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February 19th 2009 AlbaNova Instrumentation Seminar 1
Christian BohmInstrumentation Physics, SU
Upgrading the ATLAS detector
OverviewMotivationThe current design and whyWhy upgradeHowPlanning the short range development
February 19th 2009 AlbaNova Instrumentation Seminar 2
MotivationAccelerator upgrades will increase the luminosity above the design value 1034 cm-2s-1
Phase II Bunch Crossing (BC) rate may change 25->50 ns
February 19th 2009 AlbaNova Instrumentation Seminar 3
Design criteria/considerations for an ATLAS type detector • Higher energies to study new phenomena
• Large luminosity to study rare events – many events to reach 5
February 19th 2009 AlbaNova Instrumentation Seminar 4
Design criteria/considerations for an ATLAS type detector • Higher energies to study new phenomena
• Large luminosity to study rare events – many events to reach 5
• Tracker near beam pipe to determine the source position• Magnet around beam pipe for momentum information
• Large E/M calorimeter to stop and measure energy of electrons and photons – not too large to stop hadrons as well
February 19th 2009 AlbaNova Instrumentation Seminar 5
Design criteria/considerations for an ATLAS type detector • Higher energies to study new phenomena
• Large luminosity to study rare events – many events to reach 5
• Tracker near beam pipe to determine the source position• Magnet around beam pipe for momentum information
• Large E/M calorimeter to stop and measure energy of electrons and photons – not too large to stop hadrons as well
• Large hadron calorimeter to stop and measure energy of hadrons• Minimize matter in front of calorimeters to improve resolution
• Should the magnet be inside or outside the calorimeters• Large muon detector with strong magnetic field to measure muon energies with high precision.
February 19th 2009 AlbaNova Instrumentation Seminar 6
Design criteria/considerations for the on-detector electronics
Radian tolerance and reliability main problems
Long design cycles -> problems with obsolescence
Paradigm shifts during long development processes
February 19th 2009 AlbaNova Instrumentation Seminar 7
Design criteria/considerations for the on-detector electronics
Radiation tolerance and reliability main problems
Long design cycles -> problems with obsolescence
Paradigm shifts during long development processes
• Radiation tolerance achievable – bandwidth expensiveOn-detector logic and memories – transfer only if necessary• Radiation tolerance expensive – bandwidth achievable
Minimize on-detector electronics – transfer as soon as possible• Radiation tolerance achievable – bandwidth achievable
On-detector logic OK but minimize for reliability – protect for transient errors
February 19th 2009 AlbaNova Instrumentation Seminar 8
Design criteria/considerations for the on-detector electronics
Radian tolerance and reliability main problems
Long design cycles -> problems with obsolescence
Paradigm shifts during long development processes
• Radiation tolerance achievable – bandwidth expensiveOn-detector logic and memories – transfer only if necessary• Radiation tolerance expensive – bandwidth achievable
Minimize on-detector electronics – transfer as soon as possible• Radiation tolerance achievable – bandwidth achievable
On-detector logic OK but minimize for reliability – protect for transient errors
ASICs -> FPGAs (sometimes even on-detector)
Another change:During phase 0 LHC projects were often driving technology development
Now it is telecom
February 19th 2009 AlbaNova Instrumentation Seminar 10
Current design ATLAS data Flow
40M
Hz
LHC physics looks for rareevents – 1 in 1014
High event rates andHigh selectivity
new data every 25 ns
About 100 million channels
February 19th 2009 AlbaNova Instrumentation Seminar 11
Current design ATLAS data Flow
40
M H
z
1 event in 400
new data every 25 ns
Since all data must be stored while waiting for the L1 decision the L1 processing must be quick – <2.5ns
Data from entire detector but with low spatial resolution and reduced dynamic range from calorimeters and muon detector
About 100 million channels
75
k
Hz
The high granularity datais merged into roughly 64x64 trigger towers each.1x.1 in and where = log
Design requirement
February 19th 2009 AlbaNova Instrumentation Seminar 12
Current design ATLAS data Flow
2 k
Hz
40
M H
z
