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Tanja Horn Jefferson Lab
The Pion Form Factor Tanja Horn Jefferson Lab BNL Nuclear Physics Seminar, 27 Feb, 2007
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JLab Fπ-2 Collaboration
R. Ent, D. Gaskell, M.K. Jones, D. Mack, D. Meekins, J. Roche, G. Smith, W. Vulcan, G. Warren, S. Wood Jefferson Lab, Newport News, VA , USA E. Brash, G.M. Huber, V. Kovaltchouk, G.J. Lolos, C. Xu University of Regina, Regina, SK, Canada H. Blok, V. Tvaskis Vrije Universiteit, Amsterdam, Netherlands E. Beise, H. Breuer, C.C. Chang, T. Horn, P. King, J. Liu, P.G. Roos University of Maryland, College Park, MD, USA W. Boeglin, P. Markowitz, J. Reinhold Florida International University, FL, USA J. Arrington, R. Holt, D. Potterveld, P. Reimer, X. Zheng Argonne National Laboratory, Argonne, IL, USA H. Mkrtchyan, V. Tadevosyan Yerevan Physics Institute, Yerevan, Armenia S. Jin, W. Kim Kyungook National University, Taegu, Korea M.E. Christy, L.G. Tang Hampton University, Hampton, VA, USA J. Volmer DESY, Hamburg, Germany T. Miyoshi, Y. Okayasu, A. Matsumura Tohuku University, Sendai, Japan B. Barrett, A. Sarty Saint Mary’s University, Halifax, NS Canada K. Aniol, D. Margaziotis California State University, Los Angeles, CA, USA L. Pentchev, C. Perdrisat College of William and Mary, Williamsburg, VA, USA I. Niculescu James Madison University, Harrisonburg, VA, USA V. Punjabi Norfolk State University, Norfolk, VA, USA E. Gibson California State University, Sacramento, CA, USA
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Hadronic Form Factors in QCD
Quantum Chromo-Dynamics (QCD) is very successful describing strong interactions BUT, we are unable to construct a quantitative description of hadrons in terms of the underlying constituents, quarks and gluons. We know that there is an asymptotic limit, but how do we get there and what governs the transition? - JLAB Short Distance Asymptotic Freedom Perturbative QCD Long Distance Binding Collective degrees of Freedom Fπ Form factors provide important information about the transition between non-perturbative and perturbative regimes Meaningful constraint on theoretical models requires measurements at high precision
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Scientific Motivation – why pions?
The pion form factor is one of the simplest objects available for experimental studies Simple qq valence structure Expect pQCD description to be valid at lower values of Q2 relative to nucleon Test case for all models of hadronic structure At large Q2 one can calculate Fπ in pQCD – in the Q2→∞ this reduces to the well known form One hard gluon exchange where f2π=93 MeV is the π+→μ+ν decay constant
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Modeling QCD – the transition from the non-perturbative regime
Fundamental question: what is the structure of π+ at finite values of Q2? – i.e. at experimentally accessible energies At what value of Q2 will pQCD dominate over soft contributions? Theoretical challenge: at moderate values of Q2 both hard and soft contributions must be taken into account Braun et al. calculate ~30% at Q2=1 GeV2 Feynman Mechanism The limits on Fπ are well defined and many treatments for soft physics are available, BUT experimental data are needed to de-convolute the role of soft and hard contributions at intermediate values of Q2 – study of space-like Fπ unique to JLab
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More modeling or implications
Following slides are in progress … mostly placeholders at the moment
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Fπ via Pion Electroproduction
Fπ can be measured directly from π+e scattering (S.R. Amendolia et al., NP B277 (1986)) up to Q2~0.3 GeV2 No “free pion” target – to extend measurement of Fπ to larger Q2 values use “virtual pion cloud” of the proton The t-channel diagram dominates sigL at small -t Method check - Extracted results are in good agreement with π+e data
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Pion Electroproduction Kinematics
Q2= |q|2 – ω2 t=(q - pπ)2 W=√-Q2 + M2 + 2Mω scattering plane reaction plane Hadronic information determined by Lorentz invariants Q2= |q|2 – ω2 W=√-Q2 + M + 2Mω t=(q - pπ)2 pπ = momentum of scattered pion θπ = angle between scattered pion and virtual photon φπ = angle between scattering and reaction plane
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Pion Electroproduction Cross Section
The virtual photon cross section can be written in terms of contributions from transversely and longitudinally polarized photons. In general, LT and TT → 0 by integrating over φ acceptance
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“Simple” Longitudinal-Transverse Separation
From φ-dependence have σTT and σLT Determine σT+ ε σL for high and low ε in each t-bin for each Q2 Isolate σL, by varying photon polarization, ε
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Cross Section Separation
Cross Section Extraction φ acceptance not uniform Measure σLT and σTT Extract σL by simultaneous fit using measured azimuthal angle (φπ) and knowledge of photon polarization (ε)
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Extracting Fπ from π+ Electroproduction Data
Extraction of Fπ from σL relies on pion pole dominance In this simple picture the t-channel process dominates σL BUT no reliable phenomenological extrapolation to the t=mπ2 pole More reliable technique: Extract Fπ from σL data using a model incorporating pion electroproduction Test of this technique: 12 GeV
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Kinematic Considerations
For maximal contribution from the π+ pole need data at smallest possible –t For a given Q2, -tmin gets smaller as W increases Smaller -tmin means Fπ measurements with reduced model uncertainty in the Fπ extraction The t-dependence of σL must be known for the extraction of Only three of W, Q2, -t and θ are independent To measure the t-dependence we vary θ - for nonzero values of θ the interference terms contribute and must be measured explicitly
