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Cosmic Rays Data Analysis with CMS-ECAL Mattia Fumagalli (Università di Milano Bicocca) CIAO!

Cosmic Rays Data Analysis with CMS-ECAL Mattia Fumagalli (Università di Milano Bicocca) CIAO!

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Page 1: Cosmic Rays Data Analysis with CMS-ECAL Mattia Fumagalli (Università di Milano Bicocca) CIAO!

Cosmic Rays Data Analysiswith CMS-ECAL

Mattia Fumagalli

(Università di Milano Bicocca)

CIAO!

Page 2: Cosmic Rays Data Analysis with CMS-ECAL Mattia Fumagalli (Università di Milano Bicocca) CIAO!

Mattia Fumagalli - Summer Student Session 2008 2

Brief Review of CMS-ECAL.

BARRELL:36 supermodules

ENDCAPS: 2 dees each

ECAL BARREL:

61200 PbWO4 scintillating

crystals equipped with APD

Crystals point to the

Interaction Vertex

Page 3: Cosmic Rays Data Analysis with CMS-ECAL Mattia Fumagalli (Università di Milano Bicocca) CIAO!

Mattia Fumagalli - Summer Student Session 2008 3

CMS-ECAL Calibration Strategy

• PRECALIBRATION:

• 120 GeV electron TEST BEAM (2006): 1/4 of the ECAL barrel. 0.3% in reproducibility

• Cosmic Muons at Point H4: precision 1.3% to 2% depending of η.

To have…

•FINAL CALIBRATION! PHYSICS EVENTS @ LHC:

• Phi-Symmetry and Calibration with Pions

• Z ee and W e processes: intercalibration of different regions

•absolute Energy scale setting.

2.7% 1500.5%

MeV

E EE

we need

Page 4: Cosmic Rays Data Analysis with CMS-ECAL Mattia Fumagalli (Università di Milano Bicocca) CIAO!

Mattia Fumagalli - Summer Student Session 2008 4

In Situ Calibration with CosmicsCRUZET RUNS: no magnetic fieldalmost every part of CMS working ~70M events taken in 3 sessions

(5-7 days each) (4th CRUZET coming!)

INTERCALIBRATION:Independent check of the previous Calibrationswith the detector alreadyIn-Situ!

TrackerECALHCALMuons Drift Tubes

Page 5: Cosmic Rays Data Analysis with CMS-ECAL Mattia Fumagalli (Università di Milano Bicocca) CIAO!

Mattia Fumagalli - Summer Student Session 2008 5

Muon Events at ECAL

BEST EVENTS !Cluster made of just one Crystal

(GOLDEN MUONS)

SEED CRYSTAL

Cosmic Muons are Minimum Ionizing Particles_ No Electromagnetic Shower_ Energy deposited just in the hit Crystals_ Energy proportional to Path Lenght

Page 6: Cosmic Rays Data Analysis with CMS-ECAL Mattia Fumagalli (Università di Milano Bicocca) CIAO!

Mattia Fumagalli - Summer Student Session 2008 6

• Two Cluster Events

• Delta between clusters > 90°

• Impact Parameter < 10 cm

• Cosmic Muons that point to the Interaction Vertex

• Muon Path almost parallel to the Crystal Axis

InteractionVertex

Impact Parameter

NOT IN SCALE!

Selecting the Events

Page 7: Cosmic Rays Data Analysis with CMS-ECAL Mattia Fumagalli (Università di Milano Bicocca) CIAO!

Mattia Fumagalli - Summer Student Session 2008 7

Energy and PathsGOAL! Cross Check of the ECAL Pre-Calibration

According to the Behaviour of a MIP

Peak at 0.012 GeV/cm

Comparison between the Energy deposited and the Path Length

(Inter)Calibrationcoefficients

i i iCLUSTER CLUSTER

dEL E c AdX

Inverse Matrix Tecnique

ECAL

Page 8: Cosmic Rays Data Analysis with CMS-ECAL Mattia Fumagalli (Università di Milano Bicocca) CIAO!

Mattia Fumagalli - Summer Student Session 2008 8

OccupancyStatistics on each Crystals

Energy Distribution on the ECAL

SHAFT

Page 9: Cosmic Rays Data Analysis with CMS-ECAL Mattia Fumagalli (Università di Milano Bicocca) CIAO!

Mattia Fumagalli - Summer Student Session 2008 9

What’s good… and what’s bad!

Low Statistics, depending on eta.Calibration not possilbe everywhere

Data from other parts of CMSPossibility of Track Reconstruction

Page 10: Cosmic Rays Data Analysis with CMS-ECAL Mattia Fumagalli (Università di Milano Bicocca) CIAO!

Mattia Fumagalli - Summer Student Session 2008 10

Future Work• Fully Exploit the Statistics

• Implementation of a Calibration Algorithm

• Coefficients to cross check previous Calibrations

…and Thanks!GRAZIE!