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Flux
tube
forms
between
The Jefferson Lab Hall D Project
Curtis A. Meyer
Carnegie Mellon University
SLAC Seminar, 10 January, 2002
The Search for QCD Exotics and
q
qbe
fore
q
q
befo
re
q
q
befo
re
q
q
befo
reOutline
Meson spectroscopy and gluonic excitations
Experimental Evidence
The Hall D Project
History and Timelines
Summary
Light Quark Meson Spectroscopy
q
q
J = L + S
P = (1)L
C = (1) (L+S)
Nonets
uds
Orb
ital
exc
itat
ion
s
Radial excitations
QCD is a theory of quarks and gluons
What role do gluons play in the mesonspectrum?
Lattice calculations predict a spectrumof glueballs. The lightest 3 have JPC
Quantum numbers of 0++ , 2++ and0-+.
The lightest is about 1.6 GeV/c2
Glueball Mass Spectrum
Morningstar et al.f0(980)
f0(1500)
f0(1370)
f0(1710)
a0(980)
a0(1450) K*0(1430)
Flux Tubes andConfinement
Color Field: Because of self interaction, confining flux tubes form between static color charges
Notion of flux tubes comes about from model-independentgeneral considerations. Idea originated with Nambu in the ‘70s
š/r
ground state
transverse phonon modes
Lattice QCD Flux tubes realized Flux
tube
forms
between
Confinement arises from flux tubes and
their excitation leads to a new
spectrum of mesons
Hybrid mesons
Normal mesons
1 GeV mass difference
linear potential
From G. Bali
Normal Mesons Normal mesons occur when theflux tube is in its ground state
LS
S
1
2
S = S + S1 2
J = L + S
C = (-1)L + S
P = (-1)L + 1
Spin/angular momentum configurations& radial excitations generate our knownspectrum of light quark mesons
Nonets characterized by given JPC
Not allowed: exoticcombinations:
JPC = 0-- 0+- 1-+ 2+- …
q
q
q
q
Excited Flux TubesHow do we look for gluonic
degrees of freedom in spectroscopy?
First excited state of flux tube has J=1 andwhen combined with S=1 for quarksgenerate:
JPC = 0-+ 0+- 1+- 1-+ 2-+ 2+-
exotic
q
q
Exotic mesons are not generated when S=0
JPC = 1-- 1++
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
f0(1500)
f2(1270)
f0(980)
f2(1565)+700,000 000 Events
Crystal Barrel Results: antiproton-proton annihilation at rest
f0(1500)
250,000 0 Events
Discovery of the f0(1500) Discovery of the a0(1450)
f0(1500) ’, KK, 4
f0(1370)
The Scalar Mesons
1.5
0++
2.5 2.51.5
0++
Central Production WA102Observes f0(1370)f0(1500)f0(1710)
OverpopulationStrange Decay PatternsSeen in glue-rich reactionsNot in glue-poor
Glueball and Mesonsare mixed, but what isthe mixing scheme?
J/ Decays?
f0(1370) seenf0(1500) ????f0(1710) seen
Awaiting CLEO-c
What about 2++ and 0?
ppE852 Results (18 GeV)
The a2(1320) is the dominantsignal. There is a small (few %)exotic wave.
Interference effects showa resonant structure in .(Assumption of flat backgroundphase as shown as 3.)
Mass = 1370 +-16+50
-30 MeV/c2
Width= 385 +- 40+65-105 MeV/c2
a2
(1400)
Crystal Barrel Results: antiproton-neutron annihilation
Mass = 1400 +- 20 +- 20 MeV/c2
Width= 310+-50+50-30 MeV/c2
Same strength as the a2.
Produced from states with one unit
of angular momentum.Without 1 2/ndf = 3, with = 1.29
Results of Partial Wave Analysis
a1
a2
BenchmarkResonances
a1(1270)a2(1320)2(1670)
2
Benchmarksare needed toshow resonant behavior.
An Exotic Signal in E852
LeakageFrom
Non-exotic Wavedue to imperfectly
understood acceptance
ExoticSignal
1
Correlation ofPhase
&Intensity
M( ) GeV / c2
1(1600)
3 m=1593+-8+28-47 =168+-20+150
-12
’ m=1597+-10+45-10 =340+-40+-50
Current Evidence
Glueballs Hybrids
Overpopulation of thescalar nonet and LGT
predictions suggest thatthe glueball and the
scalar mesons are mixed
JPC = 1-+ states reported
1(1400)
1(1600) ’
by BNL E852, CBARand VES
Complication ismixing with conventional qq
States
Need to observe additionalglueball states
Not without controversy
Not in expected decay modes
Have gluonic excitations been observed ?
