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Faster tracking in hadron collider experiments

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Use differences between physics event and pile-up to clean up the event first! ... hit-filter: once z is known, it rejects pile-up/noise/ghost hits ... – PowerPoint PPT presentation

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Title: Faster tracking in hadron collider experiments


1
Faster tracking in hadron collider experiments
  • The problem
  • The solution
  • Conclusions

Hans Drevermann (CERN) Nikos Konstantinidis
( Santa Cruz)
2
The problem
  • General problem with tracking is combinatorics
  • Soon, at hadron colliders many pp interactions in
    one the physics event plus several pile-up
    events (20 at LHC design L )
  • increased hit occupancy, especially in inner
    layers
  • higher combinatorics

    gt longer processing time gt increased hit
    misassociation
    (i.e. performance
    degradation of the tracking algorithms)
  • At the LHC (design L )
  • typically 20K-40K hits/event
  • bunch crossing every 25ns
    gt LVL2
    trigger algorithms should take not more than 20ms

3
A typical event in ATLAS
4
A traditional approach (ATLAS)
  • To reduce combinatorics work in a Region of
    Interest (RoI), defined from calorimeter info
  • RoI a rectangular slice in (h,f), but extended
    in z

5
The new idea
  • Use differences between physics event and pile-up
    to clean up the event first!
  • Physics event vs. pile-up two main differences
  • pp interactions happen at different z positions
  • (at LHC sz 6 cm, i.e. pp interactions within
    30 cm)
  • the physics event has (on average) higher pT
  • Use these two differences to reduce combinatorics
  • First, find the z position of the physics event
  • Then, select groups of hits which could be due to
    a track coming from the above z position, reject
    all other hits (pile-up, noise, ghost)

6
Physics event vs. pile-up
7
Quantitative Examples
  • ATLAS at the LHC design luminosity
  • Results demonstrated with RoIs from
  • pT40GeV/c isolated electrons
  • Size of RoI Dh0.2 Df0.2 Dz11cm
  • Average number of hits per RoI 230
  • Thin QCD jets (bkg to electron RoIs)
  • Size of RoI Dh0.2 Df0.2 Dz11cm
  • Average number of hits per RoI 250
  • Jets from WH (mH100GeV/c2 and H bb)
  • Size of RoI Dh1.0 Df1.0 Dz15cm
  • Average number of hits per RoI 1250

8
The z - finder
  • The principle
  • Divide the RoI into many small f bins
  • In each f bin, make all pairs of hits from
    different layers
  • For each pair, find the z by linear extrapolation
    and fill a 1D-histogram
  • z is the bin of the 1D-histogram with the max.
    of entries
  • No need to reconstruct tracks
  • Key are the small f bins
  • they naturally give more weight to high pT tracks
    (i.e. physics event vs. pile-up)
  • they reduce combinatorics drastically, hence,
    reduce the quadratic time behaviour of the
    algorithm

9
Example of a z-histogram
From a WH(100) jet RoI
10
Performance issues
  • Efficiency - Resolution - Timing
  • ( Timing measurements with a Pentium- III 600MHz
    processor )
  • Flexibility - Robustness
  • ( Very important for trigger algorithms )

11
Efficiency - Resolution - Timing
Efficiency (pT40GeV electrons)
( RoIs with zreco-ztruelt5mm )
Resolution (pT40GeV electrons)
Timing (in ms)
pT40GeV electrons lttgt 340ms
QCD jets lttgt 370ms
12
Flexibility - Robustness
  • Robustness is very important for trigger
    algorithms and is closely linked to flexibility
  • Example what if the first pixel layer of ATLAS
    dies (due to radiation)? (studied with electron
    RoIs)
  • Efficiency 96.5 gt 94.5
  • Resolution 250mm gt 400mm
  • Speed 340msec gt 230msec
  • Same algorithm can be used in widely different
    physics cases (e.g. electrons/jets), by simple
    change of parameters
  • first / last Si layer to be used
  • f bin width
  • Example
  • electron RoIs one high-pT track giving the
    z-info, so very thin f bins use all layers (
    benefit from combinatorics 7 hits give 6x7/221
    entries)
  • WH RoIs several tracks, so no need to use more
    than 3 layers

13
The hit filter a simple example
(3)
(1)
(2)
14
The hit filter in words
  • The principle
  • After finding the z position of the physics
    event, make a 2D-histogram in
    (h,f)
  • Each bin in that histo corresponds to a small
    solid angle
  • A track (above certain pT) from the physics event
    will be fully contained in one such bin, while a
    pile-up track from a different z will cross many
    bins
  • Therefore, in each bin, count how many DIFFERENT
    LAYERS have been hit. If more than N, accept all
    hits in this bin, else reject all hits in this
    bin
  • Cluster hits from neighboring bins into groups
    (very often a group contains the hits of just one
    track, i.e. this is a 1st order pattern
    recognition!)

15
Example electron RoI
16
Example QCD jet RoI
17
Performance of the hit filter
  • The efficiency depends on the curvature of tracks
    (pT, magnetic field) and the size of f bins in
    the 2D-histogram
  • In ATLAS, for f bins of 2o gt eff100 for
    pTgt2GeV/c (modulo detector inefficiencies)
  • Timing the algorithm is linear (for ATLAS
    t(ms)2.5xNhits)
  • pT40GeV/c electron RoIs lttgt 600ms

18
Summary
  • Two general algorithms to clean up the
    spacepoints of the tracking detectors at hadron
    collider experiments
  • z-finder it determines the z-position of the
    physics event
  • hit-filter once z is known, it rejects
    pile-up/noise/ghost hits
  • Both algorithms are fast / efficient / robust /
    flexible
  • Can help to prepare data for further processing,
    leading to significant reduction of
    combinatorics.
  • General enough to be usable in many physics cases
  • single isolated electron/muon track
    reconstruction
  • tracking inside hadronic jets gt b-tagging at the
    LVL2 trigger

Focusing on just the physics event at the trigger
level should give great benefits in performance!
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