Top Banner
The Commissioning The Commissioning of the ATLAS Pixel of the ATLAS Pixel Detector Detector XCIV National Congress Italian Physical Society Genova, 22-27 Settembre 2008 Nicoletta Garelli
13

The Commissioning of the ATLAS Pixel Detectorstatic.sif.it/SIF/resources/public/files/congr/mc2008/garelli_08.pdf · The Commissioning of the ATLAS Pixel Detector XCIV National Congress

Jul 20, 2018

Download

Documents

dokhanh
Welcome message from author
This document is posted to help you gain knowledge. Please leave a comment to let me know what you think about it! Share it to your friends and learn new things together.
Transcript
Page 1: The Commissioning of the ATLAS Pixel Detectorstatic.sif.it/SIF/resources/public/files/congr/mc2008/garelli_08.pdf · The Commissioning of the ATLAS Pixel Detector XCIV National Congress

The Commissioning The Commissioning of the ATLAS Pixel of the ATLAS Pixel

DetectorDetector

XCIV National Congress Italian Physical Society

Genova, 22-27 Settembre 2008

Nicoletta Garelli

Page 2: The Commissioning of the ATLAS Pixel Detectorstatic.sif.it/SIF/resources/public/files/congr/mc2008/garelli_08.pdf · The Commissioning of the ATLAS Pixel Detector XCIV National Congress

Large Hadronic ColliderLarge Hadronic Collider

Opal

Delphi

SPS

PS

 

LHCAleph

L3

LHCb

Alice

ATLAS

CMS

MOTIVATION: Find Higgs Boson and New Physics Beyond the Standard Model

LHC is being built in a circular tunnel 27 km in circumference, 50-175 m underground.

Beams inside continuous vacuum guided by superconducting magnets.

Bunch cross every 25 ns 600 million collisions per second

4 collision points

Machine

Beams

Energy

Luminosity

LHC p p 14 TeV 1034 cm-2s-1

LHC Pb Pb 5.5 TeV

1027 cm-2s-1

Tevatron p anti-p

2.0 TeV

1032 cm-2s-1

LEP e+ e- 200 GeV

1032 cm-2s-1

2

Page 3: The Commissioning of the ATLAS Pixel Detectorstatic.sif.it/SIF/resources/public/files/congr/mc2008/garelli_08.pdf · The Commissioning of the ATLAS Pixel Detector XCIV National Congress

SM Higgs BosonSM Higgs Boson

LEP direct search: mH>114.4 GeV/c2

@95%CL

LEP Electroweak Fit Limit: mH<144 GeV/c2 @95%CL

3

Page 4: The Commissioning of the ATLAS Pixel Detectorstatic.sif.it/SIF/resources/public/files/congr/mc2008/garelli_08.pdf · The Commissioning of the ATLAS Pixel Detector XCIV National Congress

Higgs Mass Range – Detector Higgs Mass Range – Detector RequirementsRequirements

114.5 < MH < 130 GeVGolden channel: Hγ γ But small decay rate! QCD background.

130 < MH < 800 GeVGolden channel: HZZ/ZZ*4l

• Powerful inner tracking systems in magnetic field with high granularity and secondary vertex reconstruction capability. Crucial for background rejection.

• High granularity hadronic calorimeter with full coverage for good missing ET resolution, jet trigger and reconstruction.

• Electromagnetic calorimeter with good energy and spatial resolution, capability to separate γ /π0 .

• Efficient muon spectrometer for identification, trigger, and momentum measurement of high energetic muons.

800 < MH< 1000 GeVHWWlνjjET missing

4

Page 5: The Commissioning of the ATLAS Pixel Detectorstatic.sif.it/SIF/resources/public/files/congr/mc2008/garelli_08.pdf · The Commissioning of the ATLAS Pixel Detector XCIV National Congress

ATLASATLAS A Thoroidal LHC ApparatuSA Thoroidal LHC ApparatuS

Cylindrical ‘Onion-like’ Detector

5

Page 6: The Commissioning of the ATLAS Pixel Detectorstatic.sif.it/SIF/resources/public/files/congr/mc2008/garelli_08.pdf · The Commissioning of the ATLAS Pixel Detector XCIV National Congress

The ATLAS Inner DetectorThe ATLAS Inner DetectorTechnique: high granularity + low occupancy + 2D track measurementGeometry:3 Barrel layers (r = 5, 9, 12 cm) + 2 End-Caps with 3 Disks each

3 space points for η< 2.5 with resolution 16µm – 115 µm

PIXEL

6

Page 7: The Commissioning of the ATLAS Pixel Detectorstatic.sif.it/SIF/resources/public/files/congr/mc2008/garelli_08.pdf · The Commissioning of the ATLAS Pixel Detector XCIV National Congress

The Pixel DetectorThe Pixel DetectorHigh multiplicity tracking detector:

~ 1200 tracks per bunch crossing high granularity (80 million ⇒channels!)

