The ATLAS High Level Trigger
Véronique Boisvert CERN
On behalf of the ATLAS Trigger/DAQ High Level Trigger Group
Université de Montréal-McGill Seminar
August 18th 2003 Rockefeller Center NY, USA
Outline
Physics Motivation
Selection Strategies
ATLAS detector
LHC environment
Trigger Architectures
High Level Trigger (HLT) Selection Software
Measurements
Conclusions
V. Boisvert
The Big Questions
Is there unification of all forces?
What breaks it?
What breaks EW Symmetry?
What is the origin of mass?
What is the physics beyond The SM? New particles?
New interactions?
Flavor Puzzles:
Can we understand the masses And mixing of fermions.
Where does CP come from?
Are there more forces?
Particles? Symmetries?
Explain the masses of The p and e, and the
Relative strengths of The fundamental forces
Do we understand the Structure and fate of
The universe?
Are there extra Dimensions? What is the
structure of spacetime?
What is the right description Of gravity and where does it Become relevant for particle
Physics?
VLHC 100TeV
pp
0.5-1.0 TeV e+e- Collider
Mu Collider
Nu Factory
High Luminosity
Z Factory
B,K,tau/charm Factory
Tevatron 2TeV
pp
Particle Astrophysics 14 TeV
Pp
LHC
Can we explain the universe?
Why is it matter dominated?
Cosmological Constant?
Dark Matter Problem?
Some Answers from the LHC
Electroweak symmetry breaking
Precise Standard Model measurements
B physics
Physics beyond the Standard Model:
SUSY
Exotics
The unknown!
V. Boisvert
Electroweak Symmetry Breaking
SM Higgs:
114.4GeV < mH < 1TeV
LHC Higgs production and cross-sections
Higgs decays:
Fully hadronic:
Large QCD background
Gold plated modes:
H
Signature: pT >= 50GeV/c
~6 for mH=120GeV, 30 fb-1
Electroweak Symmetry Breaking
Gold plated modes:
H ZZ(*) 4l
• Signature: 4 high pT l
• =3-25 (dep. mH), 30fb-1
•
Other typical signatures:• tt,bb,ll,ll,lljj
•
MSSM Higgs• Typical signatures for H0, h0, A, H:
• ,,,tb
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Precision Measurements of SM
High Luminosity and High E
LHC is the ultimate factory:
B, top, W, Z, H, …
1:1013 for Higgs
Deviations from SM
Hints of new physics
Precise W mass
W jj
• Large QCD background
• W e()
• reco. in transverse plane!
Precision Measurements of SM
Precise W mass
Very dependent on E scale (0.02%)
Built-in calibration system
e,, ATLAS, CMS: mW~15MeV (today ~34MeV)
Precise Top mass: tt
t Wb Signatures:
• Jets (including b-jets), l, Etmiss
• All channels, ATLAS, CMS:
mt~1-2GeV (today ~ 5.1GeV)
• Indirect mH~25%! (today
LHC
V. Boisvert
B physics
Copious production of B’s:
CP-violation, Bs oscillations, Rare decays, etc.
B
d J/ K
S• Max performance: (sin2)=0.010
• Min performance: (sin2)=0.016
• Rare decays
• Forward-Backward A: B0d K*0 +-
• Lowest mass region: enough accuracy to detect New Physics
• Signatures: di-leptons (), semi- exclusive reconstruction
q2/MB2 AFB
SuperSymmetry
SM is an effective theory:
Gauge coupling unification (families, gravity, etc.)
Fine-tuning
Hierarchy problem
SUSY: supersymmetric partners s-1/2
Pros:
Elimination of fine-tuning by exact cancellations between partners
Quark masses: radiative corrections in SUSY
Consistent with string theories (incl. gravity)
Cons:
No observation! broken, many free parameters and extensions
V. Boisvert
SUSY
MSSM particle spectrum, current limits:
ml, > 90-100 GeV (LEP)
mq,g > 250 GeV (Run 1)
Lightest SUSY Particle (LSP) is 10
Cold dark matter candidate
Do neutralino reconstruction!
Signature: ETmiss
Decay chains
No SM background, 2-body kinematics
Need jets, l, ETmiss
l
mq~L
~
q
l
l
~
R
Beyond the SM
SUSY, Technicolor, Little Higgs, New fermions and gauge bosons, compositeness,…
Large Extra Dimensions
Solves hierarchy problem:
1 fundamental scale: EW scale (TeV)
Gravity is weak because propagate in 3+n dimensions
Cosmological implications
Constraints from astrophysics
Possible explanation for dark matter
Etc.
