h4sim, a geant4 simulation program for the cms...

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3-10 November 2005 Geant4 10th international conference 1 H4sim, a Geant4 simulation program for the CMS ECAL supermodule Laboratoire Leprince-Ringuet, École polytechnique, IN2P3-CNRS, Palaiseau, France [email protected] Philippe Miné, on behalf of the CMS collaboration

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3-10 November 2005 Geant4 10th international conference

1

H4sim, a Geant4 simulation programfor the CMS ECAL supermodule

Laboratoire Leprince-Ringuet, École polytechnique, IN2P3-CNRS, Palaiseau, [email protected]

Philippe Miné, on behalf of the CMS collaboration

3-10 November 2005 Geant4 10th international conference

2

The CMS electromagnetic calorimeter

Geant4 implementation

Comparison with test beam data : electrons

Comparison with test beam data : pions

Precalibration with cosmic muons

Outline

3-10 November 2005 Geant4 10th international conference

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The CMS electromagnetic calorimeter

Compact Muon Solenoid at CERN LHC (2007)7+7 TeV p-p, heavy ions

ECAL : 75848 leadtungstate crystals

22×23×230 mm3

Density = 8.28 g/cm3

X0 = 0.89 cmRM = 2.10 cm

Fast < 15 nsRadiation hard20 interactions/25 ns

3-10 November 2005 Geant4 10th international conference

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The CMS electromagnetic calorimeter

Non-pointing geometry 3° in η(beam axis) and in ϕ

Barrel 36 supermodules,2 end-caps

120 GeV e-

η

ϕ

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The CMS electromagnetic calorimeter

Beam

Readout Electronics: 2 avalanche photodiodes + MGPA (multi gain pre-

amplifier) 3 gains (12,6,1), 10 samples

trigger

Scintillating

fibers

Movable table:

Used to reproduce for the impinging

particle the same almost pointing

geometry of CMS

Supermodule

4 photoelectrons / MeV 35.6 MeV / ADC count

3-10 November 2005 Geant4 10th international conference

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The CMS electromagnetic calorimeter

Test in the H4 beam at CERN SPS since 1997 : electrons 20 to 250 GeV, pions, muons, laser light

Energy and position resolution, containment, cracks, irradiation recovery

Precalibration with electrons in the H4 beam : 2004 - 2006

Precalibration with cosmic muons : 2004 - 2006

In situ monitoring with laser

In situ calibration with electrons from Z, W, …

3-10 November 2005 Geant4 10th international conference

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Geant4 implementation

CMS has a Geant4 simulation program, OSCAR, for the complete detector, interfaced with the reconstruction

H4sim is a standalone simulation of one supermodule in H4

Geometry description by Geant4 data cards with a text fileDDD (Detector Description Database) in XML format

Aluminiumframe

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Geant4 implementation

No magnetic field (time consuming tracking)No matter behind the crystalsCan add specific H4 devices, e.g. hodoscopesOutput of the crystal energies in a ROOT file, interface toRRF (Raw Root File) to simulate beam data

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.XML files

.txt or .root

files

.mac files

Geant4 implementation

XML readout

Output

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Geant4 implementation

Production cuts :

