Upload
others
View
4
Download
0
Embed Size (px)
Citation preview
Results on charmonium(-like) states from Belle
V. ZhukovaBelle Collaboration
“Quarkonium Working Group”, Beijing, 6-10 November 2017
1 / 21
New measurement and angular analysis of thee+e− → D
(∗)+D
∗− process near the open charmthreshold with initial state radiation
2 / 21
Introduction and motivation
Spectrum of charmonium
Vector states above open-charmthreshold are not fully understood
Parameters of ψ states obtainedfrom σtot(e
+e− → hadrons)
are model-dependenthave large uncertainties
Data collected should allow forcoupled-channel analysis
3 / 21
Introduction and motivation
Spectrum of charmonium
Vector states above open-charmthreshold are not fully understood
Parameters of ψ states obtainedfrom σtot(e
+e− → hadrons)
are model-dependenthave large uncertainties
Data collected should allow forcoupled-channel analysis
Solution =⇒ Measure exclusive cross sections
3 / 21
Introduction and motivation
Comparison with previous results
Belle and BaBar resultsagree with each other
Statistics is too low tostudy the structure of thecross sections
Sum of all measuredexcusive cross-section toopen-charm channelssaturates the total crosssection
4 / 21
Introduction and motivation
Comparison with previous results
Belle and BaBar resultsagree with each other
Statistics is too low tostudy the structure of thecross sections
Sum of all measuredexcusive cross-section toopen-charm channelssaturates the total crosssection
Goals:
To improve accuracy of cross section measurements
To measure separately cross sections for all 3 possible helicity combinations(TT, LT, LL) for the D∗D̄∗ final state
4 / 21
Introduction and motivation
MethodPartial reconstruction
Reconstruct D∗, γISR
e+
e−
γISR
γ
D(∗)
D∗ πslow
D
Mrecoil(D(∗)γ) =
√
(Ec.m. −ED(∗)γ)
2 − p2
D(∗)γ
Mrec(D*+γisr) GeV/c2
Eve
nts/
0.1
GeV
/c2
0
1
2
3
×104
1 1.25 1.5 1.75 2 2.25 2.5 2.75 3
D+D∗−
ց
D∗+D∗−
ւ
5 / 21
Introduction and motivation
MethodPartial reconstruction
Reconstruct D∗, γISR
e+
e−
γISR
γ
D(∗)
D∗ πslow
D
Mrecoil(D(∗)γ) =
√
(Ec.m. −ED(∗)γ)
2 − p2
D(∗)γ
Mrec(D*+γisr) GeV/c2
Eve
nts/
0.1
GeV
/c2
0
1
2
3
×104
1 1.25 1.5 1.75 2 2.25 2.5 2.75 3
D+D∗−
ց
D∗+D∗−
ւ
Problem: Cannot distinguish between D, D∗ and D∗∗ in the final state
5 / 21
Introduction and motivation
MethodPartial reconstruction
Reconstruct D∗, γISR and πslow
e+
e−
γISR
γ
D(∗)
D∗ πslow
D
∆Mrecoil = Mrecoil(D(∗)γISR)−Mrecoil(D
(∗)πslowγ)
e+e− → D+D∗−
∆Mrec Gev/c2
N /0
.5 G
eV/c
2
01000200030004000500060007000
0.14 0.145 0.15 0.155 0.16
Recoil mass difference∆Mrecoil
ւ ց
cut:
±3MeV/c2
e+e− → D∗+D∗−
∆ Mrec Gev/c2
N /0
.5
M
eV/c
2
0
5000
10000
15000
20000
25000
0.14 0.145 0.15 0.155 0.16
6 / 21
Introduction and motivation
MethodPartial reconstruction
Reconstruct D∗, γISR and πslow
M(D(∗)+D∗−) ≡ Mrecoil(γISR)
e+
e−
γISR
γ
D(∗)
D∗ πslow
D
Mrecoil(γISR) =√
(E2c.m. − 2Ec.m. ·EγISR
)
Refit Mrecoil(D(∗)γISR) to D∗ mass to improve the Mrecoil(γISR) resolution
