October 2006GHP 20061 The GlueX Experiment Curtis A. Meyer CH L-2.
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Transcript of October 2006GHP 20061 The GlueX Experiment Curtis A. Meyer CH L-2.
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October 2006 GHP 2006 1
The GlueX ExperimentThe GlueX Experiment
Curtis A. Meyer
CHCHL-2L-2
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October 2006 GHP 2006 2
CHL-2CHL-2
Upgrade Upgrade magnets and magnets and
power power suppliessupplies
JLab UpgradeJLab Upgrade
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October 2006 GHP 2006 3
What’s New: The CEBAF Upgrade will take advantage of recent advancesin computing power, combined with a doubling of the existing energy of theelectron beam, to create a 12 giga-volt electron beam capable of providingmuch more precise data on the structure of protons and neutrons. Specifically,the upgrade will enable scientists to address one of the great mysteries ofmodern physics – the mechanism that “confines” quarks together. Newsupercomputing studies indicate that force fields called “flux-tubes” may beresponsible, and that exciting these should lead to the creation of neverbefore-seen particles.
November 2003
12 GeV Upgrade CD-0 Signing at Jefferson LabApril 19, 2004
Deputy Energy SecretaryKyle McSlarrow
February 2006: Project Receives CD-1
Secretary of Energy Announces Approval and Funding for Facilities Upgrade at the Thomas Jefferson National Lab and Highlights Lab’s Successful Education Programs
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October 2006 GHP 2006 4
The GlueX Collaboration
The search for gluonic excitations
Approximately 70 Collaborators
Members from seven countries
Active collaboration since 1998
New Members are very welcome
http://www.gluex.org/
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October 2006 GHP 2006 5
1.0
1.5
2.0
2.5
qq Mesons
L = 0 1 2 3 4
Each box correspondsto 4 nonets (2 for L=0)
Radial excitations
(L = qq angular momentum)
exoticnonets
0 – +
0 + –
1 + +
1 + –
1– +
1 – –
2 – +
2 + –2 + +
0 – +
2 – +
0 + +
Glueballs
Hybrids
Lattice 1-+ 1.9 GeV
Spectrum
0++ 1.6 GeV
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October 2006 GHP 2006 6
Flux TubesFlux Tubes
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October 2006 GHP 2006 7
m=0 CP=(-1) S+1
m=1 CP=(-1) S
Flux-tube Model
ground-state flux-tube m=0
excited flux-tube m=1
built on quark-model mesons
CP={(-1)L+S}{(-1)L+1} ={(-1)S+1}
S=0,L=0,m=1
J=1 CP=+
JPC=1++,1--
(not exotic)
S=1,L=0,m=1
J=1 CP=-JPC=0-+,0+-
1-+,1+-
2-+,2+-exotic
normal mesons
1-+ or 1+-
Hybrid MesonsHybrid Mesons
,
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October 2006 GHP 2006 8
Hybrid PredictionsHybrid PredictionsFlux-tube model: 8 degenerate nonets 1++,1-- 0-+,0+-,1-+,1+-,2-+,2+- ~1.9 GeV/c2
Lattice calculations --- 1-+ nonet is the lightest UKQCD (97) 1.87 0.20MILC (97) 1.97 0.30MILC (99) 2.11 0.10Lacock(99) 1.90 0.20Mei(02) 2.01 0.10Bernard(04) 1.792§0.139In the charmonium sector:1-+ 4.39 0.080+- 4.61 0.11
Splitting = 0.20
1-+ 1.9§ 0.22+- 2.0§ 0.110+- 2.3§ 0.6
S=0 S=1
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October 2006 GHP 2006 9
E852 (BNL): Exotic reported at a mass of 1.6 GeV
A new analysis with 10 times the statistics in two final states.What are the waves that are needed? E852E852
JPC = 1-+
-p! n +--
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October 2006 GHP 2006 10
Exotic Exotic SignalsSignals
1(1400) Width ~ 0.3 GeV, Decays: only weak signal in p production (scattering??) strong signal in antiproton-deuterium.
1(1600) Width ~ 0.16 GeV, Decays ,’,(b1) Only seen in p production, (E852 + VES)
1 IG(JPC)=1-(1-+)
’1 IG(JPC)=0+(1-+)
1 IG(JPC)=0+(1-+)
K1 IG(JPC)= ½ (1-)
1(2000) Weak evidence in preferred hybrid modes f1 and b1
NOT AHYBRID
What is reallyhere?
