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Electroproduction of η mesons in the S11(1535) resonance region at high momentum transfer

M. M. Dalton et al.
Phys. Rev. C 80, 015205 – Published 16 July 2009

Abstract

The differential cross section for the process p(e,e'p)η has been measured at Q2~5.7 and 7.0(GeV/c)2 for center-of-mass energies from threshold to 1.8 GeV, encompassing the S11(1535) resonance, which dominates the channel. This is the highest momentum-transfer measurement of this exclusive process to date. The helicity-conserving transition amplitude A1/2, for the production of the S11(1535) resonance, is extracted from the data. Within the limited Q2 now measured, this quantity appears to begin scaling as Q3—a predicted, but not definitive, signal of the dominance of perturbative QCD at Q2~5(GeV/c)2.

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  • Received 26 February 2009

DOI:https://doi.org/10.1103/PhysRevC.80.015205

©2009 American Physical Society

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Vol. 80, Iss. 1 — July 2009

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Images

  • Figure 1
    Figure 1
    The one-photon exchange diagram of the resonance electroproduction process, where, for example, ki is the four-momentum vector of the incoming electron composed of energy E and momentum ki.Reuse & Permissions
  • Figure 2
    Figure 2
    The scattering and reaction plane coordinate systems.Reuse & Permissions
  • Figure 3
    Figure 3
    A plan view of Hall C showing the beamline, target, and the SOS and HMS spectrometers that detected electrons and protons, respectively. Figure from Ref. [2].Reuse & Permissions
  • Figure 4
    Figure 4
    A side view of the HMS detector stack, which is also representative of the SOS. The detected particles travel from left to right, encountering first the two drift chambers (DC) then the first two arrays of scintillators (S1) oriented in the X and Y directions, then the gas Čerenkov detector, the third and fourth scintillator arrays and finally the calorimeter. Figure from Ref. [2]Reuse & Permissions
  • Figure 5
    Figure 5
    The W acceptance of the detector pair for the e(p,e'p)η reaction, in the lower-Q2 configuration, as a function of the laboratory scattering angle and momentum of the proton. The contours are constant W of the hadronic system, for an electron at 47.5° and momentum of 1.74 GeV/c, for the full range of θ* and ϕ=0° and 180°. The solid central contour is W=1.5 GeV, from which they increase in steps of 100 MeV to the outermost at W=1.9 GeV. In practice, the angle and momentum bite of the SOS causes the contours to be much broader. Each black box is the acceptance of a particular HMS setting (Table ). The alternate settings are offset by 1.5° and are a 4.7% increase in momentum, so that they are approximately centered on the points where the boxes join.Reuse & Permissions
  • Figure 6
    Figure 6
    The correlation between Enorm and Np.e. for all the lower-Q2 data. The particle ID cuts to select electrons, Np.e.>0.5 and Enorm>0.7, are visible as dashed lines in the figure. All other cuts listed in Table have already been applied to the data.Reuse & Permissions
  • Figure 7
    Figure 7
    Coincidence time spectrum for the lower-Q2 data with all of the “standard” cuts except the coincidence time cut. The dark-gray shaded region represents the 3-ns-wide proton cut. The 2-ns beam structure is clear in the accidental background. Data from the light-gray shaded regions was used to estimate the amount of accidentals in each (W, cosθη*, ϕη* and mx2) bin under the proton peak.Reuse & Permissions
  • Figure 8
    Figure 8
    Missing-mass-squared, mx2, from Eq. (1), for all the lower-Q2 data.Reuse & Permissions
  • Figure 9
    Figure 9
    The ϕη dependence of missing-mass-squared distributions for W=1.5 GeV and cosθη*=0.916. The (green) points are the data while the solid fill is the sum of the simulations. The multipion background component is the light-gray filled area and η production simulation component has the darker gray fill. The dot-dashed lines shows the region within which the background fit is done while the dashed lines show the region within which the η cross section is extracted.Reuse & Permissions
  • Figure 10
    Figure 10
    The ϕη dependence of missing-mass-squared distributions for W=1.5 GeV and cosθη*=0.416. Symbols as in Fig. 9. Panels with ϕη=1.178, 1.963, 4.320, and 5.105 are the out-of-plane ϕ bins where the simulations of the signal and background are sufficiently similar to make a two-parameter bin-by-bin fit unreliable.Reuse & Permissions
  • Figure 11
    Figure 11
    The W dependence of missing-mass-squared distributions for cosθη*=0.916 and ϕ=3.534 radians. Symbols as in Fig. 9.Reuse & Permissions
  • Figure 12
    Figure 12