1mm for e-,e+ and γcorrespond to :~ 1.15 MeV for electrons in PbWO4

~ 0.59 MeV in Al

Version 6.2. p 02

Execution time : 1.4 s for 50 GeV on 2 GHz

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Geant4 implementation

- Interactiveversiongraphical interface & visualization - Batch version

Special H4sim commands

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Geant4 implementation

Centre of crystal face Centre of crystal 120 GeV calibration

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Geant4 implementation

100 GeV → π 500 GeV µ-

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TEST BEAM

E25 = 97,5 %

E9 = 94,5 %

E1 = 78,9 %

MONTE CARLO

E25 = 97,5 %

E9 = 94,6 %

E1 = 78,9 %

Electron beam dataElectron beam data

3-10 November 2005 Geant4 10th international conference

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y (mm)-10 -5 0 5 10

E1

0.5

0.6

0.7

0.8

0.9

1

1.1

E1 vs Y (hodoscopes) normalized

testbeam

simulation

x (mm)-10 -5 0 5 10

E1

0.5

0.6

0.7

0.8

0.9

1

1.1

E1 vs X (hodoscopes) normalizedtestbeam

simulation

y (mm)-10 -5 0 5 10

E1

0.5

0.6

0.7

0.8

0.9

1

1.1

E1 vs Y (hodoscopes) normalized

testbeam

simulation

x (mm)-10 -5 0 5 10

E1

0.5

0.6

0.7

0.8

0.9

1

1.1

E1 vs X (hodoscopes) normalizedtestbeam

simulation

Test beam

Simulation

X (mm) Y (mm)

Position scan at centre of crystal 204

Electron beam data

Y goodX ~ 2 %

3-10 November 2005 Geant4 10th international conference

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Phi EtaData

Simulation

log(E2/E1)-3 -2 -1 0 1 2 3

SU

M 9

0.96

0.965

0.97

0.975

0.98

0.985

0.99

0.995

1

1.005

1.01

Test-Beam

Monte-Carlo

comparaison Test-Beam / Monte-Carlo @120 GeV Xtal 1104ηS9 vs log(E1/E2)

log(E2/E1)-3 -2 -1 0 1 2 3

SU

M 9

0.96

0.965

0.97

0.975

0.98

0.985

0.99

0.995

1

1.005

1.01

Test-Beam

Monte-Carlo

comparaison Test-Beam / Monte-Carlo @120 GeV Xtal 1104φS9 vs log(E1/E2)

Electron beam data

3x3 crystals impact position measured by log(E2/E1) function

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Electron beam data

3X3 5X5

S = stochastic

N = noise

C = constant

2

222

CE

N

E

S

E+

+

=

σ

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Electron beam data

ECAL used in trigger

Simulation of the TPG linearity (Trigger Primitive Generator)

Data (green)Simulation (black)

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Pion beam data

GeV

# Entries5x5 energy

for 50, 120 &

180 GeV

pions

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Pion beam data

Compare the mean valuesµ ± σof Landau-fit for 4 crystals@ 3 energies

for 4 crystals @ 3 energies

204 704 1104 1404

204 1104 1404

204 704 1104 1404

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Pion beam data

Minimum ionizing particle (mip) are visible

50 GeV

λ ~ 23 cm

E = 270 MeVGeV

# E

ntr

ies

Pedestal

mip

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Less good agreement for crystals 1104 & 1404

Pion beam data

Almost constant, as it should be for mips

3 energies for 4 crystals

204 704 1104 1404

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Precalibration by cosmic muons

Raise the APD gain by a factor 4

Select the muons parallel to the crystal axisVeto neightbouring crystals

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MC

Precalibration by cosmic muons

data

Module 1

Event selection: E1 > 10 ADC counts & E2 < 3 ADC counts

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More difficult for module 4 (eta angle)⇒ incline the supermodule by10 degrees

Precalibration by cosmic muons

Intercalibration precision of 2-3% can be reached with 1 week of continuous cosmic ray data taking

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Peak after final selection:

good agreement between data (after calibration) and MC

Precalibration by cosmic muons

Data: <evts/xtal/day> = 55±2 MC: <evts/xtal/day> = 61±2

Disagreement ~ 10% due to trigger inefficiency and uncertainty on the overall normalization

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Conclusion

Geant4 based H4sim is widely used by the ECAL CMS communityInterpretation of test beam dataTest of algorithms and cosmic precalibration

Acknowledgments to :T. Frisson, J. Gilly, P. Mora de Freitas, S. Bimbot, P. Paganini, P. Meridiani, R. Salerno, P. Jarry, J. Descamps, A. Ghezzi, S. Vigano, C. Marchica, A. Holzner, P. Bloch, A.Zabi and the ECAL group