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Highlights from the 9 th Pisa Meeting on Advanced Detectors Calorimetry Session Riccardo Paramatti University of Rome La Sapienza and INFN Rome Detector Seminar CERN 18/07/2003

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Page 1: Highlights from the 9 Pisa Meeting on Advanced Detectors · Highlights from the 9th Pisa Meeting on Advanced Detectors ... Ł Continuos beam @ PSI (108 µ/s) ... The emission reaction

Highlights from the 9th Pisa Meeting on Advanced Detectors

Calorimetry Session

Riccardo ParamattiUniversity of Rome �La Sapienza� and INFN Rome

Detector Seminar � CERN18/07/2003

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9th Pisa Meeting

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9th Pisa Meeting: the program

Tracking Sessions: talk by Silvia Schuh (4th july)

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9th Pisa Meeting:calorimetry session

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Liquid-Xenon photon detector for µ-> eγPhysics motivations: in the Standard Model this decay is forbidden;in the SM + Neutrino Oscillation this decay is strongly suppressed;in SUSY framework the Branching Ratio could be just below the currentlimit by MEGA (BR ≈ 10-11). MEG sensitivity down to 10-14

� Continuos beam @ PSI (108 µ/s) on a stopping target� Positron and photon back-to-back and in time� Photon detected by Liquid Xe Photon Detector� Positron detected by the Solenoidal Magnetic Spectrometer with a gradedmagnetic field

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Liquid-Xenon photon detector for µ-> eγ (2)

Signal: a positron and a photon back-to-back with E = 52.8 MeVBackground:� Radiative µ+ decay (if neutrinos carry small amount of energy) � Positron from usual decay with E = mµ/2 and photon fromradiative muon decay or from annihilation in flight of positron(not in time)

Requirements: fast response, good energy, position and time resolution -> Liquid Xenon

Absorption of scintillation lightThe emission reaction can�t happen in the reverse way; only impurity (water, oxygen) could absorb the light.Absorption length increased, 7cm -> >1 m by Xenon purification.

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Liquid-Xenon photon detector for µ-> eγ (3)

Small prototype:� 32 PMT surrounding 2.34 litres of active volume� without purification system� gamma-rays sources of differentelements� α source for PMT calibration

Energy (MeV)

Energy, position and time resolution measurements in agreement with Montecarlosimulation.Results published in 2002.

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Liquid-Xenon photon detector for µ-> eγ (4)

Large prototype:� 228 PMT surrounding 68.6 liters of active volume (120 liters of liquid xenon in total)� development and test of purification system for Xenon� PMT long term operation at low temp.� gamma beam test up to 40 MeV� 60 MeV electron beam� absorption length measurement

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GLAST Calorimeter� High energy gamma rays: 20 MeV � 300 GeV� GLAST will be launched in september 2006� The CDE have to operate in space at ≈ -10 0C� 2 of 4 long side depolished to increase the tapering

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GLAST Calorimeter (2)� 14 CDE have been assembled and tested with cosmic muons� The CsI LY decrease with temperature: test -20 0C -> 30 0C

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ATLAS Electromagnetic Calorimeter

The ATLAS calorimeter is built in 8 construction sites:Annecy, Saclay, CERN, Grenoble, Stockholm (barrel) and Marseille, Madrid, Novosibirsk (endcap)

� Lead - liquid Argon sampling calorimeter

� Accordion geometry� 2 half-barrels: |η| < 1.475� 2 endcaps: 1.375 < |η| < 3.2� Outside the solenoid

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ATLAS Electromagnetic Calorimeter (2)Longitudinal segmentation will provide good particle ID.

uniform

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CMS Electromagnetic Calorimeter

ECAL

� Crystal calorimeter� ≈ 75000 lead tungstate PbW04

crystals � Magnetic field: B = 4 T� Endcap preshower: 1.65 < |η| < 2.6

Two barrelRegional Centers: CERN (lab 27) and INFN/ENEA -Rome

Endcapconstruction:UK, CERN

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CMS Electromagnetic Calorimeter (2)

� Fast scintillation� Small Xo and Rm� Intrinsic radiation hardness� Relatively easy to grow� Massive production capability

� Low Light Yield� High index of refraction� Strong LY dependance on T

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ATLAS: construction status

Module assembly� Geometrical measurements� Gap thickness measurements� Electrical test during assembly

- HV performance (2200 V)� Module cabling� Tests in final configuration

Electromagnetic shower simulation Electrode composition

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ATLAS: construction status (2)

η = 0 η = 1.5

η = 1.4 η = 3.2

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ATLAS: construction status (3)

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ATLAS: construction status (4)

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CMS: construction status

2 in one!