M(D*+ D*– ) resolution Gev/c2
Eve
nts/
5 M
eV/c
2
0
5000
10000
15000
-0.2 -0.1 0 0.1 0.2
Mrecoil(γISR) resolution:
Before re-fit — hatched histogramAfter re-fit — solid line
7 / 21
Analysis
Comparison with previous analysis
Increased data sample: 547 fb−1 =⇒ 951 fb−1
Additional modes for D reconstruction =⇒
Extended signal region for Mrecoil(D(∗)γISR)
|(Mrecoil(D(∗)+γISR)−M(D∗−))| <
300✟✟200 MeV/c2
σ[e+e− → D(∗)+D∗−] =dN/dM
ηtot(M) · dL/dM
dL/dM up to second-order QED corrections(Kuraev & Fadin (1985))
D0 decay channels:
1 K−π+
2 K−K+
3 K−π−π+π+
4 K0Sπ
+π−
5 K−π+π0
6 K0SK
+K−
7 K0Sπ
0
8 K−K+π−π+
9 K0Sπ
+π−π0
8 / 21
Analysis
Backgrounds
1 Combinatorial background under the reconstructed D(∗)+ peak
2 Real D(∗)+ mesons and a combinatorial πslow
3 Both the D(∗)+ meson and πslow are combinatorial
4 Reflections from the processes e+e− → D(∗)+D∗−π0γISR
where the π0 is lost
5 Contribution of the e+e− → D(∗)+D∗−π0fastwhere the hard π0fast is misidentified as γISR
Background contribution estimated from the data
9 / 21
Cross sections
√s GeV
σ (n
b)
0
1
2
3
4
4 4.5 5 5.5 6
0
2
4
4 4.2 4.4
√s GeV
σ (n
b)
0
1
2
3
4 4.5 5 5.5 6
0
1
2
3
4 4.2 4.4
D+D∗− D+D∗−
√s GeV
σ (n
b)
0
1
2
3
4
5
3.8 4 4.2 4.4 4.6 4.8 5√s GeV
σ (n
b)
01234567
4 4.2 4.4 4.6 4.8 5
PRL 98, 092001 (2007)
Belle 2007Belle 2017
PRL 98, 092001 (2007)
Belle 2007Belle 2017
10 / 21
Angular analysis
Angular analysis of the process e+e− → D
+D
∗−
Study D∗ helicity angle distributionin each bin of M(D+D∗−)
D∗ are transversely polarized=⇒ Check method
4.05 < M(D+D∗−) < 4.3GeV/c2
0
50
100
150
200
-1 -0.5 0 0.5 1
F (cos θ) = η(cos θ)·dM/dL·(fL + fT )
0
2
4 D+ D*-T
σ (n
b)
D+ D*-L
√s GeV
0
2
4
4 4.5 5 5.5 6
fL = σL · cos2 θfT = σT · (1− cos2 θ)
11 / 21
Angular analysis
Angular analysis of the process e+e− → D
∗+D
∗−
Study of the D∗ helicity angle distribution in each bin of M(D∗+D∗−)Helicity composition of the D∗+D∗− final state:
D∗+T D∗−
T , D∗+T D∗−
L and D∗+L D∗−
L
D∗
T ≡ transversely polarized D∗ mesonD∗
L ≡ longitudinally polarized D∗ meson
Total cross sectionσ = σTT + σTL + σLL
f = η(c1, c2)· dL/dM ·(fLL+fTL+fTT )+fbg
c1 ≡ cos θf c2 ≡ cos θp
θ’s are D∗’s helicity angles
fTT = σTT · (1− c21) · (1− c22)
fTL = σTL ·(
(1− c21) · c22 + c21 · (1− c22))
fLL = σLL · c21 · c22
cosθ fcosθ
p -1-0.5
00.5
1
-1-0.5
00.5
1050
100150
12 / 21
Angular analysis
Fit results
0
0.5
1
1.5
4 4.5 5 5.5 6√s GeV
σ (n
b) D*+T D*-
T
0
0.5
1
1.5
4 4.1 4.2 4.3 4.4 4.5
0
0.5
1
1.5
4 4.5 5 5.5 6√s GeV
σ (n
b) D*+T D*-
L
0
0.5
1
1.5
2
4 4.1 4.2 4.3 4.4 4.5
0
0.5
1
4 4.5 5 5.5 6√s GeV
σ (n
b)
D*+L D*-
L
0
0.5
1
4 4.1 4.2 4.3 4.4 4.5
13 / 21
Summary
Conclusions
We measured the exclusive cross sections of thee+e− → D+D∗− and e+e− → D∗+D∗− processes
The accuracy of the cross section measurements is increased
The systematic uncertainties are significantly reduced
For the e+e− → D∗+D∗− process we measured separatelythe cross sections for all three possible helicity final states(TT, LT and LL)
