the cms construction

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The CMS Construction

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The CMS Construction. (CMS) Design Criteria. Very good muon identification and momentum measurement Trigger efficiently and measure sign of TeV muons dp/p < 10% High energy resolution electromagnetic calorimetry ~ 0.5% @ E T ~ 50 GeV Powerful inner tracking systems - PowerPoint PPT Presentation

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Page 1: The CMS Construction

The CMS Construction

Page 2: The CMS Construction

(CMS) Design Criteria

Very good muon identification and momentum measurementTrigger efficiently and measure sign of TeV muons dp/p < 10%

High energy resolution electromagnetic calorimetry~ 0.5% @ ET ~ 50 GeV

Powerful inner tracking systemsMomentum resolution a factor 10 better than at LEP

Hermetic calorimetryGood missing ET resolution

(Affordable detector)

Transparency from the early 90’s

Page 3: The CMS Construction

Experimental Challenge

High Interaction Rate

pp interaction rate 1 billion interactions/sData can be recorded for only ~102 out of 40 million crossings/secLevel-1 trigger decision takes ~2-3 s electronics need to store data locally (pipelining)

Large Particle Multiplicity

~ <20> superposed events in each crossing~ 1000 tracks stream into the detector every 25 nsneed highly granular detectors with good time resolution for low occupancy

large number of channels (~ 100 M ch)

High Radiation Levels radiation hard (tolerant) detectors and electronics

LHC Detectors (especially ATLAS, CMS) are radically different from the ones from the previous generations

Page 4: The CMS Construction

The CMS Detector

Page 5: The CMS Construction

The CMS Collaboration (2007)

2310 Scientific Authors 38 Countries 175 Institutions

CERN

France

Italy

UK

Switzerland

USA

Austria

Finland

GreeceHungary

Belgium

Poland

Portugal

SpainPakistan

Georgia

Armenia

Ukraine

Uzbekistan

CyprusCroatia

China, PR

Turkey

Belarus

EstoniaIndia

Germany

Korea

Russia

Bulgaria

China (Taiwan)

Iran

Serbia

New-Zealand

Brazil

Ireland

1084

503

723

2310

Member States

Non-Member States

Total

USA

# Scientific Authors

59

49

175

Member States

Total

USA

67Non-Member States

Number ofLaboratories

Associated Institutes

Number of ScientistsNumber of Laboratories

629

Oct. 3rd 2007/gm

Mexico ColombiaLithuania

Page 6: The CMS Construction

Exploded View of CMS

Minus SidePlus Side

Page 7: The CMS Construction

Assembly of Iron Yoke

2003

Page 8: The CMS Construction

Assembly of the Coil

Page 9: The CMS Construction

Assembly of the Coil

Coil: 230 tonsOuter vacuum tank: 13 m long SS tube, =7.6 m

Sept 05Sept 05

Page 10: The CMS Construction

Surface Hall: Barrel Muons

Page 11: The CMS Construction

Lowering of Heavy Elements

YE+1 (Jan’07)

Page 12: The CMS Construction

Lowering of Heavy Elements

Feb 2007

Page 13: The CMS Construction

Insertion of Barrel ECAL

Jul’07

Page 14: The CMS Construction

Completion of Services on YB0

Nov. ‘07

Page 15: The CMS Construction

Lowering of Tracker

Dic. ‘07

Page 16: The CMS Construction

Tracker Insertion

Dic. ‘07

Page 17: The CMS Construction

Tracker in CMS

Dic. ‘07

Page 18: The CMS Construction

Extreme engineering: 4T, big dimensions & large magnetic deformation

0.0

2.0

4.0

6.0

8.0

10.0

12.0

10 100 1000 10000

E/M

(kJ

/kg)

Stored Energy (MJ)

CMSSDC-model

ATLAS -sol.

ALEPH

DELPHI

H1CDF

VENUS

ZEUS

TOPAZCLEO2

ATLAS Barrel

ATLAS End-caps

The CMS SC Solenoid

Solenoid composed by 5 modules

(CB-2, CB-1, CB0, CB+1, CB+2)

5 modules 6900 mm ; L 2500 mm ; W= 50 t

I = 20kA

Design Goal: Measure 1 TeV/c muons with < 10% resolution

Page 19: The CMS Construction

Winding of the Coil

Specific winding technology developed by INFN Genova in collaboration with Ansaldo Superconduttori

Winding

Page 20: The CMS Construction

Test of the Magnet (2006)

24 July28 August

19 kA, 4 Tesla!

