12 th CBM Collaboration Meeting October 13-18, 2008, JINR, Dubna
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Transcript of 12 th CBM Collaboration Meeting October 13-18, 2008, JINR, Dubna
12th CBM Collaboration MeetingOctober 13-18, 2008, JINR, Dubna
A. Zinchenko1
(L.Naumann2, D.Peshekhonov1, V.Peshekhonov1) 1VBLHEP, JINR, Dubna
2Forschungszentrum Dresden-Rossendorf, FZD
Feasibility study of the straw tube detector option for some MUCH
stations
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1. MC
2. Reconstruction
3. Some performance numbers
4. Summary and outlook
Outline
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Tube diameters: 4, 4, 4, 4 mm; σdrift = 0.2 mm6 layers per station arranged in 3 doublets: Y, U (+10o), V(-10o)
Geometry
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Straw tube occupancy for Au-Au @ 25 GeV
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Straw tube occupancy for Au-Au @ 25 GeV
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Makes use of L1 Kalman Filter framework (CbmL1SttTrackFinder)
Starts from STS tracks
Tracking strategy: extrapolate track to STT plane and select hits around track with χ2 < 20 (100)
Track accepted if contains hits from all STT doublets
Track reconstruction
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Reference tracks: muon tracks from J/ψ found in STS and passing through all layers of STT (producing STT MC points with given MC track ID)
Tracking efficiency
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J/ψ to dimuon @ 25 GeV w/out background
1165 / 1185 = 98.3 %
1166 / 1194 = 97.7 %
1165 / 1185 = 98.3 %
1166 / 1194 = 97.7 %
100
1106 / 1185 = 93.3 %
1113 / 1194 = 93.2 %
1113 / 1185 = 93.9 %
1118 / 1194 = 93.6 %
20
4 stations (hit merging)
3 stations (hit merging)
4 stations3 stationsχ2-cut
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J/ψ to dimuon + central Au-Au @ 25 GeV
1157 / 1183 = 97.8 %
1162 / 1195 = 97.2 %
1160 / 1183 = 98.1 %
1162 / 1195 = 97.2 %
100
1063 / 1183 = 89.9 %
1110 / 1195 = 92.9 %
1107 / 1183 = 93.6 %
1120 / 1195 = 93.7 %
20
4 stations (hit merging)
3 stations (hit merging)
4 stations3 stationsχ2-cut
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• STT occupancy inside MUCH is below 10% in stations 4-6 for central Au-Au for 25 GeV/c
• first track reconstruction results from STS seeds (without MUCH tracking) look promising both for 3 and 4 STT stations
Summary
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• realistic STT geometry
• STT software
• performance with MUCH tracks
Outlook