muon calibration difficulties

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Muon Calibration Difficulties Calibration Shortcomings Angular Dependence Old Path Length Correction New Correction Results

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Muon Calibration Difficulties. Calibration Shortcomings Angular Dependence Old Path Length Correction New Correction Results. Problems With Old Method. Old Calibration Required Double Ended Hits Beam Muons Show Even/Odd Asymmetry. Angular Distribution. Large Angular Asymmetry at CalDet. - PowerPoint PPT Presentation

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Page 1: Muon Calibration Difficulties

Muon Calibration DifficultiesCalibration ShortcomingsAngular DependenceOld Path Length CorrectionNew CorrectionResults

Page 2: Muon Calibration Difficulties

Ryan Nichol, Chris Smith

Problems With Old Method

• Old Calibration Required Double Ended Hits• Beam Muons Show Even/Odd Asymmetry

Page 3: Muon Calibration Difficulties

Ryan Nichol, Chris Smith

Angular Distribution

Large Angular Asymmetry at CalDet. Due To Orientation of Planes.

Page 4: Muon Calibration Difficulties

Ryan Nichol, Chris Smith

Angular Dependence of Pulse Height

Corner Clippers Removed.

Two Views Have Similar Dependence.

Strange Bimodal Shape.

Page 5: Muon Calibration Difficulties

Ryan Nichol, Chris Smith

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??

Page 6: Muon Calibration Difficulties

Ryan Nichol, Chris Smith

Old Path Length Correction

dzdy

dzdy

dzdsZdz

dsY

dzdy

dzdsYZ

ds2

. 22

Tries To Account For: Angle Finite Strip Width Minimum Path Length

Doesn’t Succeed. Introduces Even/Odd

Bias.

Page 7: Muon Calibration Difficulties

Ryan Nichol, Chris Smith

Simulation Results

Simulated Muons In CalDet With Measured Angular Distribution.

Calculated Path Length Differs From True Path Length.

Page 8: Muon Calibration Difficulties

Ryan Nichol, Chris Smith

New Path Length Correction

The ‘Solution’:92%

Only Accounts For Angles.

Corrects to 2% level.

1)1(92.0 dzdsds

Page 9: Muon Calibration Difficulties

Ryan Nichol, Chris Smith

Results

New Calibration Removes Some Of The Even Odd Asymmetry

•Still not an ideal calibration.

Page 10: Muon Calibration Difficulties

Ryan Nichol, Chris Smith

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’

Page 11: Muon Calibration Difficulties

Ryan Nichol, Chris Smith

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.

Page 12: Muon Calibration Difficulties

Ryan Nichol, Chris Smith

More Front-Back Fun

Page 13: Muon Calibration Difficulties

Ryan Nichol, Chris Smith

New Tracker Working Well

Page 14: Muon Calibration Difficulties

Ryan Nichol, Chris Smith

Transverse Position Across Strip

Pulse Height Depends on Transverse Position Across Strip.

Page 15: Muon Calibration Difficulties

Ryan Nichol, Chris Smith

Error On Determination Of Angle

Bands Correspond To Muon Track Length.

Accuracy Limited By Strip Resolution.

Page 16: Muon Calibration Difficulties

Ryan Nichol, Chris Smith

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.