2 days stable operation at 3.8 T

Magnet Current Cycles achieved during August

Page 21: The CMS Construction

Tracking at LHC

Fluence over 10 years of

LHC Operation

Need factor 10 better momentum resolution than at LEP1000 particles emerging every crossing (25ns)

Page 22: The CMS Construction

Layout of CMS Tracking

Si pixels surrounded by silicon strip detectors

Pixels: ~ 1 m2 of silicon sensors, 65 M pixels, 100x150 m2 , r = 4, 7, 11 cmSi strips : 223 m2 of silicon sensors, 10 M strips, 10 pts, r = 20 – 120 cm

120 cm

TOB

TIDTIB

TEC

Pix300 cm

CMS

Page 23: The CMS Construction

The CMS Tracker

Pixel Silicon Strip Tracker

Largest Silicon Strip Detector ever built:

~200m2 of silicon,

instrumented volume ~24m3

TIB (4 layers ) TID (3 disks, 3 rings ) TOB (6 layers) TEC (9 disks, 7 rings )

Page 24: The CMS Construction

Si Modules and Electronics Chain

Si Sensors

75k chips using 0.25m technology

Ride on technology wave

Page 25: The CMS Construction

System Components

Module Sensor + FE Hybrid

chip: APV25 (128 strips) - analog Optical converter (AOH)

one laser/fiber = 256 strips Controls/Clock/Trigger

Control chip (CCU) I2C protocol with modules rings of CCUs

Digital optical converted (DOH) optical link to VME controller (FEC)

Controls

Hybrid+AOH

String

Page 26: The CMS Construction

System Components

DOM (Firenze)DOM (Firenze)

Mother cable (Bari)Mother cable (Bari)

CCUM (Cern)CCUM (Cern)

AOH (Perugia)AOH (Perugia)Modules (all)Modules (all)

Page 27: The CMS Construction

The Start of the TIB Integration

The first string

Apr. ‘05

Page 28: The CMS Construction

Si Tracker

TIB TEC

Page 29: The CMS Construction

Si Tracker

Page 30: The CMS Construction

Si Tracker

Page 31: The CMS Construction

Tracker Readied for Installation

Dead channels ~ 0.5 ‰ stable in timeNoisy channels ~ 0.5 % stable in time

Page 32: The CMS Construction

Lead Tungstate ECAL Design Goal: Measure the energies of photons from a decay of

the Higgs boson to precision of ≤ 0.5%CMS chose scintillating crystals

1972

1985

1989

1986

1990

1999

2008

m3

Crystal Ball

672 NaI(Tl)

Cleo II

7800 CsI(Tl)

L3

12000 BGO

Crystal Barrel

1380 CsI(Tl) TAPS

600 BaF2

KTeV

3100 CsI

Babar

6580 CsI(Tl)

Belle8816 CsI(Tl)

Alice

17920 PWO

CMS75000 PWO

From Crystal Ball

5

10

To CMS

P. Lecoq

Page 33: The CMS Construction

CMS Requests and PWO

1995 1998

T dependent: -2%/°C

To comply with LHC and CMSTo comply with LHC and CMSconditions ECAL must be:conditions ECAL must be:• fastfast• compactcompact• highly segmented highly segmented • radiation resistantradiation resistant

Very low light outputVery effective in highenergy containment

2

Page 34: The CMS Construction

ECAL layout

barrelbarrelSuper ModuleSuper Module(1700 crystals)(1700 crystals)

endcapendcapsupercystalssupercystals(5x5 crystals)(5x5 crystals)

Pb/Si preshowerPb/Si preshower

barrel cystalsbarrel cystals

EndCap “Dee”EndCap “Dee”3662 crystals3662 crystals

Barrel: Barrel: ||| < 1.48| < 1.48

36 Super Modules36 Super Modules61200 crystals (61200 crystals (2x2x23cm2x2x23cm33))

EndCaps: EndCaps: 1.48 < |1.48 < || < 3.0| < 3.0

4 Dees4 Dees14648 crystals 14648 crystals (3x3x22cm(3x3x22cm33))

PWO: PbWO4

about 10 m3, 90 t

Page 35: The CMS Construction

Choice of the Photodetector

20

40mdeff ~6m

Avalanche photodiodes (APD)

Two 5x5 mm2 APDs/crystal- Gain: 50 QE: ~75% @ peak= 420 nm- Temperature dependence: -2.4%/OC- Gain dependence on bias V: 3%/V

Page 36: The CMS Construction

PWO Production

BARREL ingot

45000

47000

49000

51000

53000

55000

57000

59000

61000

63000

Dec-05 Mar-06 Jul-06 Oct-06 Jan-07 Apr-07

Del

iver

ed B

arre

l cr

ysta

ls

BARREL CRYSTALS ~ 1150 xl/m

EE INGOT

ENDCAPS ingots

Page 37: The CMS Construction

EB Construction: Regional Centers

CERN Lab.27 EP-CMA

Casaccia

&

Assembly and test of modules in RC: ENDED in March 2007

Submodule 2x5 crystals

Submodule 2x5 crystals

Module400 crystals

Page 38: The CMS Construction

INFN/ENEA Regional CenterCheck crystals in Rome RC

Glue subunits and check APD gain

The first submodule!The first module!