new data every 25 ns
About 100 million channels
1 event in 100
Data from ROIs with high spatial resolution and full dynamic range from all subdetectors 7
5
kH
z
February 19th 2009 AlbaNova Instrumentation Seminar 13
Current design ATLAS data Flow
new data every 25 ns
20
0 H
z2
kH
z7
5
kH
z4
0M
Hz
About 100 million channels
1 event in 100
Entire detector with high spatial resolution and full dynamic range from all subdetectors
To Grid
February 19th 2009 AlbaNova Instrumentation Seminar 14
Current design L1 Trigger algorithms
Look for isolated particles
e/ /had
Simplistically regard the L1 processor as consisting of 4096
parallel processors – one for each .1x.1
trigger tower
Count the number different threshold combinations in the central trigger
processor (CTP)
February 19th 2009 AlbaNova Instrumentation Seminar 15
Current design L1 Trigger algorithms
Look for JETs
0.4 x 0.4
0.6 x 0.6
0.8 x 0.8
ROI Identification Identify 0.4 x 0.4 windows
that are local maxima Jet Identification
Apply thresholds to 0.4, 0.6, or 0.8 clusters around the local maxima
8 Jet definitions available, each with selectable energy threshold and cluster size
Simplistically regard the L1 processor as consisting of 1024
parallel processors – one for each .2x.2
trigger tower
Count the number different threshold combinations in the CTP
February 19th 2009 AlbaNova Instrumentation Seminar 16
The x3 increased luminosity will lead to increased radiation levels and more pile-up
Phase I upgrade, 6 months
The inner layer of the inner detector must be replaced due to radiation damage
February 19th 2009 AlbaNova Instrumentation Seminar 17
The phase I upgrade
Since the innermost layer cannot be replaced a new layer (IBL) is insertedcloser to the beam pipe -> smaller beam pipe
Another detector part that may need replacement is the FCAL electronics
Increased luminosity ->more events
Unrealistic to change level 2 rate ->Improve L1 rejection
One way is to increase thresholds
Another way is to improve L1 trigger by bringingsome L2 processing down to
L1
February 19th 2009 AlbaNova Instrumentation Seminar 18
The phase I upgrade
Topological algorithms can be introduced in the L1 calorimeter trigger
Use the ROI position information
Takes additional time to determine in L1Calo and
to evaluate in the L1 CTP
The latency margin seem to suffice
The main part of L1Calo stays
inserting a new layer between L1Calo and CTP
and a new CTP
February 19th 2009 AlbaNova Instrumentation Seminar 19
The x10 increased luminosity will lead to more increased radiation levels and still worse pile-up
Phase II upgrade, 1.5 years
All the on detector electronics has reached its designed life
time
February 19th 2009 AlbaNova Instrumentation Seminar 20
Phase II upgrade
Completely new inner detectorThe rest of the detector more or less OK
New calorimeter on-detector and off-detector electronics
Increased luminosity ->new electronicsIncreased luminosity ->more events->more logic
Level 2 rate fixed?!
Completely new L1 trigger
February 19th 2009 AlbaNova Instrumentation Seminar 21
Phase II upgrade
Increased luminosity -> increased L1 trigger efficiency -> more information to L1
High granularity, depth segmented info from calorimeters
Higher thresholds not enoughmore info from muon detector?
or a Track trigger?Simulations needed
February 19th 2009 AlbaNova Instrumentation Seminar 22
Calorimeter ideas
Full readout
Minimize on-detector electronics
Massive data transfers
Preprocessor delivers tower info with flagse.g. high granularity or depth flags
February 19th 2009 AlbaNova Instrumentation Seminar 23
Track trigger ideas
High Pt trigger
Supply track info on demand -> much longer latencies
L 1.5 track trigger
Very challenging
February 19th 2009 AlbaNova Instrumentation Seminar 24
Practical planning Less work than phase 0
FinancingLong lead times
Radiation tolerance testingSIMULATIONS NEEDED
Experience from running ATLAS (radiation damage)Coordination with machine, CMS,…
Organize installationOrganizational structures: USGs, UPOs, ATLAS weeks, meetings,
meetings,….
SchedulePhase I (2013) and phase II (2017) – mostly controlled by machine
development which is not primarily affected by the delay,the schedule may thus not slide with the startup delay.
Atlas upgrade LoI 2009, IBL TDR 2009,upgrade TP 2010 (maybe with options),
upgrade TDR 2011
We are already late compared to phase 0!