Nonpole Backgrounds in the Extraction of Fp - PowerPoint PPT Presentation

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Nonpole Backgrounds in the Extraction of Fp

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Non-pole Backgrounds in the Extraction of Fp ... A. Mkrtchyan, H. Mkrtchyan, V. Tadevosyan, E. Brash, K. Aniol, J. Calarco, P. King, J. Roche ... – PowerPoint PPT presentation

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Title: Nonpole Backgrounds in the Extraction of Fp


1
Non-pole Backgrounds in the Extraction of Fp
H. Avakian, P. Bosted, H. Fenker, R. Feuerbach,
D. Gaskell, D. Higinbotham, T. Horn, M. Jones,
D. Mack, C. Butuceanu, G. Huber, A. Sarty, W.
Boeglin, P. Markowitz, J. Reinhold, D. Dutta, V.
Koubarovski, P. Stoler, A. Asaturyan, A.
Mkrtchyan, H. Mkrtchyan, V. Tadevosyan, E. Brash,
K. Aniol, J. Calarco, P. King, J. Roche JLab,
Regina, Saint Marys, Florida International,
Mississippi State, RPI, Yerevan, CNU, California
State, New Hampshire, Ohio University
  • Motivation
  • Experimental Details
  • Summary

Hall A Collaboration Meeting
January 2006
2
Extracting Fp from sL data in p production
  • In t-pole approximation
  • Want smallest possible -t to ensure t-channel
    dominance

3
Results from Fp-2
  • The VGL Regge model describes sL for p well
  • Note that at tmin (maximal pole contribution)
    still only have sL/sT 1 at Q22.45 GeV2
  • Constraint on non-pole backgrounds requires
    experimental data

Horn et al., Phys. Rev. Lett. 97, 192001 (2006)
Vanderhaeghen, Guidal and Laget, Phys. Rev. C57,
1454 (1998).
4
Context
  • Understanding of hadronic structure via
    measurement of Fp is one of the high priorities
    at 12 GeV
  • Extraction of Fp relies on pion pole dominance
    what about other processes?
  • Limited knowledge of non-pole contributions
    limits kinematic range of Fp measurement
  • Interpretation on experimental data widely
    considered reliable only below t0.2 GeV2
  • This kinematic contraint is the primary reason
    why we are limited to Q22.5 GeV2 at JLab at 6 GeV

5
Size of non-pole contributions
  • CarlsonMilana indicated a significant
    contribution of non-leading processes
    complicating the extraction of Fp
  • Background ratio rises dramatically once tmingt0.2
  • Other theoretical predictions can be obtained
    from
  • VGL/Regge model
  • GPD formalism

Interpretation of Fp data considered reliable for
-tlt0.2 GeV2
  • But constructing an upper bound on -t difficult
    due to poor quality of existing data.

Carlson Milana, Phys. Rev. Lett. 65, 1717
(1990)
6
Motivation -
  • Non-pole contributions can be constrained using
    the po longitudinal cross section
  • Can be related to the one from p using e.g. GPD
    formalism
  • Many studies of po unseparated cross sections in
    the resonance region, but contribution of sL
    effectively unknown above the resonance region
  • JLab preliminary data from Hall A (DVCS,
    Q21.5-2.5 GeV2, W1.9-2.3 GeV) and Hall B (e16,
    Q21-5 GeV2) available both unseparated

7
Theoretical Predictions for p and po cross
sections
Separated sL
  • Theoretical models based on Regge and GPD
    formalism describe sL for p quite well
  • But po prediction for sL differs by order of
    magnitude
  • Theoretical uncertainty quite large
  • Preliminary unseparated po data from Hall A/B in
    this kinematic region
  • No information on relative sL contribution

Vanderhaeghen, Guidal and Laget, Phys. Rev. C57,
1454 (1998).
Vanderhaeghen, Guichon and Guidal, Phys. Rev.
D60 (1999).
8
Non-pole contributions in the GPD Framework
VGG/GPD prediction
  • Amplitudes for p and po composed of the same
    GPDs, but different linear combinations

po
p
  • Obtain non-pole contributions by comparing po and
    p production amplitudes, MLApNBpN
  • In the limit t ?(mp)2 the p amplitude contains a
    strong singularity (pion pole)

9
Motivation Summary
  • Constraining the non-pole contributions in the
    extraction of Fp requires experimental data
  • Systematic measurement of po cross section could
    constrain the size
  • If the non-pole contributions are smaller than
    anticipated this would significantly increase
    the kinematic range accessible for the Fp
    measurement at 12 GeV
  • Constraining the contribution of sL in po
    production will allow for easier planning of
    Rosenbluth separations

