Search for Gluonic Excitations with GlueX at Jefferson Lab

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Search for Gluonic Excitations with GlueX at Jefferson Lab Volker Credé Florida State University Tallahassee, FL The Structure and Dynamics of Hadrons Hirschegg, 01/19/2007

Outline 1 2 3 4

Outline 1 2 3 4

The GlueX Collaboration 100 Physicists Members from 7 countries Australia Canada, Mexico, USA Greece, Russia, Scotland Active group since 1998 http://www.gluex.org New members are welcome!

Outline 1 2 3 4

Flux Tubes force 1/r 2 distance QED Confinement arises from flux tubes and their excitation leads to a new spectrum of mesons. QCD force constant distance Color Fields: Because of self interaction between gluons, confining flux tubes form between static color charges. G. Bali et al., Phys. Rev. D62, (2000) 054503

Ordinary Mesons J PC 2S+1 L J Parity P = ( 1) L+1 Charge conjugation (defined for neutral mesons) C = ( 1) L+S G parity G = C( 1) I

Ordinary Mesons J PC 2S+1 L J Parity P = ( 1) L+1 Charge conjugation (defined for neutral mesons) C = ( 1) L+S G parity G = C( 1) I L = 0, S = 1 : ρ, ω, φ (J PC = 1 ) L = 0, S = 0 : e.g. π (J PC = 0 + )

Hybrid Mesons L = 0, S = 1 : ρ, ω, φ (J PC = 1 ) flux tube J PC = 1 + or 1 + (from lattice QCD and flux-tube models) L = 0, S = 0 : e.g. π (J PC = 0 + )

Hybrid Mesons L = 0, S = 1 : ρ, ω, φ (J PC = 1 ) flux tube J PC = 1 + or 1 + L = 0, S = 0 : e.g. π (J PC = 0 + ) Pseudoscalar Mesons: quarks J PC flux tube J PC = 1, 1 ++ Vector Mesons: quarks J PC flux tube J PC = 0 +, 1 +, 2 + 0 +, 1 +, 2 +

Hybrid-Meson Production L = 0, S = 1 : ρ, ω, φ (J PC = 1 ) flux tube J PC = 1 + or 1 + L = 0, S = 0 : e.g. π (J PC = 0 + ) Pseudoscalar Probe: quarks J PC flux tube J PC = 1, 1 ++ Vector Probe: quarks J PC flux tube J PC = 0 +, 1 +, 2 + 0 +, 1 +, 2 +

Hybrid-Meson Production One result of the scattering process of an incoming probe off the target particle can be the excitation of the flux tube: Not favored for qq probe in L = 0 and S = 0 Favored for incoming vector probes with L = 0 and S = 1 Photoproduction

QCD Potential Energy density in the color field flux tube r o (V[r] V[2r o ]) excited states ground state The observation of exotic quantum numbers are the best experimental signal of gluonic excitations. Q Q r/r o Gluonic excitations provide an experimental measurement of the excited QCD potential.

Each box corresponds to 4 nonets (2 nonets for L = 0) Mass (GeV/c 2 ) L = qq angular momentum Lattice calculations: 1 + lightest: 1.9 GeV/c 2

Decays of Hybrids Decay calculations are model dependent, but the 3 P 0 model does a good job of describing normal meson decays. The angular momentum in the flux tube stays in one of the daughter mesons ((L = 1) and (L = 0)): } L = 0 π, ρ, η, ω,... ηπ, ρπ,... not preferred decays L = 1 a, b, h, f,...

Experimental Evidence for Exotic 1 + Signals π 1 (1400): Width 0.3 GeV, Decays: only πη Weak signal in πp production (scattering??) and strong signal in antiproton-deuterium annihilation Controversy In Crystal-Barrel data, the ηπ 0 channel is not conclusive. Recent analysis by A. Szczepaniak shows that the exotic wave is not resonant a rescattering effect. The signal is far too light to be a hybrid by any model.

