Λ *(1520) photoproduction from lh 2 and ld 2
DESCRIPTION
Λ *(1520) Photoproduction from LH 2 and LD 2. Jia-Ye Chen. Outline. Physics Motivation Previous Results : LAMP2 and CLAS Data Analysis Reaction Channels Analysis Scenarios Event Selections Λ *(1520) production in Kp and KK detection modes Background Linearity - PowerPoint PPT PresentationTRANSCRIPT
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2008.5.1 LEPS Collaboration Meeting In Taiwan
Λ*(1520) Photoproductionfrom LH2 and LD2
Jia-Ye Chen
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Outline
Physics Motivation Previous Results : LAMP2 and CLAS Data Analysis
Reaction Channels Analysis Scenarios Event Selections Λ*(1520) production in Kp and KK detection modes Background Linearity K- decay asymmetry in Λ*(1520) Helicity frame
• Side-Band Subtraction• Monte Carlo Background Fitting (By Muramatsu-san)
Total Cross Section of LH2 and LD2
Summary
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)( 23 PJ
)( 21 PJ
)1( PJ)0( PJ
)1(* PJK
)0( PJK
Physics Motivation
K2sin
K
2cos3
1
Helicity Frame
γγ + + p → Kp → K++ + + Λ*(1520) Λ*(1520) →→ KK++ + + pp + + KK--
exchangeK
mz
21
exchangeK
mz
*
23
1. If ONLY spinless kaon, K-, exchange → 021
23
z
z
m
m
1
3
21
23
z
z
m
m2. If ONLY vector kaon, K*- ,exchange → (If solely determined by Clebsch-Gordon coefficients)
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Previous Results
KKKf 22 sincos
3
1)(
1
1
1cos)( dfKAssume
75.0
CLASElectroproduction
LAMP2Photoproduction
Contribution
Q2≠0
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Reaction Channels
pKKKpd *)(
Background Channels
KpKnd *
pKKKp *
pKKpp pKKp
Production Channels
NKKNN
LH2
LD2
LH2
LD2 KpKnd *0)(
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Analysis ScenariosSide-Band Subtraction Monte Carlo Background Fitting
Assuming that the background linearity is good, , the count in S0 region can be obtained accompany with the sneak-in factor from Monte Carlo simulation.
0)( 2121
0 BBB
2121
02121
0
212121
00 )()(
BBBSSS
BBSSBS
Subtracting the background components from real data mass spectrum to get the count of Λ*(1520).
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Event Selections
Kp mode ntrk > 1 3 sigma PID ikm/ipr ≠ 0 ithtofhit(ikm/ipr) > 0 prbchi2(ikm/ipr) ≥ 0.02 abs(ytof(ikm/ipr)-tofdiff(ikm/ipr)) ≤ 80 abs(itof(ikm/ipr)-tofid(ikm/ipr)) < 2 noutl(ikm/ipr) ≤ 6 -1100 ≤ vtz ≤ -900 abs(vtx) ≤ 15 0.40 ≤ missing mass of pK- ≤ 0.62 GeV photon energy ≥ 1.75 GeV abs(missing mass of proton – 1.020) > 15
MeV
KK mode ntrk > 1 4 sigma PID ikm/ikp ≠ 0 ithtofhit(ikm/ikp) > 0 prbchi2(ikm/ikp) ≥ 0.02 abs(ytof(ikm/ikp)-tofdiff(ikm/ikp)) ≤ 80 abs(itof(ikm/ikp)-tofid(ikm/ikp)) < 2 noutl(ikm/ikp) ≤ 6 -1100 ≤ vtz ≤ -900 abs(vtx) ≤ 25 abs(missing mass of proton – Mp) < 0.050
GeV photon energy ≥ 2.00 GeV abs(invm(KpKm) – 1.020) > 10 MeV
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KP Mode : LH2
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KP Mode : LD2
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Background Estimation How-to
1. Generating known reaction components individually.
2. To select 2 detected particles (K-p or K+K-) reconstructed at the forward spectrometer.
3. Skimming each component with kinematics filters.
4. Fitting all components with real data spectrum in various dependence simultaneously to obtain the scaling parameters.
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Monte Carlo Fitting : LH2 (Kp Mode)
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Monte Carlo Fitting : LD2 (Kp Mode)
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KP Mode : LH2
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KP Mode : LD2
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KK Mode : LH2
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Monte Carlo Fitting : LH2 (KK)
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KK Mode : LH2
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Background Linearity How-to
0
210
)2,1,0()2,1,0()2,1,0(
)2,1,0()2,1,0()2,1,0(
0
210
))()(()(
)(
22212
22
21
B
BBB
L
KKpBBB
KKpBBB
B
BBB
N
ErrorErrorErrorError
RNRNError
RNRNN
N
NNNLLinearity
KKp
KKp
Global Fitting Factors
KKp = 0.0282
KL* = 0.0171
phi = 0.0361
Global Fitting Factors
KKp = 0.0282
KL* = 0.0171
phi = 0.0361
Relative Ratios
RKKp = 1.