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Pion Electroproduction Models
MAID Only useful for W < 2 GeV, Fπ-2 kinematics above this region Born term models Do not describe t-dependence well away from pole VGL/Regge Appropriate at W > 2 GeV Seems to under-predict σT consistently Constituent Quark Model Same kinematic range as VGL/Regge, two free parameters Not previously used in data analysis
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VGL Regge Model Pion electroproduction in terms of exchange of π and ρ like particles Model parameters fixed from pion photoproduction Free parameters: Fπ and Fρ ρ exchange does not influence σL at small -t Fit to σL to model gives Fπ at each Q2
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Precision Fπ data up to Q2=2.45 GeV2
Extension of 1997 run at highest possible value of Q2 with 6 GeV beam at JLab New data at higher W Repeat Q2=1.60 GeV2 closer to t=m2π to study model uncertainties Successfully completed in Hall C at JLab 2003 Coincidence measurement between charged pions in HMS and electrons in SOS Separate σL/σT via Rosenbluth separation HMS: 6 GeV SOS: 1.7 GeV Exp Q2 (GeV2) W (GeV) |t| (Gev)2 Ee (GeV) Fπ-1 1.95 Fπ-2 1.6,2.45 2.22 0.093,0.189
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Experimental Details Hall C spectrometers Coincidence measurement
SOS detects e- HMS detects π+ Targets Liquid 4-cm H/D cells Al (dummy) target for background measurement 12C solid targets for optics calibration HMS Aerogel Improvement of p/π+/K+ PID at large momenta, first use in 2003 Built by Yerevan group (Nucl. Instrum. Meth. A548(2005)364)
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Good Event Selection Coincidence measurement between charged pions in HMS and electrons in SOS Coincidence time resolution ~ ps Cut: ± 1ns Protons in HMS rejected using coincidence time and Aerogel Cerenkov Electrons in SOS identified by gas Cerenkov and Calorimeter Exclusive neutron final state selected with missing mass cut: 0.92 ‹ MM ‹ 0.98 GeV After PID cuts almost no random coincidences.
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Random Background Subtraction
Random e-π background subtracted using coincidence time Contribution < 1% for H including all cuts Separate real π and p events using coincidence time Issue in random subtraction: π’s can interact in scintillators – produce slow protons Eliminate with time of flight cut Cut Efficiency: ~96% Real protons
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Kinematic Coverage Have full coverage in φ BUT acceptance not uniform
Measure σTT and σLT by taking data at three angles: θπ=0, +4, -3 degrees W/Q2 phase space covered at low and high ε is different For L/T separation use cuts to define common W/Q2 phase space Θπ=0 Θπ=+4 Θπ=-3 -t=0.1 -t=0.3 Q2=1.60, High ε Radial coordinate: -t, azimuthal coordinate: φ
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Cross Section Extraction
Compare experimental yields to Monte Carlo of the experiment Model for H(e,e’π+) based on pion electroproduction data Radiative effects, pion decay, energy loss, multiple scattering COSY model for spectrometer optics Extract σL by simultaneous fit using measured azimuthal angle (φπ) and knowledge of photon polarization (ε).
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Spectrometer Uncertainties
Uncertainty in separated cross sections has both statistical and systematic sources Statistical uncertainty in ranges between 1 and 2% Point-to-point errors amplified by 1/Δε in L-T separation Scale errors propagate directly into separated cross section Uncertainties in spectrometer quantities parameterized using over-constrained 1H(e,e’p) reaction Beam energy and momenta to <0.1% Spectrometer angles to ~0.5mrad Spectrometer acceptance verified by comparing e-p elastic scattering data to global parameterization Agreement better than 2% Source Pt-Pt Scale t-correlated Acceptance 1.0(0.6)% 1.0% 0.6% Radiative Corrections 0.1% 2.0% 0.4% Pion Absorption - Pion Decay 0.03% Model Dependence 0.2% 1.1(1.3)% Kinematics HMS Tracking Charge 0.5% 0.3% Target Thickness 0.8% Detection Efficiency
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Models for Fpi Extraction
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Regge Model
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Comparison to VGL Model
Points include 1.0(0.6)% point-to-point systematic uncertainty (dominated by acceptance) 3.5 % normalization (correlated) uncertainty (radiative corrections, pion absorption, pion decay, kinematic uncertainties) 1.8(1.9)% “t-correlated” uncertainties, influence t-dependence at fixed ε Compare to VGL/Regge model with Λπ2=0.513 (0.491) σL well described, but σT under-predicted systematically
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Fπ 1 results First phase of the measurement ran in Hall C at JLab in 1997, thesis students: J. Volmer and K. Vansyoc Measured pion electroproduction from H and 2H Extracted σL, σT, σTT, and σLT at W=1.95 GeV, Q2 = 0.6, 0.75, 1.0, 1.6 GeV2 Fπ was determined by comparing σL to a Regge calculation by Vanderhaeghen, Guidal, Laget (VGL, PRC 57(1998)1454) Model parameters fixed from pion photo-production, free parameters: Fπ and Fρ. Fit to σL to model gives Fπ at each Q2
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Outline Introduction Fπ from pion electroproduction data :
Fπ1 and Fπ2 in Hall C/Jefferson Lab Some other comment: Something else A long explanation of something relevant: A third point Summary
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Pion Electroproduction Unpolarized Cross Section
Q2= |q|2 – ω2 t=(q - pπ)2 W=√-Q2 + M2 + 2Mω scattering plane reaction plane The lab cross section can be expressed in terms of virtual photon flux, Jacobian and virtual photon cross section. The virtual photon cross section can be written in terms of contributions from transversely and longitudinally polarized photons.
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