Experimental Evidence for Exotic 1 + Signals π 1 (1400): Width 0.3 GeV, Decays: only πη Weak signal in πp production (scattering??) and strong signal in antiproton-deuterium annihilation Probably not a hybrid

Experimental Evidence for Exotic 1 + Signals π 1 (1400): Width 0.3 GeV, Decays: only πη Weak signal in πp production (scattering??) and strong signal in antiproton-deuterium annihilation Probably not a hybrid π 1 (1600): Width 0.16 GeV, Decays: ρπ, η π, (b 1 π) Only seen in πp production (E852, VES) E852 Results 3π m = 1593 Γ = 168 η π m = 1597 Γ = 340 (A. Szczepaniak: background rescattering) f 1 π m = 1709 Γ = 403 b 1 π m = 1687 Γ = 206

Experimental Evidence for Exotic 1 + Signals π 1 (1400): Width 0.3 GeV, Decays: only πη Weak signal in πp production (scattering??) and strong signal in antiproton-deuterium annihilation Probably not a hybrid π 1 (1600): Width 0.16 GeV, Decays: ρπ, η π, (b 1 π) Only seen in πp production (E852, VES) Still room for a narrower exotic state

Experimental Evidence for Exotic 1 + Signals π 1 (1400): Width 0.3 GeV, Decays: only πη Weak signal in πp production (scattering??) and strong signal in antiproton-deuterium annihilation Probably not a hybrid π 1 (1600): Width 0.16 GeV, Decays: ρπ, η π, (b 1 π) Only seen in πp production (E852, VES) Does it exist? No evidence in Dzierba et al., PRD 73 (2006)

Experimental Evidence for Exotic 1 + Signals π 1 (1400): Width 0.3 GeV, Decays: only πη Weak signal in πp production (scattering??) and strong signal in antiproton-deuterium annihilation Probably not a hybrid π 1 (1600): Width 0.16 GeV, Decays: ρπ, η π, (b 1 π) Only seen in πp production (E852, VES) Does it exist? No evidence in Dzierba et al., PRD 73 (2006) π 1 (2000): Weak evidence in preferred hybrid modes f 1 π and b 1 π Right place, needs confirmation

Exotics and QCD To establish the existence of gluonic excitations, the existence and nonet nature of the 1 + state needs to be established. Also, 0 + and 2 + nonets need to be established. Decay pattern are crucial: Have provided the most sensitive information in the scalar glueball sector

Outline 1 2 3 4

CEBAF at Jefferson Lab

Detector Requirements A partial-wave amplitude analysis is required in order to identify exotic hybrid, non-exotic hybrid, and conventional meson nonets. This puts demands on the experiment: Hermiticity (4π detector) Uniform detector acceptance in the variables appropriate for PWA Energy and momentum resolution Particle identification (sensitivity to decay modes) High statistics (photon flux and rate capability) Appropriate beam energy (reach masses/good acceptance) Identification of production mechanism (linear polarization)

Finding the Optimal Energy... Detector optimized for 8-9 GeV photons: flux of photons: millions/sec 12 10 8 6 4 2 Photon Flux in Coherent Peak electron energy: = 12 GeV = 11 GeV = 10 GeV Total Hadronic Rate constant at approx 20 KHz linear polarization 0.6 0.5 0.4 0.3 0.2 0.1 Linear Polarization electron energy: 12 GeV = 11 GeV = 10 GeV 0 7 8 9 10 11 photon beam momentum (GeV) 12 0.0 7 8 9 10 11 12 photon beam momentum (GeV)

Acceptance for Different Effective Masses γp -> n π + π + π Acceptance 1 0.8 0.6 Mass(X) = 1.4 GeV Acceptance 1 0.8 0.6 0.4 0.2 Mass(X) = 1.7 GeV Mass(X) = 2.0 GeV 5 GeV 0.4 0.2 0-1 -0.8-0.6-0.4-0.2-0 0.2 0.4 0.6 0.8 1 Cos(θ GJ ) 0-3 -2-1 0 1 2 3 φ GJ