14 / 21
2
Observation of an alternative χc0(2P ) candidatein e
+e− → J/ψDD̄
15 / 21
Introduction
Motivation
X(3915)րց
Observed by Belle, confirmed by BaBar in B → (J/ψ ω)KPRL 94, 182002 (2005), PRD 82, 011101 (2010)
Observed by both Belle and BaBar in γγ → J/ψ ωPRL 104, 092001 (2010), PRD 86, 072002 (2012)
BaBar: JP = 0+ =⇒ χc0(2P ) candidate
PRD 86, 072002(2012)
Difficulties (see, e.g., S. L. Olsen (2015), F.-K.Guo et al. (2012)):Too narrow: 20 MeV (measured) versus ∼100 MeV (expected)
Not seen in DD̄ (expected as dominating mode!)
Unnaturally small 23P2-23P1 mass splitting
Strong OZI violation: large BF in OZI-suppressed J/ψ ω mode
16 / 21
Introduction
Motivation
X(3915)րց
Observed by Belle, confirmed by BaBar in B → (J/ψ ω)KPRL 94, 182002 (2005), PRD 82, 011101 (2010)
Observed by both Belle and BaBar in γγ → J/ψ ωPRL 104, 092001 (2010), PRD 86, 072002 (2012)
BaBar: JP = 0+ =⇒ χc0(2P ) candidate
PRD 86, 072002(2012)
Difficulties (see, e.g., S. L. Olsen (2015), F.-K.Guo et al. (2012)):Too narrow: 20 MeV (measured) versus ∼100 MeV (expected)
Not seen in DD̄ (expected as dominating mode!)
Unnaturally small 23P2-23P1 mass splitting
Strong OZI violation: large BF in OZI-suppressed J/ψ ω mode
Search for alternative χc0(2P ) candidate in e+e− → J/ψDD̄ annihilation
16 / 21
Analisys
Method
e+e− → J/ψDD̄, D ≡ D0 or D+
Mrec(J/ψ,D) =√
(pe+e− − p J/ψ − pD)2
J/ψ → {e+e−, µ+µ−}Both D0 and D+ used:
D0 → {K−π+,K0sπ
+π−,K−π+π0,K−π+π+π−} (4 channels)
D+ → {K0sπ
+,K−π+π+,K0sπ
+π0,K−π+π+π0,K0sπ
+π+π−}(5 channels)
Signal and background separated using the MLP neural network
Global optimization of the selection requirements: 4 variables per Dchannel (signal regions in M J/ψ, MD, Mrec(J/ψ,D) and MLP outputcutoff value)
Resulting sample: 103 events with 24.9 ± 1.1± 1.6 background events
17 / 21
Analisys
Signal fitAmplitude analysis in 6D phase space: {MDD̄, θprod, θ J/ψ, θX∗ , φl− , φD}
S(Φ) =∑
λbeam=−1,1λℓℓ=−1,1
∣
∣
∣
∑
X∗
Aλbeam λℓℓ(Φ)AX∗(MDD̄)∣
∣
∣
2
Resonance: AX∗ — relativistic BW,Non-resonant amplitude:AX∗ =
√
FDD̄(MDD̄),FDD̄(MDD̄) - non-resonant form factor,default model: FDD̄ = 1Model: X∗ + non-resonant contribution
JPC Mass, MeV/c2 Width, MeV Significance
0++ 3862+26−32
201+154−67
9.1σ
2++ 3879+20−17
171+129−62
8.0σ
2++ 3879+17−17
148+108−50
8.0σ
2++ 3883+26−24
227+201−125
8.0σ 2, GeV/cDD
M4 4.5 5 5.5 6
2E
vent
s / 5
0 M
eV/c
0
2
4
6
8
10
12
14
16
18
X∗ + NR + bg
NR amplitude and
background
18 / 21
Analisys
JPC = 0++ versus JPC = 2++
Approach: Toy MC pseudoexperiments generated in accordance with fitresults for JPC = 0++ and 2++ and fitted for both hypotheses
(-2 ln L)∆40− 20− 0 20 40
Pse
udoe
xper
imen
ts
0
10
20
30
40
50
60
70
80Value in data
++0++2
Result:
JPC = 2++ excluded at the level 2.5σ including systematics
JPC = 0++ with CL=77% (default model)
19 / 21
Analisys
X∗(3860) versus X(3915) — the fight for χc0(2P )
Theory X(3915) X∗(3860)
JPC 0++ ± +
Mass3854 MeV/c2 (Ebert et al.)