Y 2002

Page 39: The CMS Construction

EB Construction: Super Modules

Supermodule1700 crytsalsSupermodule1700 crytsals

Cooling and electronics integration: completion by May 2007

Dead channels: 19/61200

Page 40: The CMS Construction

ECAL PerformanceResponse to high energy electrons

Temperature Stability: ≤ 0.1 °CLight response stability: ≤ 0.1%

0.5%

Page 41: The CMS Construction

ECAL: Cosmics Signal in CMS

Page 42: The CMS Construction

Layout of CMS Muon System

250 DTs 468 CSCs 480 RPCs

Page 43: The CMS Construction

Spatial resolution: Single cell 200 mChamber 100 m

Muon System: Drift Tubes

MylarMylar

Electrode Electrode StripStrip

Wire

42mm

13 mm

Page 44: The CMS Construction

Legnaro Assembly Hall

Torino Assembly Hall

Assembly of 250 DT chambers:70 Aachen, 70 Madrid70 Padova, 40 Torino• 1 layer = 70 wires• 27 gluing operations/chamber• 1 gluing operation = 1 dayPrecision of 100 m over 5-10 m2

DT Chambers Assembly

Page 45: The CMS Construction

CERN ISR

First installation Aug.03

Salvato

Peghin

First installation test Aug. 2002

Muon System: Start of Installation

Page 46: The CMS Construction

ISTALLATION OF THE LAST OF THE 250 DT CHAMBERS IN THE CAVERN. IN WHEEL YB0 26 Oct. 2007

Muon System Completed

Page 47: The CMS Construction

S11

S12

17Hz

S01

3Hz

10Hz

15HzS0330Hz

Muon System: YB0 DTs in Operation!

Page 48: The CMS Construction

Gas mixture95.5 C95.5 C22HH22FF4 4

3.5 iC3.5 iC44HH1010 0.3 SF0.3 SF66

+ RH 50%+ RH 50%

Main Unit of a RPC: Single Gap (SG)

Two SG coupled with readout plane in between

•Bakelite thickness: 2 mm•Bakelite bulk resistivity : 2-6 1010 cm• Gas Gap width: 2 mm•Operating voltage: 9.2-9.8 kV

Main characteristics of the RPCs used in CMS:

Muon System: Resistive Plate Chambers

Page 49: The CMS Construction

RB4 120 chambers (2 double gaps/chamber)

RB3 120 chambers (2 double gaps/chamber)

RB2 60 chambers (2 double gaps/chamber) + 60 chambers (3 double gaps/chamber)

RB1 120 chambers (2 double gaps/chamber)

Forward UP

Forward Down

Backward UP

Backward Down

DoubleDouble

Gap Gap DGDG

DoubleDouble

Gap Gap DGDG

RPC chamber layout

480 RPCs coupled with DTs and inserted into the iron return yoke of the magnet

Page 50: The CMS Construction

RPC Performance

Efficiency

Counting rate

All parameters are compatible with the results obtained during the production tests

Cluster size

Page 51: The CMS Construction

RPC: First Events in CMS

Page 52: The CMS Construction

First Closure of the CMS Experiment (2006)

Page 53: The CMS Construction

Magnet Test & Cosmic Challenge (MTCC)

HCAL

Magnet

Tracker

Muon chambers

ECAL

Page 54: The CMS Construction

Run 2605 / Event 3981 / B 3.8 T / 27.08.06

Page 55: The CMS Construction

Cosmics in the Tracker (Bat 186)

•The Quality of the CMS Tracker is Excellent: • Dead or Noisy Strips < 3 / 1000

• Signal: Noise > 25:1 in Peak Readout Mode

• Enormous experience gained in operating the Tracker at TIF

Normal Strips 99.852 % (241 313 Strips)

Dead Strips 0.116 % (275 Strips)

Noisy Strips 0.032 % (76 Strips)

Example of Performance

A cosmic at -15°CValidated clusters shown

Page 56: The CMS Construction

Performance of CMS: Overview

Tracking

HCAL

b-tagging