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Methods of Cherenkov pattern recognitions in high multiplicity environments. D. Di Bari - University of Bari & iNFN. HMPID in the ALICE exp. at LHC pattern recognition and RICH performance charged particle ID on real events (STAR) novel developments. Pysics Motivation. - PowerPoint PPT Presentation
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D. Di BariD. Di Bari 1IV Workshop on RICH Detectors, 5-10 June 2002 Pylos, Greece
Methods of Cherenkov pattern Methods of Cherenkov pattern recognitions in high multiplicity recognitions in high multiplicity
environmentsenvironments
•HMPID in the ALICE exp. at LHC
•pattern recognition and RICH performance
•charged particle ID on real events (STAR)
•novel developments
D. Di Bari - University of Bari & iNFN
D. Di BariD. Di Bari 2IV Workshop on RICH Detectors, 5-10 June 2002 Pylos, Greece
Pysics MotivationPysics Motivation ALICEALICE is a is a multi-purposemulti-purpose experiment experiment
aim: study the properties of the Quark Gluon Plasmaaim: study the properties of the Quark Gluon Plasma
HMPIDHMPID: to identify : to identify charged particlescharged particles with high p with high pTT in the in the
central rapidity region (central rapidity region (||| < 1| < 1)) 1 < p1 < pTT < 3 GeV/c < 3 GeV/c //KK
1.5 < p1.5 < pTT < 6 GeV/c < 6 GeV/c pp
Sub-detectors designed for Pb-Pb collisions at Sub-detectors designed for Pb-Pb collisions at s=5.5 s=5.5 TeVA with anticipated multiplicity TeVA with anticipated multiplicity dN/dy dN/dy ~ ~ 80008000
10-15% pad occupancy for RICH (80-100 part/m10-15% pad occupancy for RICH (80-100 part/m22))
D. Di BariD. Di Bari 3IV Workshop on RICH Detectors, 5-10 June 2002 Pylos, Greece
D. Di BariD. Di Bari 4IV Workshop on RICH Detectors, 5-10 June 2002 Pylos, Greece
Conversion of photons inConversion of photons in
CsI (QE 20% @ 170 nm)CsI (QE 20% @ 170 nm) RadiatorRadiator
CC66FF1414 Liquid Liquid Photo DetectorPhoto Detector
MWPC pad chamberMWPC pad chamber CHCH44 Gas Gas
Proximity Focusing
D. Di BariD. Di Bari 5IV Workshop on RICH Detectors, 5-10 June 2002 Pylos, Greece
GEANT 3.21 Simulation
= 1 100 rings
• Momentum from TPC• Matching between extrapolated point and MIP on the RICH
TPC
ITS
RICHtr
ack
quartzCH4
pad
pla
ne
D. Di BariD. Di Bari 6IV Workshop on RICH Detectors, 5-10 June 2002 Pylos, Greece
Detector responseDetector response
MIP
photons
coscoscc = 1/n = 1/n
Npad (MIP) 56
Npad (photons) 2
MWPC HV = 2100 Voperated with CH4
• raw photon clusters/ring = 14.8• res. photon clusters/ring = 16.2
D. Di BariD. Di Bari 7IV Workshop on RICH Detectors, 5-10 June 2002 Pylos, Greece
Simulation with ALIROOT (C++)
D. Di BariD. Di Bari 8IV Workshop on RICH Detectors, 5-10 June 2002 Pylos, Greece
Pattern recognition in Pattern recognition in ALICEALICE
TheThe Hough Transform MethodHough Transform Method ( (HTMHTM) represents an ) represents an efficient efficient implementation of a generalized implementation of a generalized template matchingtemplate matching strategy for strategy for detecting complex patterns in binary images (looking for detecting complex patterns in binary images (looking for local local
maximamaxima in a in a feature parameterfeature parameter space) space)
cluster coordinate
impact track parameter
solution in one dimensional
mapping space c
photon Cerenkov
angle
(x,y) ((xp,yp,p,p), c)
D. Di BariD. Di Bari 9IV Workshop on RICH Detectors, 5-10 June 2002 Pylos, Greece
c = reconstructed theta Cherenkov for each photon
c = reconstructed theta Cherenkov per particle
geometrical backtracing = reconstruction of the angle under which the “candidate” photon could have been emitted
quartz window
C6F14
CH4
MIP
photon cluster
proximity gapradiator
incomingparticle
D. Di BariD. Di Bari 10IV Workshop on RICH Detectors, 5-10 June 2002 Pylos, Greece
background estimatebackground estimate hypotesis hypotesis background background uniformly distrib.uniformly distrib.
the photons falling in opening bands of 10 mrad are the photons falling in opening bands of 10 mrad are weighted weighted for the corresponding band areafor the corresponding band area
simulation
pions in saturation( = 1)
MIP
calculated area
weight = 1/area
D. Di BariD. Di Bari 11IV Workshop on RICH Detectors, 5-10 June 2002 Pylos, Greece
0
12-1
Nend-Nstar
Improvement of (Improvement of (tracktrack,,tracktrack)) after having determined the photon candidates, a after having determined the photon candidates, a
minimizationminimization of the of the rms/rms/NN of the photon distr. has been of the photon distr. has been performed with (performed with (tracktrack,,tracktrack) as ) as free parametersfree parameters
with the new fitted with the new fitted tracktrack,,track track the Hough transform is the Hough transform is
again again applied applied
stop if the # stop if the # photons remains photons remains
the same !the same !