± +3916 MeV/c2 (Godfrey et al.)
Width Broad (Γ ∼ 100 MeV) − +
mχc2(2P )−mχc0(2P )
mχc2(1P )−mχc0(1P )0.6..0.9 − +
BF(DD̄) Large − +
BF(J/ψ ω) Small − +
In addition, X∗(3860)
is produced similarly to χc0(1P ) (Belle (2004))
agrees with the peak in γγ data with M = 3837.6 ± 11.5 MeV/c2 andΓ = 221± 19 MeV
20 / 21
Analisys
X∗(3860) versus X(3915) — the fight for χc0(2P )
Theory X(3915) X∗(3860)
JPC 0++ ± +
Mass3854 MeV/c2 (Ebert et al.)
± +3916 MeV/c2 (Godfrey et al.)
Width Broad (Γ ∼ 100 MeV) − +
mχc2(2P )−mχc0(2P )
mχc2(1P )−mχc0(1P )0.6..0.9 − +
BF(DD̄) Large − +
BF(J/ψ ω) Small − +
In addition, X∗(3860)
is produced similarly to χc0(1P ) (Belle (2004))
agrees with the peak in γγ data with M = 3837.6 ± 11.5 MeV/c2 andΓ = 221± 19 MeV
Conclusion:X∗(3860) wins!
20 / 21
Summary
Conclusions
A new charmoniumlike state X(3860) is observed
M = 3862+26 +40−32 −13 MeV/c2
Γ = 201+154 +88−67 −82 MeV
JPC = 0++ favoured
X(3860) =⇒ good χc0(2P ) candidate
21 / 21
Summary
Conclusions
A new charmoniumlike state X(3860) is observed
M = 3862+26 +40−32 −13 MeV/c2
Γ = 201+154 +88−67 −82 MeV
JPC = 0++ favoured
X(3860) =⇒ good χc0(2P ) candidate
Thank you for your attention!
21 / 21
Event selection
Criteria|dr|< 2 cm and |dz|< 4 cm
PK/π = LK/(LK + Lπ) > 0.6
KS candidates:
|Minv(π+π−)−MK0
S
| < 15 MeV/c2
the distance between the two piontracks < 1 cm
the transverse flight distance from IP> 0.1 cm
the angle between the KS momentumdirection and decay path in x− yplane < 0.1 rad
π0 candidates:
|Minv(γγ)−Mπ0| < 15 MeV/c2
D0 decaychannels:
1 K−π+
2 K−K+
3 K−π−π+π+
4 K0Sπ
+π−
5 K−π+π0
6 K0SK
+K−
7 K0Sπ
0
8 K−K+π−π+
9 K0Sπ
+π−π0
D+ decaychannels:
1 K+π−π−
2 K0Sπ
−
3 K0SK
+
D∗ decaychannels:
1 D0π+
1 / 14
Calibration of γISR energy
Analysis of the process e+e− → D
(∗)+D
∗−
Method:
partial reconstruction;
reconstruction D∗, πslow and
γISR;
e+
e−
γISR
γ
D(∗)
D∗ πslow
DMrecoil(D(∗)γ) =
√
(Ec.m. − ED(∗)γ)2 − p2
D(∗)γ
∆Mrecoil =Mrecoil(D(∗)γISR)−Mrecoil(D
(∗)πslowγ)
Mrec(D* γ) Gev/c2
N /0
.05
GeV
/c2
0
200
400
600
800
1000
1 1.2 1.4 1.6 1.8 2 2.2 2.4 2.6 2.8 3
Spectrum of Mrecoil(D∗γISR)
Mrecoil(D(∗)γ) =
√
(Ec.m. −ED(∗)γ)2 − p2
D(∗)γ
2 / 14
Calibration of γISR energy
Correction of γISR energyreference channel
e+e− → ψ(2S)γISR
ցψ(2S) → J/ψπ+π−
Conclusions:
phokhara generator describes thesecond radiation correction correctly
The same process on the other
side
The recoil mass Mrecoil(J/ψπ+π−)
0
100
200
300
400
500
2 2.5 3 3.5 4 4.5 5
0
100
200
300
400
500
2 2.5 3 3.5 4 4.5 5
3 / 14
Analysis
The recoil mass Mrecoil(D∗γISR)
before correction γISR energy
Mrec(D* γ) Gev/c2
N /0
.05
GeV
/c2
0
200
400
600
800
1000
1 1.2 1.4 1.6 1.8 2 2.2 2.4 2.6 2.8 3
after correction γISR energy
Mrec(D* γ) Gev/c2
N /0
.05
GeV
/c2
0
200
400
600
800
1000
1 1.2 1.4 1.6 1.8 2 2.2 2.4 2.6 2.8 3
cut:
|Mrecoil(D∗γISR)−M(D∗)| < 300MeV/c2
4 / 14
Analysis
Backgrounds1 Combinatorial background under the reconstructed D(∗)+ peak2 Real D(∗)+ mesons and a combinatorial πslow
3 Both the D(∗)+ meson and πslow are combinatorial4 Reflections from the processes e+e− → D(∗)+D∗−π0γISR
where the π0 is lost5 Contribution of the e+e− → D(∗)+D∗−π0fast
where the hard π0fast is misidentified as γISR
e+e− → D+D∗−
∆Mfitrec GeV/c2
M(D
)
G
eV/c
2
A
B
B
C
C
D
1.82
1.84
1.86
1.88
1.9
1.92
0.14 0.15 0.16
e+e− → D∗+D∗−
∆Mfitrec Gev/c2
M(D
* )
G
eV/c
2
A
B2
B1
C1 C2
D
2.01
2.02
2.03
0.14 0.15 0.165 / 14
Analysis
Mass spectra
M(D+D*– ) GeV/c2
Eve
nts/
20 M
eV/c
2
951 fb-1
0
100
200
300
400
4 4.5 5 5.5 6 M(D*+D*– ) GeV/c2
Eve
nts/
20 M
eV/c
2
951 fb-1
0
100
200
300
400
4 4.5 5 5.5 6
e+e− → D+D∗− e+e− → D∗+D∗−
PRL 98, 092001(2007)
547 fb−1
PRL 98, 092001(2007)
547 fb−1
6 / 14
Analysis
Reflection from the processes e+e− → D
(∗)+D
∗−π0γISR
e+e− → D+D∗− e+e− → D∗+D∗−
M(D+ D*– ) GeV/c2
Eve
nts/
20 M
eV/c
2
0
100
200
300
4 4.5 5 5.5 6M(D*+ D*– ) GeV/c2
Eve
nts/
20 M
eV/c
2
0
100
200
300
4 4.5 5 5.5 6
Background (blue points) from
e+e− → D(∗)+D∗−π0missγISR
is evaluated from the isospin-conjugated process
e+e− → D(∗)0D∗−π+missγISR
with the reconstruction of D(∗)0, π−slow and γISR7 / 14
Analysis
Backgrounds
e+e− → D∗+D∗−
a)
M(D*) GeV/c2
Eve
nts
/0.2
M
eV/c
2
0
200
400
2.01 2.02 2.03
∆Mrec GeV/c2
Eve
nts
/0.2
MeV
/c2
b)
0
200
400
600
0.14 0.15 0.16 0.17
x ≡ M(D∗) x ≡ ∆Mrec
f = fsignal + fbackground
fbackground = α ·√x · (1 + β · x+ γ · x2)
Mbg (1)-(3) = 0.58 ·Msb B + 0.53 ·Msb C − 0.307 ·Msb D
8 / 14
Analysis
Backgrounds
e+e− → D+D∗−
a)
M(D+) GeV/c2
Eve
nts
/2.0
MeV
/c2
0
500
1000
1.8 1.85 1.9 1.95
b)
∆Mfitrec GeV/c2
Eve
nts
/0.0
5 M
eV/c
2
0
500
1000
1500
0.14 0.15 0.16
x ≡ M(D+) x ≡ ∆Mrec