The rightplace. Needsconfirmation.
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October 2006 GHP 2006 11
PhotoproductioPhotoproductionn
More likely to find exotic hybrid mesons using beams of photons
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October 2006 GHP 2006 12
The angular momentum in the flux tube stays in one of the daughter mesons (L=1) and (L=0) meson.
1 b1 , f1 , , a1 1:.25:.25:.201(1300) , a1
b2 a1 , h1, a2h2 b1 ,
b0 (1300) , h1h0 b1 , h1
Lflux
Lflux
Exotic Quantum Number Hybrids
Mass and modeldependent predictions
Hybrid DecaysHybrid Decays
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October 2006 GHP 2006 13
ExoticsExotics
N N
e
X
,,
1 IG(JPC)=1-(1-+)
’1 IG(JPC)=0+(1-+)
1 IG(JPC)=0+(1-+)
K1 IG(JPC)= ½ (1-)
1-+ nonet
in Photoproductionin Photoproduction
Need to establish nonet nature of exotics: 0
Need to establish more than onenonet: 0+- 1-+ 2+-
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October 2006 GHP 2006 14
00+-+- and 2 and 2+-+- Exotics Exotics
N N
e
X
b0 IG(JPC)=1+(0+-)
h0 IG(JPC)=0-(0+-)
h’0 IG(JPC)=0-(0+-)
K0 I(JP)=½(0+)
b2 IG(JPC)=1+(2+-)
h2 IG(JPC)=0-(2+-)
h’2 IG(JPC)=0-(2+-)
K2 I(JP)= ½(2+)
a1,f0,f1
f0,f1,a1
f0,f1,a1
, a1,f0,f1
f0,f1,a1
f0,f1,a1
In photoproduction, couple to , or ?
“Similar to 1 ”
Kaons do not have exotic QN’s
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October 2006 GHP 2006 15
In order to establish the existence of gluonic excitations,We need to establish the nonet nature of the 1-+ state.
We need to establish other exotic QN nonets – the 0+- and 2+-.
In the scalar glueball sector,the decay patterns have provided the most sensitiveinformation. I expect the same will be true in the hybrid sector as well.
DECAY PATTERNS ARE CRUCIAL
Exotics and QCDExotics and QCD
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October 2006 GHP 2006 16
The GlueX The GlueX ExperimentExperiment
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October 2006 GHP 2006 17
Optimized for PWAOptimized for PWA
Nearly 4 acceptance for neutral and charged particles.
Linearly polarized photons with energy optimized for hybrid searches.
Uniform acceptance in the variables appropriate for Partial Wave Analysis.
PWA Leakage studies have been performed using Monte Carlo.
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October 2006 GHP 2006 18
-1 -0.8 -0.6 -0.4 -0.2 -0 0.2 0.4 0.6 0.8 10
0.2
0.4
0.6
0.8
1
Cos( GJ)
5 GeV
Mass(X) = 1.4 GeV
Mass(X) = 1.7 GeV
Mass(X) = 2.0 GeV
-3 -2 -1 0 1 2 30
0.2
0.4
0.6
0.8
1
GJ
-1 -0.8 -0.6 -0.4 -0.2 -0 0.2 0.4 0.6 0.8 10
0.2
0.4
0.6
0.8
1
Cos( GJ)
8 GeV
Mass(X) = 1.4 GeV
Mass(X) = 1.7 GeV
Mass(X) = 2.0 GeV
-3 -2 -1 0 1 2 30
0.2
0.4
0.6
0.8
1
GJ
-1 -0.8 -0.6 -0.4 -0.2 -0 0.2 0.4 0.6 0.8 10
0.2
0.4
0.6
0.8
1
Cos( GJ)
12 GeV
Mass(X) = 1.4 GeV
Mass(X) = 1.7 GeV
Mass(X) = 2.0 GeV
-3 -2 -1 0 1 2 30
0.2
0.4
0.6
0.8
1
GJ
p -> n
-1 -0.8 -0.6 -0.4 -0.2 -0 0.2 0.4 0.6 0.8 10
0.2
0.4
0.6
0.8
1
Cos( GJ)
5 GeV
Mass(X) = 1.4 GeV
Mass(X) = 1.7 GeV
Mass(X) = 2.0 GeV
-3 -2 -1 0 1 2 30
0.2
0.4
0.6
0.8
1
GJ
-1 -0.8 -0.6 -0.4 -0.2 -0 0.2 0.4 0.6 0.8 10
0.2
0.4
0.6
0.8
1
Cos( GJ)
8 GeV
Mass(X) = 1.4 GeV
Mass(X) = 1.7 GeV
Mass(X) = 2.0 GeV
-3 -2 -1 0 1 2 30
0.2
0.4
0.6
0.8
1
GJ
-1 -0.8 -0.6 -0.4 -0.2 -0 0.2 0.4 0.6 0.8 10
0.2
0.4
0.6
0.8
1
Cos( GJ)
12 GeV
Mass(X) = 1.4 GeV
Mass(X) = 1.7 GeV
Mass(X) = 2.0 GeV
-3 -2 -1 0 1 2 30
0.2
0.4
0.6
0.8
1
GJ
p -> p
p Xn 00n
Gottfried-Jackson frame:
In the rest frame of Xthe decay angles aretheta, phi
Mass [X] = 1.4 GeV