High radiation dose tolerance: ~50 Mrad

High impact parameterresolution: ~ 12 μm vertex resolution – secondary vertex reconstruction

High time resolution: 40 MHz bunch crossing rate

Low interaction length: ~10% χ0

7

Page 8: The Commissioning of the ATLAS Pixel Detectorstatic.sif.it/SIF/resources/public/files/congr/mc2008/garelli_08.pdf · The Commissioning of the ATLAS Pixel Detector XCIV National Congress

After ~20 years waiting… finally beams circulating in LHC!

• Beams with injection energy of 450GeV. •Pixel Detector OFF for safety reason.

The 10The 10thth September 2008 September 2008

•The way towards collisions and LHC stable operation is still long… •LHC Magnet Accident of 19th September 2008.

8

Page 9: The Commissioning of the ATLAS Pixel Detectorstatic.sif.it/SIF/resources/public/files/congr/mc2008/garelli_08.pdf · The Commissioning of the ATLAS Pixel Detector XCIV National Congress

Pixel Detector MilestonesPixel Detector Milestones

July 2007: Installation of pixel-package in the cavern.

December 2007: Finished service connections.

February – April 2008: Sign-Off (=test on light transmission to and from detector, verify that analog and digital parts of the modules are powered, check the sensor) + Cooling Plant commissioning.

August 2008: Cooling plant operative after 3 months of accident recovery, finally cosmic runs and calibration procedure.

9

Page 10: The Commissioning of the ATLAS Pixel Detectorstatic.sif.it/SIF/resources/public/files/congr/mc2008/garelli_08.pdf · The Commissioning of the ATLAS Pixel Detector XCIV National Congress

The Readout SystemThe Readout System

Pixel Module Optoboard

BOC

TXRX

S-Link

ROD

L1A

SBC

ROBIN

S-link

Signal: discriminator decision on amplified charge deposition within the pixels.

1 Module = ~50k pixelsDetector = 1744 Modules

10

16 FE chips

Bump bonds

PP0 connection

Wire bondsOptimize detector

response calibrate readout electronics, tune on-line and store results.

Page 11: The Commissioning of the ATLAS Pixel Detectorstatic.sif.it/SIF/resources/public/files/congr/mc2008/garelli_08.pdf · The Commissioning of the ATLAS Pixel Detector XCIV National Congress

Module Tuning. Motivation: Mean energy loss in pixels changes in time due to irradiation. Calibration Source: Directly inject charge (VCal) Calibration Procedure: Many! Vary VCal and determine distribution for the discriminator threshold, the noise (slope of signal rise), the Time-Over-Threshold (ToT, indirect charge deposit measurement), … for each pixel.Tune link between on-detector

Optoboards and off-detector Back-Of-Crate cards:Laser Power for the Optoboard (ViSet)Threshold at the BOC Delays at the BOCFind optimal values for individual module by varying the three parameters

The Calibration Procedure The Calibration Procedure 1/21/2

Threshold Noise

RECENT OUTCOME11

57/1744 modules with optical communication problems 80/1744 (~5%) bad modules excluded from data taking

Page 12: The Commissioning of the ATLAS Pixel Detectorstatic.sif.it/SIF/resources/public/files/congr/mc2008/garelli_08.pdf · The Commissioning of the ATLAS Pixel Detector XCIV National Congress

Calibration Procedures 2/2

The calibration procedures produce an huge amount of histograms, both on-line and off-line.

Need to analyze data on-line in order to take decision about “bad modules” to disable during the data taking.

Efficient on-line histogram dispatching system, Pixel Histo Server, using multi-threaded and distributed software.

The Software ChallengeThe Software Challenge

The Pixel Detector accesses an huge amount of information (# of channels and # of configuration parameters).

Pixel Database Server handle in a fast and efficient way the configuration of

the Pixel Detector caching mechanism

12

Page 13: The Commissioning of the ATLAS Pixel Detectorstatic.sif.it/SIF/resources/public/files/congr/mc2008/garelli_08.pdf · The Commissioning of the ATLAS Pixel Detector XCIV National Congress

Cosmic RunsCosmic Runs

First Track!First Track!Event with 7

Pixel hits (overlapping L2 modules) and 16 SCT

hits

Cosmic Trigger provided by Muon Chambers and Calorimeters5K/80·106 noisy pixels masked (occupancy >10-5)

13