    The cosθη* dependence of missing-mass-squared distributions for W=1.5 GeV and ϕ=3.534 radians. Symbols as in Fig. 9. The vertical dashed lines, which show the region within which the η cross section is extracted, vary with cosθη* to accommodate the changing resolution.Reuse & Permissions
  • Figure 13
    Figure 13
    The W dependence of the normalization coefficient of the multipion background simulation.Reuse & Permissions
  • Figure 14
    Figure 14
    The cosθ* dependence of the normalization coefficient of the multipion background simulation.Reuse & Permissions
  • Figure 15
    Figure 15
    The (green) points are the mx2 distribution of the full set of data off the “dummy” target cell, and the gray filled histogram is the simulation of multipion background from hydrogen. The simulation is arbitrarily normalized to match the data, with the same factor in all three panels. Note the similarity in shape.Reuse & Permissions
  • Figure 16
    Figure 16
    Radiative corrections for 1<cosθη<13. Uncertainty is due to Monte Carlo statistics only.Reuse & Permissions
  • Figure 17
    Figure 17
    Radiative corrections for 13<cosθη<13. Uncertainty is due to Monte Carlo statistics only. Symbols as in Fig. 16.Reuse & Permissions
  • Figure 18
    Figure 18
    Radiative corrections for ⅓ < cosθη < 1. Uncertainty is due to Monte Carlo statistics only. Symbols as in Fig. 16.Reuse & Permissions
  • Figure 19
    Figure 19
    Ratio of yield of elastic ep coincidence events to predicted yield from Monte Carlo (Yield Data/Yield MC) plotted versus θe for θSOS=47.5° and three different combinations of θHMS and pHMS. The solid line is the average ratio =0.95±0.01, of all points between θe=45.5 to 49.5°. The corresponding value of electron δ for a given θe is given by the upper x axis.Reuse & Permissions
  • Figure 20
    Figure 20
    Inclusive inelastic differential cross sections as measured by the SOS spectrometer centered at 47.5° and 70°, as a function of W, with the angular cut 30<dy/dz<30 mr. The curves are from a fit to world data [24].Reuse & Permissions
  • Figure 21
    Figure 21
    Extracted epepη differential cross sections for the lower-Q2 setting. The solid (blue) curve is a fit of Eq. (8) to each W bin. The dashed curve is the ETA-MAID [34] isobar model for η electroproduction from the nucleon at Q2=5 GeV2, projected to the appropriate Q2 for each W bin by the factor [5GeV2/Q2(W)]3. The inner error bars are statistical and the outer error bars are the quadrature sum of the statistical and systematic errors.Reuse & Permissions
  • Figure 22
    Figure 22
    Extracted parameters from fits of Eq. (8) to the lower-Q2 differential cross section, shown as curves in Fig. 21.Reuse & Permissions
  • Figure 23
    Figure 23
    The result of fits to the differential cross section, plotted as the ratio of the linear cosθη* term to the isotropic component, for the present work and other η-electroproduction data [2, 5, 6]. The black dotted line is drawn at W=1.535 GeV, the nominal mass for the S11 resonance.Reuse & Permissions
  • Figure 24
    Figure 24
    Extracted epepη differential cross sections for the higher-Q2 setting. The (blue) solid curve is a fit to the data of the form dσ/dΩ*=A+Bcosθ*. The dashed curve is the ETA-MAID model [34] at Q2=5GeV2, projected to the appropriate Q2 for each W bin by the factor [5GeV2/Q2(W)]3. The inner error bars are statistical and the outer error bars, the quadrature sum of the statistical and systematic errors.Reuse & Permissions
  • Figure 25
    Figure 25
    The ratio of the quadratic cos2θη* term to the isotropic component for fits to the η-electroproduction differential cross section for the present work and other data [2, 6]. Symbols are the same as in Fig. 23.Reuse & Permissions
  • Figure 26
    Figure 26
    A simultaneous fit to the lower-Q2 and higher-Q2 data of the sum (solid line) of a relativistic Breit-Wigner (long dash) and nonresonant background term (short dashed line). The data are the total cross section determined from 4πdσ/dΩ*. The background was constrained as described in the text.Reuse & Permissions
  • Figure 27
    Figure 27
    Plot of the 1-σ contours from the various Breit-Wigner fits to the data.Reuse & Permissions
  • Figure 28
    Figure 28
    Values for A1/2(Q2) determined from σR for the present and other data [2, 5, 6] (consistently with WR=1.53 GeV, ΓR=150 MeV, and bη=0.55). The curves are from Refs. [36, 37, 38, 39, 40].Reuse & Permissions
  • Figure 29
    Figure 29
    The Q2 dependence of Q3A1/2 for η production. Scaling in this quantity appears to begin at a photon momentum transfer of Q2~5GeV2. The dashed lines are a high Q2, pQCD calculation from Carlson and Poor [4] using three different nucleon distribution amplitudes.Reuse & Permissions
  • Figure 30
    Figure 30
    The Q2 dependence of Q3A1/2(S11)/Q4GMp for η production.Reuse & Permissions
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