Tests Gravity and String Theory in the lab!
3-brane bulk
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Beyond the SM
n2: ADD
Graviton emission
Signature: jet() + ETmiss
Randall-Sundrum:
n=1
Warped
2 branes (Planck and TeV)
Radion: represents
fluctuations of the distance between the 2 branes
Signature: Higgs like
Mini black holes!
Gr
r
So far…
With a little bit of luck the LHC could completely revolutionize our field!
Highlighted possible signatures
Other constraints on the trigger architecture?
V. Boisvert
The LHC at CERN
From: P. Sphicas 2003
The LHC environment
Interaction rate: L x (pp) = 10
34cm
-2s
-1x 70mb = 10
7mb
-1Hz x 70mb = 7x10
8Hz!
~3600 bunches in LHC
Length of tunnel is 27Km
Time between bunches: 25ns! (40MHz bunch x rate)
V. Boisvert
The LHC environment
Interactions per crossing: ~23!
Minimum bias events overlap each event of interest
We have “pile-up”
“In-time”: particles from same crossing but different pp interaction
“Out-of-time”: left-over signals from previous crossings
Need bunch crossing identification
Time of flight…
22 m
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pp collisions at high luminosity
HZZ 4
T/DAQ challenges
efficient signal selection and excellent background rejection
Interaction rate: 7x10
8Hz
Store data at 100 Hz
Bunch crossing rate: 40MHz
Out of time Pile-up
Synchronization over detectors
High number of channels at high occupancy
It’s online!!
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Selection Strategies
2 main guiding principles:
Inclusive selection
Mostly 1 or 2 objects (electron, muon, photon, jet, b- tagged jet, tau, ETmiss, ET)
High pT : > O(10GeV/c)
Worry about:
Low mass objects (eg B physics)
Exclusive selection, topology, etc.
Biases in selection
Use complementary selections
Selection Strategies
Object
Object Examples of physics coverageExamples of physics coverage NomenclatureNomenclature Electrons Higgs (SM, MSSM), new gauge
bosons,
extra dimensions, SUSY, W, top e25i, 2e15ie25i, 2e15i Photons Higgs (SM, MSSM), extra
dimensions, SUSY 60i, 260i, 220i20i Muons Higgs (SM, MSSM), new gauge
bosons,
extra dimensions, SUSY, W, top 20, 220, 21010 Jets SUSY, compositeness, resonances j360, 3j150, 4j100j360, 3j150, 4j100 Jet+missing ET SUSY, leptoquarks j60 + xE60j60 + xE60
Extended Higgs models (e.g. MSSM),
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So far…
The LHC environment is brutal to a Trigger DAQ system
How to get the job done:
Trigger Architecture
The ATLAS Trigger Architecture
40 MHz
75 kHz
~1 kHz
~100 Hz
~1 sec
~10 ms
2.5 s
Level 1 Level 1 trigger trigger
High Level TriggerHigh Level Trigger Level 2Level 2 trigger trigger
Event Event Filter Filter
Region of Interest RoI
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Introduction: Regions of Interest
Typically a few ROI / event
Ex: Pixel 0.2x0.2
~ 92 Modules ~ 332 channels
Only few % of event data
required!
ATLAS, CMS vs Other detectors
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ATLAS vs CMS
ATLAS:
Smaller bandwidth
But more complex
CMS:
Simpler system
But very high bandwidth
dependent on technology
So far…
Introduced ATLAS Trigger Architecture
Let’s look at the HLT Selection Software
Handle to making the Trigger decision
Measurements
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HLT Selection principles
Fast
Early rejection
Seeding
Data on demand (RoI or whole event)
Modify easily signatures
Precise knowledge of detectors and algorithms:
offline community
Use offline code in the HLT software
Develop Trigger Alg in offline framework
Study boundary between Level 2 and EF
Performance studies for physics analysis
HLT Selection principles
Offline into online: not an easy task!