Acceptance for Different Effective Masses γp -> n ω π 0 π + Acceptance 1 0.8 0.6 Mass(X) = 1.4 GeV Acceptance 1 0.8 0.6 0.4 0.2 Mass(X) = 1.7 GeV Mass(X) = 2.0 GeV 5 GeV 0.4 0.2 0-1 -0.8-0.6-0.4-0.2-0 0.2 0.4 0.6 0.8 1 Cos(θ GJ ) 0-3 -2-1 0 1 2 3 φ GJ

Radiator Quadrupole Return yoke 0 5m Full-energy electrons (13.4 bend) Photon beam k/e 0 = 0.95 0.90 0.80 0.70 0.60 0.50 0.40 Focal plane 0.30 0.20 Coherent Bremsstrahlung 15 micron diamond radiator 1 µa 12 GeV electron beam fine steering magnets crystal radiator mount tagging spectrometer primary collimator and sweeping magnet secondary collimator and shielding photon beam dump photon beam pipe photon source and tagger building electron beam dump experimental hall

Linear Polarization Coherent Bremsstrahlung 15 micron diamond radiator 1 µa 12 GeV electron beam Linear Polarization is helpful in extracting decay amplitudes.

Linear Polarization and Decay Angular Distributions Possible Example: ρ ππ or φ KK In the rest frame of the vector, the two-pseudoscalar w.f. is: Y m 1 (θ, φ) sin θ e imφ (s-channel helicity conservation) For circularly-polarized photons (either m = 1 or m = 1), the square of amplitude carries no φ information. However, for linearly-polarized photons: e. g. x > = R > + L > 2 sin θ cos φ For in-plane photons, there is a cos 2 φ dependence.

Linear Polarization Coherent Bremsstrahlung 15 micron diamond radiator 1 µa 12 GeV electron beam Linear Polarization is helpful in extracting decay amplitudes. essential in identifying the production mechanism. a filter for exotics.

Linear Polarization and Production Mechanism Example: Separating Natural-Parity (0 + ) from Unnatural-Parity (0 ) Exchange For circularly-polarized photons: R > (m = 1) A N + A U L > (m = 1) A N A U For linearly-polarized photons: x > = R > + L > A N R > L > y > = i 2 2 A U

Detector R & D Work: Drift Chambers Model of straw-tube chamber Cylindrical Drift Chamber Barrel Calorimeter/Central Time of Flight Cylindrical Drift Chamber Forward Drift Chambers Lead Glass Array Solenoid Target Cerenkov Vertex Detector 2 meters Forward Time of Flight

Detector R & D Work: Drift Chambers Forward Drift Chamber Cylindrical Drift Chamber

Detector R & D Work: Solenoid Refurbishment LASS Solenoid Superconducting 2.5 T Used in Los Alamos MEGA Experiment Moved to IUCF for Refurbishing

Detector R & D Work: Calorimeters Barrel Calorimeter Pb-SciFib Scintillating fibers (1 mm) embadded in matrix of lead Resolution σ/e 6.3 % E

Detector R & D Work: Calorimeters Existing Pb-Glass Forward Detector Barrel Calorimeter Pb-SciFib Scintillating fibers (1 mm) embadded in matrix of lead Resolution σ/e 6.3 % E Upstream Photon Detector

Detector R & D Work: Particle Identification 1 Time-of-Flight (TOF) 2 Cerenkov detector 3 de/dx from tracking chambers Barrel Calorimeter/Central Time of Flight Cylindrical Drift Chamber Forward Drift Chambers Lead Glass Array Solenoid Target Cerenkov Vertex Detector 2 meters Forward Time of Flight TOF Tests (IHEP)

Outline 1 2 3 4

The scale of data from GlueX will be comparable to the LHC experiments Grid technologies will be crucial Tools to parallelize the analysis of 100,000,000 event data sets are being developed Theorists need to be closely integrated into the analyses fom the start Partial wave analysis is the tool to find exotic states Theoretical underpinnings of PWA need to be looked at closely What are the model assumptions? How do they affect the results?

12-GeV Upgrade CD-0 Signing at Jefferson Lab (April 19, 2004) CD 1 for JLab Facilities Upgrade Secretary of Energy announces Approval and Funding for Project (February 2006) CD 2 in Summer 2007