Muon Calibration Difficulties - PowerPoint PPT Presentation

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Muon Calibration Difficulties

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... Required Double Ended Hits. To ... New Tracker' Enabled Lifting Of Double Ended Hit Requirement. This Led To Inclusion Of More Corner Clipping Muons. ... – PowerPoint PPT presentation

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Title: Muon Calibration Difficulties


1
Muon Calibration Difficulties
  • Calibration Shortcomings
  • Angular Effects
  • Old Path Length Correction
  • New Correction
  • Other Matters
  • Results

Ryan Nichol and Chris Smith
2
Problems With Old Method
  • Old Calibration Required Double Ended Hits.
  • To Remove Crosstalk.
  • Beam Muons Show Even/Odd Asymmetry.

3
New Tracker Working Well
4
Corner Clippers
  • New Tracker Enabled Lifting Of Double Ended Hit
    Requirement.
  • This Led To Inclusion Of More Corner Clipping
    Muons.
  • Decided To Remove Corner Clipping Hits From
    Sample.

5
Angular Distribution
  • Large Angular Asymmetry at CalDet.
  • Due To Orientation of Planes.

6
Error On Determination Of Angle
  • Bands Correspond To Muon Track Length.
  • Accuracy Limited By Strip Resolution.

7
Angular Dependence of Pulse Height
  • Corner Clippers Removed.
  • Two Views Have Similar Dependence.
  • Strange Bimodal Shape.

8
Path Length Factors
  • Angular Dependence.
  • Finite Strip Width.
  • Affects Two Orientations Differently.
  • Minimum Path Length In Strip.
  • Path Length In Neighbouring Strips.
  • Transverse Position Across Strip Width.
  • Other Effects??

9
Geometrical Constraints
  • Path Length Constrained By
  • Finite Strip Width
  • Minimum PL in Strip.
  • Maximum PL in neighbouring strips.
  • These extrema are determined by light output.

10
Transverse Position Across Strip
  • Pulse Height Depends on Transverse Position
    Across Strip.

11
Old Path Length Correction
  • Tries To Account For
  • Angle
  • Finite Strip Width
  • Minimum Path Length
  • Doesnt Succeed.
  • Introduces Even/Odd Bias.

12
Simulation Results
  • Simulated Muons In CalDet With Measured Angular
    Distribution.
  • Calculated Path Length Differs From True Path
    Length.

13
New Path Length Correction
  • The Solution
  • 92
  • Only Accounts For Angles.
  • Corrects to 2 level.

14
Results
  • New Calibration Removes Some Of The Even Odd
    Asymmetry
  • Still not an ideal calibration.

15
Forwards-Backwards Asymmetry
  • Seemingly More Energy Deposited By Cosmics
    Traveling Backwards Through The Detector.
  • Steel-Scintillator-Air or Steel-Air-Scintillator?
  • Groove Position?
  • Needs Further MC Investigation.

16
More Front-Back Fun
17
Summary
  • Large Angular Asymmetry Between Views.
  • Due To Orientation Of Planes.
  • Complicated Pulse Height Dependence.
  • Old (Current) Path Length Correction Wrong.
  • Best Results From A Fudge Factor
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