tracktrack
end start
D. Di BariD. Di Bari 12IV Workshop on RICH Detectors, 5-10 June 2002 Pylos, Greece
...at the end of the iteration
photon included after the (photon included after the (tracktracktracktrack) correction) correction
D. Di BariD. Di Bari 13IV Workshop on RICH Detectors, 5-10 June 2002 Pylos, Greece
Efficiency and Efficiency and contaminationcontamination
Efficiency and contamination as a function of the track momentum (dN/dy = 8000)
D. Di BariD. Di Bari 14IV Workshop on RICH Detectors, 5-10 June 2002 Pylos, Greece
installation of the proto-2 in the STAR experiment: unique opportunity to test the detector 5(?) years before the ALICE start
installation of the proto-2 in the STAR experiment: unique opportunity to test the detector 5(?) years before the ALICE start
D. Di BariD. Di Bari 15IV Workshop on RICH Detectors, 5-10 June 2002 Pylos, Greece
positives+
negatives
Reconstructed Theta Cherenkov vs. Reconstructed Theta Cherenkov vs. track momentum in STARtrack momentum in STAR
pth 1.26 m GeV/c
D. Di BariD. Di Bari 16IV Workshop on RICH Detectors, 5-10 June 2002 Pylos, Greece
Sample of events with track of p Sample of events with track of p >1GeV/c>1GeV/c
|| < 0.15
p
K
physics analysis
D. Di BariD. Di Bari 17IV Workshop on RICH Detectors, 5-10 June 2002 Pylos, Greece
2 < pt < 2.5 GeV/c
protons
poissonian distrib.
Evaluation of NEvaluation of Nsatsat
sin2c
sin2c,sat
= 0.677
Nsat = 5.6/0.677 Nsat = 5.6/0.677 = 8.5 = 8.5
Theta Cherenkov (rad)
clu
ste
r m
ult
iplicit
y
Nph = 9
Nph = 15 @ CERN test beam (in 2000 data lower gain)
D. Di BariD. Di Bari 18IV Workshop on RICH Detectors, 5-10 June 2002 Pylos, Greece
Tuning of the n(Tuning of the n(,T) ,T) m
ass
(G
eV
)
momentum (GeV/c)
n/T -0.0005 / ºC
momentum (GeV/c)
mass
(G
eV
)
m = PTPC/(RICHpions
kaonsprotons
p > 1 GeV
D. Di BariD. Di Bari 19IV Workshop on RICH Detectors, 5-10 June 2002 Pylos, Greece
Fitted peak positions for /K/pin agreement with the expected
Cherenkov vs. pt curves
/K and K/p separation as function of pt
D. Di BariD. Di Bari 20IV Workshop on RICH Detectors, 5-10 June 2002 Pylos, Greece
pK-
K+
p
positives
negatives
The signal of , and p could be extracted by
fitting the distribution of reconstructed Cherenkov in
different pT ranges
Signal extractionSignal extraction
D. Di BariD. Di Bari 21IV Workshop on RICH Detectors, 5-10 June 2002 Pylos, Greece
Charged particle ratios Charged particle ratios with RICH in STARwith RICH in STAR
not corrected for •acceptance•efficiency
D. Di BariD. Di Bari 22IV Workshop on RICH Detectors, 5-10 June 2002 Pylos, Greece
candidatescandidates identifiedidentified efficiencyefficiency(%)(%)
err (%)err (%)
protonsprotons 157157 126126 80.380.3 3.23.2
antiprotonsantiprotons 8181 6464 79.079.0 4.54.5
Proton Identification Proton Identification efficiencyefficiency
(Anti)Proton identification efficiency has been evaluated by the identification of the (anti) protons coming from the charged dacay of (anti)lambda
p -
overall efficiency in the range 1.5 < pT < 2.5 GeV/c
D. Di BariD. Di Bari 23IV Workshop on RICH Detectors, 5-10 June 2002 Pylos, Greece
SVMSVM is a is a newnew (1995) and promising (1995) and promising classification technique with high classification technique with high generalization power.generalization power.
It is particularly apts with complex images. It is particularly apts with complex images. Basic idea: separate the classes with a Basic idea: separate the classes with a surface that surface that maximizesmaximizes the margin between the margin between them and them and minimizeminimize the error in the the error in the misclassification of data.misclassification of data.
Support Vector Support Vector MachinesMachines
References:
1) E.E. Osuna, R. Freud, F. Girosi, Support Vector Machines: Training end Applications MIT, (1997).
2) M. Feindt, C. Haag, DELPHI Collaboration, Support Vector Machines for Classification Problems in High Energy Physics, Institute fur experimentelle Kernphysik, Universitat Karlsruhe, (1999).
3) L. Maglietta, “Support vector machines for electron/antiproton discrimination by a transition radiation detector” (Pamela exp.), Università degli Studi di Bari, Thesis Degree, march 2002.
RICH Classification problem: pions/kaons/protons discrimination.
Input space: photon Cherenkov angles.
Output space: class membership probability.