RL* = 0.60638
Rphi = 1.28014
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Linearity by Photon Energy
Kp
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K? exchange5 Energy Slices
LH2(Kp vs KK)
Contribution
1. Both in the Kp(LH2 & LD2) and KK(LH2) detection mode, the results between side-band subtraction and Monte Carlo fitting are consistent.
2. In the Kp detection mode, there is an energy dependence on the K* exchange in LH2
case; however, no obvious energy dependence in LD2 case.
3. The results between from Kp and KK detection mode are compatible in higher photon energy region, even if the statistics is lower in KK detection mode.
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5 SlicesLH2
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5 SlicesLD2
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5 SlicesLH2(KK)
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Comparison betweenLAMP2, CLAS and LEPS
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Total Cross Section
*0 Kn* Kp
S.-II Nam, A. Hosaka and H.-C. Kim, Phys. Rev. D 71, 114012.
The contact term is absent, since the process γ+n→K0Λ* is the neutral one. Its absence cause the total cross section to become much smaller than that for the proton target.
PRELIMINARY
PRELIMINARY
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Eγ NYieldAcceptanc
eNγ
1.75-1.85
57 0.01202.421E+
11
1.85-1.95
83 0.01152.7095E
+11
1.95-2.05
99 0.01173.0042E
+11
2.05-2.10
47 0.01241.6071E
+11
2.10-2.15
44 0.01271.6187E
+11
2.15-2.20
47 0.01301.8283E
+11
2.20-2.25
40 0.01371.876E+
11
2.25-2.30
47 0.01401.862E+
11
2.30-2.35
46 0.01471.8304E
+11
2.35-2.40
11 0.01581.9476E
+11
Eγ NYieldAcceptanc
eNγ
1.75-1.85
121 0.01043.5112E
+11
1.85-1.95
182 0.01144.1133E
+11
1.95-2.05
209 0.01194.9196E
+11
2.05-2.10
97 0.01222.5873E
+11
2.10-2.15
116 0.01212.6265E
+11
2.15-2.20
103 0.01292.959E+
11
2.20-2.25
93 0.01303.0304E
+11
2.25-2.30
110 0.01342.9449E
+11
2.30-2.35
82 0.01382.9198E
+11
2.35-2.40
78 0.01483.0008E
+11
bcm
cmg
ett cmNLH
17123
23
arg2
1076574.61076574.6
00794.1
1002.60708.016:
2
3
LH2 LD2
bcm
cmg
ett cmNLD
17123
23
arg2
1013904.81013904.8
01355.2
1002.6169.016:
2
3
225.0
762.0
52.0
*
1
pK
ntag
trans
BR
P
P
BRPPNNAccNb ntagtransettphotonYield 1arg/Nγ : /np1b/v01/sp8lep/OfficialMacro/runinfo/Photo_llh(d)2.dat by Sumihama-san
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Summary In the study of K- decay asymmetry in Λ* helicity frame, if the background linearit
y is reasonable, the consistency between side-band subtraction and Monte Carlo fitting is good.
Without phi exclusion cut, it is very difficult to study in the KK detection mode; in the Kp detection mode, however, there is no significant difference between the results with and without phi exclusion cut in decay asymmetry study. The results between from Kp and KK detection mode are compatible in higher photon energy region, even if the statistics is lower in KK detection mode.
To make a comparison between different targets, LH2 and LD2, in Kp detection mode, no obvious photon energy dependence was observed in LD2 data. This difference might come from the Λ* photoproduction of neutron.
In Λ* photoproduction, the dominance of K* exchange is proportional to photon energy; in the low energy region, K exchange become important and the contribution from K and K* exchange are equivalent. From our result, it provides a nice bridge between LAMP2 and CLAS experiment, in the high energy, K* exchange significantly dominate the Λ* photoproduction. (Clebsch-Gordon coefficients)
Refer to “Phys. Rev. D 71, 114012“, the absence of the contact term in neutron process leads to the total cross section to become much smaller than that for the proton target. Therefore, from our result, the total cross section of neutron is small, but, not as small as the theoretical prediction, 1/30. On the other hand, our result are not consistent with the theoretical prediction, it is about a factor of 2.
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2008.5.1 LEPS Collaboration Meeting In Taiwan
Backup Slices
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Photon Energy SpectrumLH2(Kp) LH2(KK)
LD2(Kp) LD2(KK)
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KK Mode : LD2
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KK Mode : LD2
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KK Mode (W/O Phi exclusion Cut)
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KK Mode (W/O Phi exclusion Cut)
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KK Mode (W/O Phi exclusion Cut)
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Full Photon Energy
LH2(Kp vs KK)
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2 Energy Slices
LH2(Kp vs KK)
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3 Energy Slices
LH2(Kp vs KK)
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4 Energy Slices
LH2(Kp vs KK)
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Full Photon Energy
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2 Slices : LH2(Kp)
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2 Slices : LD2(Kp)
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2 Slices : LH2(KK)
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3 Slices : LH2(Kp)
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3 Slices : LD2(Kp)
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3 Slices : LH2(KK)
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4 Slices : LH2(Kp)
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4 Slices : LD2(Kp)
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4 Slices : LH2(KK)