 from pure 1/q .
Confirms KS expected forms
18
Pole mass sensitivity
MV=2.1 MA=2.5
2 2 2( )q H q
q H (q )2 2 20
MV= MA=
2 2 2( )q H q
2 2 2( )q H q
2 2 2( )q H q
2 2 20q H (q )
Data fits spectroscopic poles and constant form factors equally well
19
Confirming the s-wave phase
( 0.896m K ( 0.896m K
2 2 (GeV )q
V
V saw cos
asym for m(K K
t
Focus
erm :
* pol
Re co
e fro
(20 )
m
02
siAe BW
20 0 Re{ exp( }H h q A i BW BW
Re
Im
BW
A
For 40 the high mass BW is nearly to s-wave amp and interference nearly vanishes.
Our interference “Ho (q2) ho
(q2)” should also vanish above pole if 40 and it does!
Focus
CLEO-c
20
Search for D-wave K
2 2D F2 2
1 1No evidence for h ( ) or h ( ) q q
q q
20 ( )DH h q
*m K *m KGuard against “phase cancellation” by showing above and below the K*
Add a D-wave projector
q2 GeV2
21
(1) New result on BF D+ and fD
from CLEO-c 281/pb and preliminary fDs from BaBar
(2) Exclusive BF of semileptonic decays from CLEO-c.• With just 56 pb-1, many CLEO SL BF are already the world best.
Results on 281 pb-1 coming soon!.• Inclusive BF of D Xepreliminary from 281/pb. Consistent with
SL(D0)/ SL(D+) = 1. The sum of exclusive BF almost saturates
the inclusive BF
(3) Non-parametric form factor measurement from FOCUS
for D K l , in comparison with the latest unquenched light-
flavor LQCD results and preliminary BaBar results
Summary
22
Summary Continues…
(4) Preliminary non-parametric Form Factor measurements for D V l from CLEO-c 281/pb
a. H+, H-, H0 appear very consistent with expected K&S shapes.
b. Data fits constant A1(q2), A2 (q2), V (q2) as well as it fits spectroscopic pole dominance no sensitivity to q2 dependence
c. Statistically significant Ho (q2) ho (q2) interference term ho (q2) 1/q confirming s-wave interference effect.
d. The effective “Ho (q2) ho (q2) ” vanishes above the K* pole, suggesting an s-wave amplitude phase near 40 which is consistent with the Focus phase.
e. No evidence for a K non-resonant d-wave or f-wave contribution.
23
Question slides
24
More semileptonic signals
U ( = Emiss – |Pmiss| ) plots
(~1311 events) (~545 events)
The first 56pb-1
0 D K e
Ev
ents
/ 1
0 M
eV
0;D e
(~8 events) First Observ.
(~422 events)
0 0* *,D K e K K
0D K e
25
Vcd (1.1%) from 3 generation unitarity
D+ (0.3%) well-measured
fD from Absolute Br(D+ +)|fD|2
|VCKM|2
2222 2
21
8( ) / ( )F
cdD D DD
mGB D f m M V
M
• Based on 281 pb–1,158,354 tags and 50 signal events.• Background ~ three events.
0.09 40.12
2.83.4
5
4.40 0.66 10
222.6 16.7 MeV
2.4 10 @90%
D
B D
f
B D e CL
2+1 flavorPRL 95, 122002
26
Summary of CLEO-c (56 pb-1) Exclusive BF
Phys. Lett. B608, 24 (2005)
Phys. Lett. B 597, 39 (2004)
References: PRL 95 181801 and PRL 95 181802
(2005)
2 2 2
| | 0.957 0.017(exp) 0.093( )
| | 0.213 0.008(exp) 0.021( )
1 | | | | | | 0.037 0.181( )
cs
cd
cs cd cb
th
th
tot
Using the lastest LQCD (PRL 94, 011601),
V
V
V V V
27
Expected q2 Dependence of Helicity FF
Only 0 helicity components can survive at q2 0because of V-A helicity laws.
22 2
V
2 2 20 0 2
2Since A ( ) ( , )
c0 constant or H 0 , 0
q
d H q f
H q q h q
q l
2
c
q
28
q2 dependence: Deconvolution
2genq2
genq2genq
2genq 2
genq
2recq 2
recq2recq
2recq
2recq
1 2 2 2 3 21 1 1 2 1 3
1
2 21
122 2 2 3 2
2 1 2 2 2 3
1 2 2 2 3 23 1 3 2
22
33 3
2
2 23
1/ / /
/ / /
/ / /
G G GM M M
G G GM M M
G G GM M M
N f N f N f f qM
M f qN f N f N f
N f N f N f M f q
We actually use a 10 10 matrix
A deconvolution matrix is constructed from the number of events generated in thei-th q2 bin that end up reconstructed in the j-th q2 bin. This matrix is then used to correct data for resolution and efficiency.
29
Information on vector-axial pole masses
V
H--H
+
A1
H
++
H-
q2 q2
Difference and sum of non-parametric H+ and H- data
A1 and V are very consistent with spectroscopic pole forms and measured rV.
But the slopes are only a few sigma from 0, so no useful pole mass information can be obtained with present statistics.
30
M K
Preliminary CLEO D+ Ke FOCUS D+ K
Comparing CLEO-c & FOCUS Results
2 2q (GeV )
2 2+H (q ) 2 2H (q )-
2 20H (q )
20 0h H (q )´
Data 11397
2 2q (GeV )
Data 2472
M K
2 2+H (q )
2 20H (q ) 2
0 0h H (q )´
2 2H (q )-
2 2meas trueq -q
2 0.2 GeVs=
2 2meas trueq -q
20.02 GeVs=q2 res
q2 res
31
IV. c. Isospin Conjugation Test.0
0 0
( ( ) ) ( ( ) ),
( ) / ( ) 1.35 0.19 !D K e D K
D qd l D qu
e
l
We expect iso-spin conjugati
However, PDG04,
on
0
0 0( ) / ( ) 0.87
( )
0.11
D
D K D
K
K
From FOCUS (04) BR measurement,
From CLEO-c (56pb-1) measurements,
0
0
( )1.00 0.05 0.04
( )
D K e
D K e
0
0.140.110
( )0.75 0.04
2 ( )
D e
D e
0 *
*0
( )0.98 0.08 0.04
( )
D K e
D K e
ii
B