CollaborationUS Experimental Groups
A. Dzierba (Spokesperson) - IUC. Meyer (Deputy Spokesperson) - CMUE. Smith (JLab Hall D Group Leader)
L. Dennis (FSU) R. Jones (U Conn)J. Kellie (Glasgow) A. Klein (ODU)G. Lolos (Regina) (chair) A. Szczepaniak (IU)
Collaboration Board
Carnegie Mellon University
Catholic University of America
Christopher Newport University
University of Connecticut
Florida International University
Florida State University
Indiana University
Jefferson Lab
Los Alamos National Lab
Norfolk State University
Old Dominion University
Ohio University
University of Pittsburgh
Renssalaer Polytechnic Institute
University of Glasgow
Institute for HEP - Protvino
Moscow State University
Budker Institute - Novosibirsk
University of Regina
CSSM & University of Adelaide
Carleton University
Carnegie Mellon University
Insitute of Nuclear Physics - Cracow
Hampton University
Indiana University
Los Alamos
North Carolina Central University
University of Pittsburgh
University of Tennessee/Oak Ridge
Other Experimental Groups
Theory Group
90 collaborators25 institutions
New Arc
5 NewCryomodules
5 New Cryomodules
Photon Tagger
Hall D
The Jlab 12 GeV UpgradeThe Jlab 12 GeV Upgrade
Up to 11 GeV electrons
12.2 GeVelectrons
Polarized
Photons
20 Cryomodules
20 Cryomodules
Intense tagged, linearly polarized photons
$70 Million Accelerator$35 Million for Hall D$45 Million for A,B and C
DetectorLead GlassDetector
Solenoid2.5Tesla
Electron Beam from CEBAF
Coherent BremsstrahlungPhoton Beam
Tracking
Target
CerenkovCounter
Time ofFlight
BarrelCalorimeter
Note that tagger is80 m upstream of
detector
Event rate to processor farm:10 kHz and later 180 kHz correspondingto data rates of 50 and 900 Mbytes/sec
respectively
Solenoid & Lead Glass Array
At SLAC
Now at JLab
Recycling of existing equipment
Being Moved to JLab
BNL E852 Pb-Glass ArrayLASS/MEGA Solenoid
flu
x
photon energy (GeV)
12 GeV electronsCoherent Bremsstrahlung
This technique provides requisite energy, flux
and polarization
collimated
Incoherent &coherent spectrum
tagged
0.1% resolution
40%polarization
in peak
electrons in
photons out
spectrometer
diamondcrystal
Optimal Photon Energy
1.0
0.8
0.6
0.4
0.2
0.0
rela
tive
yie
ld
11109876
beam photon energy (GeV)
m[x] = 1.0 GeV = 1.5 GeV = 2.0 GeV = 2.5 GeV
Figure of merit based on:
1. Beam flux and polarization2. Production yields3. Separation of meson/baryon production
Electron endpointenergy of 12 GeV
producedmeson mass
rela
tive y
ield
Staying below 10 GeV allows usto use an all-solenoidal detector.
Optimum photon energyis about 9 GeV
Why Photoproduction ?
A pion or kaon beam, when scattering occurs,
can have its flux tube excitedor
beam
Quark spins anti-aligned
Much data in hand but littleevidence for gluonic excitations
(and not expected)
q
q
befo
req
qaft
er
q
q
aft
er
q
q
befo
re
beamAlmost no data in hand
in the mass regionwhere we expect to find exotic hybrids
when flux tube is excited
Quark spins aligned
__
__
Very little photoproduction data exist.What little there is hint at a differentresonance structure than what is seenin pion production.
In one year of initialrunning, expect 100times pion statistics
In one year of initialrunning, expect 100times pion statistics
Detector designed to do Partial Wave Analysis
Double blind studies of 3 final states
p
n
X
Polarization
m [GeV/c2]
GJ
a2
Detection of Exotic Mesons
f1, b1high multiplicity)’aa
Hybrids predicted to decay to S+P mesons S= nonets P=bj,aj nonets
Predicted Observed?
p -> [, ,
Hybrid Decays
Hall D will be sensitive to a wide variety of decay modes - the measurements of which will be compared against theory predictions.
To certify PWA - consistency checks will be made among different final states for the same decay mode, for example:
b1 0 3
0 2
Should givesame results
Gluonic excitations transfer angular momentum in their decays tothe internal angular momentum of quark pairs not to the relative angularmomentum of daughter meson pairs - this needs testing.
X b1For example, for hybrids: favored
not-favoredX Measure many decay modes!
-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
Acceptance
-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 n
p Xn 00n
Acceptance in
Decay Angles
Gottfried-Jackson frame:
In the rest frame of Xthe decay angles aretheta, phi
assuming 9 GeVphoton beam
Mass [X] = 1.4 GeV
Mass [X] = 1.7 GeV
Mass [X] = 2.0 GeV
Acceptance is high and uniform
Complete Study of neutral and charged final states
Hybrids are expected to decay into complicated final states.Exotic QN’s are smoking guns, but there are non exotic QN’s as well. Need to know decay patterns to understand mixing.
Initial running will be at 5*107 /s, will eventually reach 108
One year of initial running will yield 100 times pion statistics in the channel. Many weaker channels will have sufficient statistics for full PWA. (Will probe fraction of nb cross sections)
PWA is sensitive to channels at about 0.5% of major component and to widths of several hundred MeV.
If Exotics are there, they will be seen. If they are not there, then we will need to reexamine our understanding of QCD.The first hints of exotic states already disagree with what we think we understand about them.
PROJECT STATUS
January 1999 Letter of Intent to Jlab PACDecember 1999 Cassell Committee Review of ProjectAugust 2000 Key Part of the JLAB 12 GeV UpgradeDecember 2000 Presentation at NSAC Town MeetingApril 2001 Reccomendation in NSAC LRPAugust 2001 DOE Review of JLAB, push for CD0January 2002 NSAC LRP ReleasedWinter 2002 CD0 Status at DOE .... 2007 Start Data Taking (hopefully).
SummaryQCD predicts a spectrum of states directly associated with the gluonic degree of freedom and confinement. Exotic Quntum numbers are a definitive signature
Experiments have started to observe states with exotic quantum numbers, but the observations are few, and not in agreement with theoretical expectations.
Photoproduction is expected (vector meson beams) are expected be a very good, yet unexplored way to produce these states.
Hall D will be able to map out a detailed picture of these states and their decays with statistics 100 times better than current pion experiements. Such information will yield important data on the dynamics of glue and its role in QCD.