10
Cross Section Separation via Rosenbluth Technique
  • Cross Section Extraction
  • For uniform f-acceptance, sTT, sLT 0 when
    integrated over f
  • Determine sT e sL for high and low e in each
    t-bin for each Q2
  • Isolate sL, by varying photon polarization, e
  • Small sL makes traditional Rosenbluth separation
    difficult due to unfavorable error propagation
    with two different acceptances

VGG/GPD
VGL/Regge
11
Cross Sections via Recoil Polarization
  • In parallel kinematics can relate sL/sT to recoil
    polarization observables
  • Avoids some of the adverse systematic effects due
    to small R in Rosenbluth technique.
  • Using the properties of the independent helicity
    amplitudes in parallel kinematics sL/sT is
    related to Pz
  • From the combination of R and s0 one can obtain sL

12
Experiment Overview
  • 100uA, 5.75 GeV beam, 80 polarized, 10-cm LH2
    target
  • Standard Hall A setup
  • Coincidence measurement with recoil proton into
    HRS with FPP and electrons in the electron arm,
    H(e,ep)po
  • FPP analyzing power relatively large in this
    region
  • Kinematics chosen to overlap with p data from
    Fp-2 and pCT allowing for direct comparison

Fp-2
pCT
13
Parallel Kinematics
  • For recoil polarization analysis all data taken
    in parallel kinematics
  • Cuts in ?/f select events
  • Taking data to left and right of virtual photon
    could allow for t-dependent studies of
    unseparated cross section
  • Radial coordinate ?
  • Azimuthal coordinate f

14
FPP analyzing power
  • Low momentum protons lt760 MeV Los Alamos fit
    applicable, McNaughton et al., Nucl. Instrum.
    Meth. A241, 435 (1985)
  • But in 2006 LEDEX took data for similar proton
    momenta in Hall A, so use this
  • FoM relatively large for proposed kinematics

Preliminary LEDEX data courtesy of R. Gilman et
al.
15
Hard Photon Backgrounds
  • Reconstructed photon smeared out under po peak
    Mx cuts not useful
  • Use simulation for fitting both peaks
  • Subtract bin-by-bin from azimuthal dependence of
    the asymmetry in FPP
  • Relative contribution of po and hard photon
    background in good agreement with Hall B
    preliminary data
  • Relative scaling based on VGL po cross sections
    and VGG DVCSBH cross sections

Q23.8, W2.0, x0.55
po
?
Vanderhaeghen, Guichon and Guidal, Phys. Rev.
D60 (1999).
16
DVCS and Bethe-Heitler Contributions
  • Contribution of hard photons requires full
    background subtraction.
  • Bethe-Heitler process dominates photon cross
    section
  • Contribution of DVCS to total cross section
    10-20
  • Bethe-Heitler propagators are no problem for
    these kinematics

Vanderhaeghen, Guichon and Guidal, Phys. Rev.
D60 (1999).
17
Other Backgrounds
  • End caps subtracted using dummy target data
  • Online singles rates are low, removed with
    offline cuts
  • Electron momentum is too low for elastics to be
    in acceptance
  • Missing mass cuts separate po/?

18
What is needed?
  • Standard Hall A HRS configuration with FPP
  • Installation of standard 10-cm LH2 cryotarget
  • 5.75 GeV beam, 80 polarization
  • Some FPP checkout and calibration

19
Projected Uncertainties
  • Measure po cross section at Q22.45, 4.0 GeV2,
    where p data are available
  • Statistical uncertainty in recoil polarization
    measurement dominates uncertainty
  • Measure sL/s0 contribution to 10

po
p
20
Projected Uncertainties
  • Fixed W scan at three values of Q2 up to Q24.0
    GeV2
  • Measure relative sL/s0 contribution of to 10

21
Beam Time Estimate
  • Elastic data for proton absorption studies and
    calibration
  • Spectrometer angle and momentum changes
  • Some FPP checkout
  • Polarization measurement

22
Summary
  • Non-pole contributions in the extraction of Fp
    are an unresolved issue constraint on non-pole
    backgrounds requires experimental data.
  • Open door for larger kinematic reach in Fp
    measurement at 12 GeV
  • Increase knowledge of largely unknown po sL at
    large Q2 above resonance region
  • Easier planning for future Rosenbluth separation
    exp.
  • Requires 17 days of data at 5.75 GeV
  • An relatively easy experiment making use of
    existing Hall A standard equipment.
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