Requirements of speed and multi-threading on core infrastructure
different steering philosophy:
Offline: typically process entire events in a sequential fashion (post data on a whiteboard)
Online: seeded and early rejection
Appointment of a Reconstruction Task Force
Look at issues regarding offline-online unification
High Level Design (data flow, EDM)
Subdetectors reconstruction
Combined reconstruction
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HLT Design Overview
HLT Selection Software
HLTSSW
Steering
ROBData Collector
Data Manager
HLT Algorithms Processing
Application
Event DataModel Processing
Application
Interface Dependency Package
Event Filter
HLT Core Software
HLT Algorithms
Level2
HLT Selection Software
HLT DataFlow Software
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The Steering
Requirement:
Early rejection
Chosen strategy:
Seeding mechanism
Step wise process
Iso lation
pT>
30GeV
Cluster shape
track finding
Iso lation
pT>
30GeV
Cluster shape
track finding
EM20i + EM20i e30i + e30i
e30 + e30
e + e
ecand + ecand Signature
Signature
Signature
Signature
Level1 seed
STEP 1 STEP 4
STEP 3
STEP 2
Steering
HLT algorithms: e, selection
Level1: selects calorimeter info over coarse granularity
Level2:
1)cluster E, position, shower- shape variables
Refine L1 position: max E (1, 1)
Refine (1, 1) with Energy
weigthed average in window 3x7:
(c, c)
Parameters to select clusters:
Sam. 2: Rshape = E37/E77
Sam. 1: Rshape = E1-E2/E1+E2
EM LAr calorimeter
~190,000 channels
For 25GeV: E/E~7%, ~8mrad, r~1.6mm
HLT Algorithms
V. Boisvert
HLT algorithms: e, selection
Level 2:
2) need Track in InDet for el: Pixel, SCT
algorithm
Z-finder
Hit Filter
Group Cleaner
Track Fitter
z
Momentum res.: pT/pT ~ 0.1 pT (TeV) Impact parameters: r< 20m z < 100m
HLT Algorithms
HLT algorithms : e, selection
Event Filter:For electrons passing Level 2, reexamined at EF
Use offline reconstruction algorithms
Calibrated data for the InnerDetector
More tools for reconstruction since full event
Measurements: single el, p
T=25GeV/c
Fully simulated events, latest software
Pile-up for low and high lum
Up to date geometry, amount of material, B field
HLT Algorithms
Trigger Step Rate (Hz) Efficiency (%) Level2 Calo 2114±48 95.9.3
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The Data Access
Algorithm Region Selector
HLT
Algorithm Region
Selector
Trans.
Event Store
Data Access
Byte Stream Converter
Data source organized
by ROB
Transient EventStore
region list DetElem IDs
ROB ID raw event DetElems data
list DetElem IDs list DetElem IDs
DetElems Data Manager
Collection Number Number of ROBs
Pixel module 1744 81
SCT side of module 8176 256
TRT straw layer 19008 256
LAr Trigger Tower 7168 768
Tile module 256 32
Muon MDT chamber 1168 192
Muon CSC chamber 32 32
Muon RPC chamber 574 32
Muon TGC chamber 1584 32
Data access granularity
Preliminary
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The Event Data Model
Raw Data in byte stream format
Level1, Level2, EF results, ROB data
Different formats of Raw Data for particular subdetector
RawDataObjects are object representation of Raw Data
For InnerDetector the RDOs are skipped for Level2 (data preparation in converters)
Features
Clusters, Tracks, electrons, jets, etc.
MCTruth info
For debugging and performance evaluation
Trigger Related data
ROI objects, Trigger Type, Trigger Element, Signatures
Offline dependencies!
Event DataModel
HLT Selection Software
HLTSSW
Steering
ROBData Collector
Data Manager
HLT Algorithms Processing
Application
Event DataModel Processing
Application
Interface Dependency Package
Event Filter
HLT Core Software
HLT Algorithms
Level2
HLT Selection Software
HLT DataFlow Software
<<import>>
<<import>>
<<import>>
<<import>>
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Timing Measurements
Timing on 2GHz machine Level2 Calo ~2ms Level2 Tracking ~3ms
~EF ~0.5s
Steering
Algorithms
Region Selector Data Access
1GHz, 3 seeds: 1.2ms
Infrastructure: ~23μ
aaae: Muo <8(GHz) Lar/Tile <(GHz)
Iereeor iproveeuerwa
1GHz, Tile: 0.03ms, Pixel:0.2ms, TRT:1.1ms
Measurements
Putting it all together in the most realistic
environment: the Level 2 Test bed
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Conclusions
The LHC: quite a challenge!
The LHC detectors Trigger DAQ systems
Interesting comparisons coming!
The ATLAS architecture
RoI mechanism
Use of offline code in online environment
HLT selection software is adequate and performant