Further increase of the PbWO ingot diameter is foreseen: 2Endcap or 4Barrel

crystals in one ingot are in test phaseBARREL ingot

� Crystal R&D phase (1995-1998)� 6000 crystal preproduction (1998-2000)� Crystal production (2001-> ); 2-in-one crystal production is starting now

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CMS: construction status (2)CERN (lab 27) and INFN/ENEA (Casaccia) Regional Centers:� Automatic measurements of:

crystal dimensions, trasmission, light yield and uniformity� Submodule assembly (10 crystals)� Module assembly (40-50 submodules)

Module type 2 - Rome

Module type 4 - Cern

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CMS: construction status (3)

Modules from Rome RCSupermodule assembly at CERN

Modules production

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cEb

Ea

E⊕⊕=σ

Energy Resolution

The discovery potential of an intermediate mass Higgs boson via the two photon decay channel depends on the energy resolution.

� a: stochastic term from Poisson-like fluctuations� sampling contribution

(natural advantage of omogeneous calorimeters)� b: noise term from electronic and pile-up

� relevant at low energy� c: constant term

� dangerous limitation to high energy resolution� important contribution from intercalibration constants

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the stochastic term

Total stochastic terma = 2.7 %

� photostatistics contibution:- light yield- light collection efficiency- geometrical efficiency of

the photodetector- photocatode quantum

efficiency

� electron current multiplication in APD

� lateral containment of the shower

CMS ATLAS

Total stochastic term:a ≈ 10 %

� pure sampling fluctuations� deterioration for increasing η:

- increase of amount of material- decrease of sampling frequency

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CMS: the constant term

� leakage (front, rear, dead material)CMS full shower simulation < 0.2 %

� temperature stabilization < 0.1 ûC(dLY/dT = -2.0%/ûC @ 18ûC ; dM/dT ~ -2.3 %/ûC)

� APD bias stabilization (±20 mV / 400 V)(dM/dV = 3%/V)

� light collection uniformity (next slide)� intercalibration by monitor and physics signals

Total constant term c = 0.5 %

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CMS: the constant term (2)� A non uniformity of the light collection in the shower max region maysignificantly contribute to the constant term in the energy resolution.� Uniformity can be controlled by depolishing one lateral face with a given roughness

FNUF

Ideal light collection shape

(crystals all polished)

Lab measurementCfnuf < 0.3%

Max Front d(LY)/dX0=±0.35%/X0

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ATLAS: the constant term

Local constant term c = 0.5 %over a small area (∆η x ∆φ = 0.2 x 0.4 -> 128 cells in the

middle sector) with independent cell to cell electronics calibration

Global constant term c = 0.7 %in situ-calibration with Z → e+ e- decays to correct

long-range non-uniformity

� Absorber and gap thickness� Ionization signal dependence with temperature

(argon density vs T = -0.45 %/ûCdrift velocity vs T = -1.55 %/ûC)

� High Voltage stabilization� Leakage, material in front of calorimeter

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Performance: H -> γγ

10000

12500

15000

17500

20000

105 120 135

mγγ (GeV)

Eve

nts

/ 2 G

eV

0

500

1000

1500

105 120 135

mγγ (GeV)

Sig

nal-

back

grou

nd, e

vent

s / 2

GeV

ATLAS - 100 fb-

CMS - 100 fb-1

MH=120 GeV

MH=130 GeV

S/√√√√B ≈≈≈≈ 6.5->4.3 with MH = 120->150 GeV

S/√√√√B ≈≈≈≈ 13->8 with MH = 120->150 GeV

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ATLAS: Test beam

For every tested point: stochastic term

a < 10 % (barrel)a < 12,5% (endcap)

� 1999-2000: barrel and endcap full-size prototype� 2001-2002: 7 (4 barrel and 3 endcap) production modules� 2002: combined endcap runwith hadronic

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ATLAS: Test beam (2)barrel

σσσσ/E=0.49%

endcap

Global non-uniformity ≈ 0.6%for whole module

Global non-uniformity ≈ 0.5%for whole module

Global constant term ≈ 0.7% within specifications

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ATLAS: Future test beam

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CMS: Precalibration� Only few Supermodules will be calibrated at the Cern

Test Beam facilities (intercalibration ≈ 2%)� All crystals are intercalibrated in the lab. module

assembly phase by Light Yield measurements (≈ 4%)

LY meas. of reference crystals in INFN/ENEA Regional Center

(with PMT and tyvek wrapping at 18 0C)

σ σ σ σ = 3-4%

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CMS: Test Beam 2002

σ σ σ σ = 4.7%

Intercalibration: lab.