f = fsignal + fbackground
fbackground = α ·√x · (1 + β · x+ γ · x2)
Mbg (1)-(3) = 0.5 ·Msb B + 0.5 ·Msb C − 0.25 ·Msb D
9 / 14
Analysis
Cross sections calculation
e+e− → D+D∗−
M(D+ D*-) Gev/c2
N /2
0
MeV
/c2
0
0.0025
0.005
0.0075
0.01
4 4.2 4.4 4.6 4.8 5
total efficiency
e+e− → D∗+D∗−
M(D*+ D*-) Gev/c2
N /2
0
MeV
/c2
0
0.002
0.004
0.0060.008
0.01
4 4.25 4.5 4.75 5
total efficiency
σe+e−→D(∗)+D∗− = dN/dM
ηtot(M)·dL/dM
dN/dM - mass spectrum,
ηtot - total efficiency,
dL/dM - differential luminosity;
10 / 14
Analysis
4.0 < M(D∗+D∗−) < 4.1GeV/c2
cosθ fcosθ
p
a)
-1-0.5
00.5
1
-1-0.5
00.5
10255075
4.25 < M(D∗+D∗−) < 4.6GeV/c2
cosθ fcosθ
p
c)
-1-0.5
00.5
1
-1-0.5
00.5
1050
100
4.1 < M(D∗+D∗−) < 4.25GeV/c2
cosθ fcosθ
p -1-0.5
00.5
1
-1-0.5
00.5
1050
100150
M(D∗+D∗−) > 4.6GeV/c2
cosθ fcosθ
p
d)
-1-0.5
00.5
1
-1-0.5
00.5
1050
100150
11 / 14
Analysis
The summary of the systematic errors in the cross section calculation.
Source D+D∗− D∗+D∗−
Background subtraction 2% 2%Reconstruction 3% 4%Selection 1% 1%Angular distribution − 2%Cross section calculation 1.5% 1.5%
B(D(∗)) 2% 3%MC statistics 1% 2%
Total 5% 7%
12 / 14
Analysis
Signal fit
S(Φ) =∑
λbeam=−1,1λℓℓ=−1,1
∣
∣
∣
∑
X∗
Aλbeam λℓℓ(Φ)AX∗(MDD̄)
∣
∣
∣
2
, (1)
Here, Aλbeam λℓℓ(Φ) is the signal amplitude calculated using the helicity formalizm
(the phase space Φ is 6-dimensional). For resonance, AX∗ = relativisticBreit-Wigner. For nonresonant amplitude, AX∗ =
√
FDD̄(MDD̄), whereFDD̄(MDD̄) is the nonresonant amplitude form factor (FDD̄ = 1 by default).Alternatives: mass dependence of NRQCD prediction for e+e− → ψχc [PRD 77,014002 (2008)], FDD̄ =M−4
DD̄[Victor Chernyak, based on PLB 612, 215 (2005)].
4 4.5 5 5.5 6 6.5 72, GeV/c
DDm
0
0.2
0.4
0.6
0.8
1
1.2
ConstantNRQCD
-4DD
M
13 / 14
Analysis
Signal fit resultsFit results in the default model. For the 2++ hypothesis, there are three solutions(fit is started 1000 times from random initial values in order to check for that).
JPC Mass, MeV/c2 Width, MeV Significance
0++ 3862+26−32 201+154
−67 9.1σ2++ 3879+20
−17 171+129−62 8.0σ
2++ 3879+17−17 148+108
−50 8.0σ2++ 3883+26
−24 227+201−125 8.0σ
Red dashed line - only background and nonresonant amplitudes, blue solid line -X∗, JPC = 0++.
2, GeV/cDD
M4 4.5 5 5.5 6
2E
vent
s / 5
0 M
eV/c
0
2
4
6
8
10
12
14
16
18
14 / 14