timing calibration efforts in cosmic ray veto for mu2e
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Timing Calibration Efforts in Cosmic Ray Veto for Mu2e Experiment Payton Beeler Standard Model Charged lepton flavor violation Why is it important? Breaks standard model How its supposed to work How it actually works (maybe)


  1. Timing Calibration Efforts in Cosmic Ray Veto for Mu2e Experiment Payton Beeler

  2. Standard Model • Charged lepton flavor violation • Why is it important? • Breaks standard model

  3. How it’s supposed to work

  4. How it actually works (maybe) ฀฀ ฀฀ e - Why is this important? Means that the standard model needs some work.

  5. Mu2e • Run by Department of Energy • Located in Batavia, Illinois Detector • Will hopefully have results by 2020

  6. Resolution Problems • Extremely rare decay Events Energy

  7. PROBLEM: it’s raining apples

  8. Solution: Cosmic Ray Veto (CRV)

  9. Layout

  10. Counters • 1,632 on CRV-T • 4 fibers run through each • Fibers connect to SiPMs 5600 mm 15 mm 20 mm 20 mm 50 mm

  11. Noise Problems 3 1 t 3 t 1 t 4 4 t 2 2

  12. Oscilloscope Readout (ideal world) 1 t 1 2 t 2 3 t 3 4 t 4

  13. Oscilloscope Readout (real world) Timing error ≈ ±300 ps

  14. Method • Shoot cosmic ray at specific point in counter • Find theoretical time it takes to get to detector • Introduce error to theoretical time to simulate measured time • Try to get original position from simulated time using chi squared test

  15. Method

  16. Results Average Difference vs. Position 0.004 0.002 0 0 1 2 3 4 5 6 -0.002 Difference (m) -0.004 y=0.025 m y=0.015 m y=0.050 m -0.006 -0.008 -0.01 -0.012 -0.014 Position (m)

  17. Results RMS vs Position 0.009 0.008 0.007 0.006 Root Mean Squared 0.005 0.004 0.003 0.002 0.001 0 0 1 2 3 4 5 6 Position (m)

  18. Next Problem • Attenuation • Amplitudes

  19. Scenario • When a cosmic ray hits the polystyrene 25 photoelectrons come out Number of Photoelectrons vs. Position Number of PE to Counters 1 and 2 Number of PE to Counters 3 and 4 30 25 20 Number of Photoelectrons 15 10 5 0 0 1 2 3 4 5 6 Position (m)

  20. Oscilloscope Readout 1 t 1 t 1 2 t 2 t 2 t 3 3 t 3 t 4 4 t 4

  21. Results Difference vs Position 0.02 0.015 0.01 0.005 Differnece 0 0 1 2 3 4 5 6 -0.005 -0.01 -0.015 -0.02 Position

  22. Results RMS vs Position 0.0035 0.003 0.0025 0.002 RMS 0.0015 0.001 0.0005 0 0 1 2 3 4 5 6 Position (m)

  23. Results Difference vs Position 0.035 0.03 0.025 0.02 Difference (m) 0.015 0.01 0.005 0 0 1 2 3 4 5 6 -0.005 -0.01 Position (m)

  24. Acknowledgements • Big thanks to Glenn Horton-Smith and Tim Bolton for allowing me to work with them this Summer • Thank you to the NSF for funding

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