measurementsvs test beam

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CMS: Laser Monitoring

EB

[Gy]

EE

[cm

]

Total dose after 10 years of running (5x105 pb-1)

→ Only e.m. radiation produces a damage→ Scintillation mechanism is not affected → Only crystal transparency is reduced

creation of color centers→ Damage level depends on dose rate

creation and annealing of color centers at room temperature

→ Damage level reaches an equilibrium after a small administered dose

→ Partial damage recovery in few hours→ Loss in extracted light of few % is

tolerable and can be followed with a monitor system

Dose rates [Gy/h] in ECAL at luminosity L=1034cm-2s-1

EB

EE 0.15

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CMS: Test Beam 2002 (2)

αααα σσσσ/µµµµ = 6.1%

αααα

αααα

αααα

� The relation between XL response to e (S/S0) and response to laser (R/R0) varies in the same way during recovery and irradiation phases.

� Crystals irradiated 2-3 times produce same slope α

� Light monitoring system operational and stable

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�Collisions� Dose 2.5 Gy in 8 h

�Filling�

Time scale for absolutecalibration with Z events

High luminosity simulation at η=0, based on data taken in test beam

� laser OK for correction of electron response

� 2003 test beam withother modules (differentpseudorapidity) and more statistics

CMS: Laser Monitoring (2)

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CMS: In situ calibration

� At the beginning of detector operation -> fast intercalibration method based on the φ symmetry in minimum bias events.

� Energetic electrons from Z → e+ e- decay -> intercalibration of different regions and absolute energy scale setting.

� Once the Tracker fully functional -> intercalibration of individual crystals with E/p measurement (W → eν events).

TRACKER MATERIAL:the amount of material (~ 1 X0) between interaction point and ECAL is the main difficulty in performing calibration.

In-situ calibration with physics events: this is the main tool to reduce the constant term to the design goal of 0.5%.

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CMS: In situ calibration (2)

Aim: reduce the number of intercalibration constants at the startup: from 61200 (crystals) to 170 (rings) in the barrel.

Assumption: the total transverse energy deposited from a large number of events should be the same for all crystals at fixed η

φφφφ symmetry

Studies with fully simulated Montecarlo give a precision of 1.3% -3.5%, in case of limited knowledge of φ inhomogeneity.

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CMS: In situ calibration (3)Z →→→→ e+ e-

� The rings can rapidly be intercalibrated using Z→e+e-

without tracker momentum measurements, using reconstruction of the invariant mass� A large fraction of events allows to intercalibrate the endcaps with respect to the barrel� The Z→e+e- rate is ~ 1 Hz (almost flat in η)

� The electron shower involves many crystals -> algorithm to unscramble individually the calibration constants.� The W→ eν rate is ~ 10 Hz.

W →→→→ e νννν

In few weeks at 2*1033 cm-2 s�1, exploiting the full tracker information, this high statistics channel will allow to reach 0.5% resolution

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ATLAS: In-situ calibration

constant

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ATLAS

(not only) Tracker Material� Complex tracking system + frames + cooling + cables and services� Some radiation lenghts between the interaction point and the electromagnetic calorimeter !� Bremsstrahlung and photon conversion (big non-gaussian tails in physical distributions)

CMS

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Bremsstrahlung

e

γ

The electron cluster is spread byBremsstrahlung (mainly in φ)� Too little recostructed cluster: not full containment of brem. photons� Too big recostructed cluster: noise, pile-up

CMS Energyrecovery:SuperCluster = clustering withdynamic algos.

ATLAS Energy recovery: cluster with fixed and optimized dimension.

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ATLAS: electron reconstruction

η η

φ

φ

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CMS: electron reconstruction

single electrons,single electrons,pptt> 28 > 28 GeVGeV

only singleonly singleclustersclusters

supersuper--clustersclusters

� Hybrid Algorithm:� Used in the barrel

� Island Algorithm:� Used in the endcaps

To be compared with intrinsic calorimeter resolution < 0.9%

SUPERCLUSTERs

Electronic noiseNo Pile-Up

Electronic noiseNo Pile-Up

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ATLAS: position resolution

η

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☺ A brief ECAL comparison ☺

"☺Endcaps construction status

☺"Energy resolution: stocastic term

##Energy resolution: constant term

#☺Barrel construction statusCMSATLAS

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☺ A brief ECAL comparison (2) ☺

#☺γ/πo separation

☺#Electron reconstruction

" "" "Tracker material, (bremsstrahlung and photon conv.)

☺#Intercalibration in situ withphysics events

CMSATLAS