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January PREx Test Run: Compton Photon Analysis

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Title: January PREx Test Run: Compton Photon Analysis


1
January PREx Test RunCompton Photon Analysis
  • Diana Parno
  • Carnegie Mellon University
  • HAPPEX Collaboration Meeting

2
Outline
  • Compton photon DAQ
  • Integrating method
  • FADC design
  • Test run results
  • Problem areas

3
Photon DAQ Integrating Method
  • 3 ways to measure a Compton-scattering asymmetry
  • Differential scattered photon count as a
    function of energy
  • Integrated scattered photon count without energy
    information
  • Energy-weighted total energy deposited (no
    photon counts)
  • New DAQ allows us to use energy-weighted method
  • At low energies, detector response function
    becomes complicated and thus harder to know with
    precision
  • Energy-weighted integrated method is less
    sensitive to the precision of the detector
    response function

4
FADC Design
  • As specified, the FADC (from Struck DE) samples
    the data at 200 or 250 MHz (programmable)
  • Six accumulators sum over a time interval (30
    ms).
  • Each signal sample contributes to at least two
    accumulators, depending on which criteria it
    meets.
  • Data can be read out in sampling mode (first
    50000 sample words are included along with
    accumulator words) or integrating mode
    (accumulator values only)

5
FADC Design Accumulators
  • Thresholds, and degree of stretching, are
    programmable
  • Ideally, Compton events fall within the window
    so we can compute asymmetries using
    Accumulators 0, 2, and 4

6
Test Run Goals DAQ
  • See Compton events with new FADC
  • Test signal splitting (to use original DAQ and
    new DAQ simultaneously)
  • Compute asymmetries and beam polarization using
    only energy-weighted integrated data
  • Study software, hardware behavior and systematics

7
Outline
  • Compton photon DAQ
  • Results
  • FADC functionality
  • PMT performance
  • Accumulator signals
  • Asymmetries and polarization measurement
  • Problem areas

8
Studying Pulses Two Modes
  • Integration mode Read accumulators only no
    deadtime
  • Several pulses in each 30-ms event
  • Sampling mode Read individual 5-ns samples.
    Detect peaks with a software threshold
  • Detailed study of individual pulses (e.g.
    snapshots)
  • Precise location of pedestal

9
Saturation
  • Plotting pulse area vs. pulse amplitude shows
    clear saturation during the test run
  • PMT (12-stage, -2500 V) major contributor
  • Compton events are in relatively linear region

10
Accumulator Physics Signals
  • The raw accumulator values can be used to extract
    the total physics signal
  • We can apply a deadtime correction to the physics
    signals from the window accumulators (2 and 4)

Number of samples
Average signal
Average pedestal value
11
Sample Run Accumulator Signals
12
Dilution Factors
  • S includes Compton signal C and background signal
    B
  • The measured asymmetry in S differs slightly from
    the asymmetry in C
  • We can correct for this by dividing the asymmetry
    in S by a dilution factor D

13
Dilution Factors
  • Computed dilution factors for four production runs

Run 60325
Run 60326
  • Small D means low SN

Run 60327
Run 60328
14
Asymmetries!
Sign flip IHWP change
  • 3 accumulators, 4 production runs

Sign flip Laser pol. change
15
Accumulator Combinations
  • Suppose we combine two accumulators to compute
    asymmetries

Left circularly polarized laser
Laser off background only
16
Sensitivity to Pedestal
  • A small mistake in finding the pedestal has a
    large effect on the computed asymmetries

Correct pedestal value (2017.2)
Incorrect pedestal value (2016)
17
Electron Beam Polarization
  • Megan Friends Geant simulation of analyzing
    power 0.02316 for test run
  • Still to be included PMT, PMT nonlinearity
  • We have everything we need to compute beam
    polarization

18
Outline
  • Compton photon DAQ
  • Results
  • Problem areas
  • Shape of energy spectrum
  • Signal size
  • Discrepancy between left/right polarization
    states

19
Problem Shape of Energy Spectrum
  • Compton cross section s(?) is a parabola. In the
    past, this shape has been echoed in the detected
    photon energy spectrum.
  • In January, the measured energy spectrum did not
    look remotely like a parabola. Why not?

January test run (central Saclay crystal)
20
Signal Size Mystery
  • During the test run, signal from the new detector
    seemed smaller than expected
  • Afterward, cosmic ray measurements at CMU (same
    detector) showed a much bigger response

Photon source Approx. deposited energy Pulse area response Pulse amplitude response
Compton 130.9 MeV 44 RAU-S/MeV 7.3 RAU/MeV
Cosmics 20.4 MeV 138 RAU-S/MeV 39 RAU/MeV
21
Discrepancy Left and Right
  • Large discrepancy between asymmetries (and thus
    polarizations) measured when laser
    left-circularly polarized vs. right-circularly
    polarized
  • Always in the same direction even when IHWP
    flips electron beam helicity

22
Future Work
  • With GEANT, investigate energy spectrum shape
  • Incorporate PMT into analyzing power model
  • Investigate L/R discrepancy
  • Improve analysis code incorporate coincidence
    data
  • Improve detectors and mounts in beamline

23
  • Thank you!
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