Title: January PREx Test Run: Compton Photon Analysis
1January PREx Test RunCompton Photon Analysis
- Diana Parno
- Carnegie Mellon University
- HAPPEX Collaboration Meeting
2Outline
- Compton photon DAQ
- Integrating method
- FADC design
- Test run results
- Problem areas
3Photon 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
4FADC 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)
5FADC 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
6Test 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
7Outline
- Compton photon DAQ
- Results
- FADC functionality
- PMT performance
- Accumulator signals
- Asymmetries and polarization measurement
- Problem areas
8Studying 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
9Saturation
- 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
10Accumulator 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
11Sample Run Accumulator Signals
12Dilution 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
13Dilution Factors
- Computed dilution factors for four production runs
Run 60325
Run 60326
Run 60327
Run 60328
14Asymmetries!
Sign flip IHWP change
- 3 accumulators, 4 production runs
Sign flip Laser pol. change
15Accumulator Combinations
- Suppose we combine two accumulators to compute
asymmetries
Left circularly polarized laser
Laser off background only
16Sensitivity 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)
17Electron 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
18Outline
- Compton photon DAQ
- Results
- Problem areas
- Shape of energy spectrum
- Signal size
- Discrepancy between left/right polarization
states
19Problem 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)
20Signal 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
21Discrepancy 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
22Future 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