Mass [X] = 1.7 GeV
Mass [X] = 2.0 GeV
AcceptanceAcceptance
p!++-n
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October 2006 GHP 2006 19
Partial Wave Analysis
p ! 1+n! ++-n
! +00n
p
n
X
m [GeV/c2]
GJ
a2
Double blind studies of 3 final states
Polarization
GlueX Monte Carlo
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October 2006 GHP 2006 20
neutral
charged
Leakage
If your acceptance is not well understood, The PWA can “leak” one wave into another.
Break the GlueX detector in Monte Carlo: distort B-field degrade resolution change hole sizes distort beam energy
Largest leakage is ~ 1/2% of a strong signal. a1(1++) $ 1(1-+)
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October 2006 GHP 2006 21
Partial Wave Analysis
Have been able to pull out signals that are ~1% ofa strong signal using PWA.
It is extremely difficult to produce leakage that isas large as 1%.
Assuming a good theoretical understanding, if hybrids are present at ~1% of normal mesons strength, this detector will be able to find them.
Studies are currently being redone with detectorsoftware.
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October 2006 GHP 2006 22
Solenoid RefurbishmentSolenoid Refurbishment
LASS Solenoid
Superconducting 2.5T
Used in Los AlamosMEGA Experiment.
Moved to IUCF forrefurbishing, whichis nearly done.
Single coil test planned
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October 2006 GHP 2006 23
Detector R&D Detector R&D WorkWork
Drift Chambers
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October 2006 GHP 2006 24
CalorimetersCalorimeters
Barrel Calorimeter Pb-SciFib
Existing Pb-Glass for Forward
Backwards Veto
Beam tests just finished
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October 2006 GHP 2006 25
ElectronicsElectronics
The F1TDC
Flash ADC System
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October 2006 GHP 2006 26
DetectorDetector ReviewsReviews
July 2003: Held a 2-day review of GlueX Electronics
October 2004: Held a 2-day review of the GlueX Detector.
November 2004: Solenoid Assessment
January 2006: Tagger Review
Spring 2007: Drift Chamber Review
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October 2006 GHP 2006 27
Analysis Analysis PreparationPreparation
From the very start, the GlueX Collaboration has had an active theorygroup. It is well recognized that theorists need to be closely integratedinto the analysis from the start.
The scale of data from GlueX will be comparable to LHC experiments.However, the needs are different – GRID technologies will be crucial.Also, the tools to parallelize the analysis of 100,000,000 event datasets are being developed.
The theoretical underpinnings of Partial Wave Analysis need toBe looked at closely now that large data sets are becoming available.What exactly are the model assumptions and how do they affectThe results.
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October 2006 GHP 2006 28
SummarySummary The GlueX Collaboration is moving forward!
The DOE 20-year plan and CD0 have opened the door to a great deal of interest by new groups in GlueX.
The Collaboration is pressing forward with detector R&D coupled with external reviews of what we are doing. The Collaboration is working hard to make sure that analysis issues due to the large data sets are in hand.
We are paying close attention to the theoretical underpinnings of PWA to make sure that what comes out of GlueX is a clear answer.
New collaborators are welcome! http://www.gluex.org