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Scintillation Detectors in High Energy Physics
Shashikant R. Dugad Tata Institute of Fundamental Research Ref. Summer Student Lecture Series 2001, by C. Joram at CERN
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Scintillators Fast Light Emitting Medium on passage of charged particle Inorganic Scintillators (Slow Response, high light o/p) Organics Scintillators (Fast Response, low light o/p) Analog Signal
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Inorganic Scintillators
Temp. dependent light o/p Inorganic Scintillators are costly and mostly used in Nuclear Physics Experiments Response time varies from ~ nsec PbWO4 is used to make calorimeter to measure energy of e+e- γ
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Organic Scintillators
Monocrystals: napthalene, anthracene, p-terephenyle Liquid and plastic scintillators: Composed of solvent + dopent (popup) used as wavelength shifter (from UV to visible) Organic scintillators are cheap and have fast response (~ few nsec) Made and used in Ooty-GRAPES3 experiment
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Properties of Organic Scintillators
Used in large area detection requirement: Sampling EM component in air showers, Hadron Calorimeter, Muon time tagging in accelerator experiment
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Scintillation Light Transport
Scintillation light comes out from all surfaces …..Needs to be navigated to photodetector GRAPES3 Scintillator
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Light transport in fibers
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Scintillating fiber tracker
UA2 experiment
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Detection of scintillation photon (photo detector)
Photo electron Photo sensitive material (photocathod) Epe = Eγ - W
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Quantum Efficiency of Photo cathode
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Estimation of Signal Strength
Charged particle passes through 1cm thick scintillator Total Energy loss by ionisation ~ 2MeV Number of scintillation photons produced ~ (λ~ nm) Number of photons captured by WLS fiber ~ 200 Number of photo electrons produced at photo cathode ~ 20 Total number of electrons at PMT last dynode (i/p of preamp) ~ 108 Typical S/B Ratio ~ 10
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PMT Signal Resolution GRAPES3 PMT
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Photo Detectors
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Hybrid Photo Diode HPDs are used in CMS experiment for HCAL detector
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Si-Photo Multiplier
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Applications μ Muon Bunch Crossing Tagging in D0 experiment p p
Scintillator Tracker (Gas Detector) p p Tracker (Gas Detector) Scintillator Muon Bunch Crossing Tagging in D0 experiment
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Shashi Dugad, WAPP, Ooty, 18 Dec 2012
SiPM Response to Muons SiPM Make SiPM Size (mm) Pixel Size (μ) # of pixels a) CPTA1 b) CPTA2 c) IRST(FBK) d) Hamamatsu 2.1 x 2.1 2.8 dia 3.0 x 3.0 50 1800 2400 3600 Shashi Dugad, WAPP, Ooty, 18 Dec 2012
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Silicon Photomultiplier
Characterization I-V characteristics Single pixel calibration Linearity, MIP sensitivity Micron resolution optical scanner for studying pixel-to-pixel response Shashi Dugad, WAPP, Ooty, 18 Dec 2012
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Shashi Dugad, WAPP, Ooty, 18 Dec 2012
IV Characteristic of SiPM Shashi Dugad, WAPP, Ooty, 18 Dec 2012
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Shashi Dugad, WAPP, Ooty, 18 Dec 2012
LED Calibration Setup Signal Generator LED SiPM Signal Trigger qADC VME Crate Computer Data Shashi Dugad, WAPP, Ooty, 18 Dec 2012
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Shashi Dugad, WAPP, Ooty, 18 Dec 2012
Noise Rate and LED Response Shashi Dugad, WAPP, Ooty, 18 Dec 2012
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Shashi Dugad, WAPP, Ooty, 18 Dec 2012
LED Test Results for Pixel 01 Shashi Dugad, WAPP, Ooty, 18 Dec 2012
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Shashi Dugad, WAPP, Ooty, 18 Dec 2012
MIPs with SiPM at Ooty WLS Fibers laid on scintillator (25 x 25 cm2) terminated onto Hamamatsu SiPM MIP signal with 44 p.e. at peak is seen (high Q.E.) Shashi Dugad, WAPP, Ooty, 18 Dec 2012
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Temperature Dependence of the Gain
Cosmic muon data taken over period of 2 days Temp. variation of 4OC Data binned in temp. slice of 0.25OC MIP peak obtained for each set plotted as function of temp. Shashi Dugad, WAPP, Ooty, 18 Dec 2012
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Shashi Dugad, WAPP, Ooty, 18 Dec 2012
CMS Detector HF HO HB HE Shashi Dugad, WAPP, Ooty, 18 Dec 2012
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Shashi Dugad, WAPP, Ooty, 18 Dec 2012
TB2009: HB Setup Shashi Dugad, WAPP, Ooty, 18 Dec 2012
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Shashi Dugad, WAPP, Ooty, 18 Dec 2012
Application of SiPM in CMS Detector Fibers from Scintillator tiles Shashi Dugad, WAPP, Ooty, 18 Dec 2012
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Shashi Dugad, WAPP, Ooty, 18 Dec 2012
HPD and SiPM Response Muons with HPD 50 GeV Discharge in HPD S/B~2 SiPM in Magnetic Field Muons with SiPM S/B~15 Shashi Dugad, WAPP, Ooty, 18 Dec 2012
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Shashi Dugad, WAPP, Ooty, 18 Dec 2012
SiPM Control Board 160 boards fabricated indigenously by GRAPES3, Ooty Shashi Dugad, WAPP, Ooty, 18 Dec 2012
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Shashi Dugad, WAPP, Ooty, 18 Dec 2012
Data Set Muon Beam at 150 GeV Beam Direction(η, φ) Pion-Beam Energy 7,3 300 GeV 225 GeV 150 GeV 100 GeV 50 GeV 30 GeV 7,4 8,3 8,4 150K events (ped+pion) events at each energy and position Shashi Dugad, WAPP, Ooty, 18 Dec 2012
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HO Calibration with 150 GeV Muons
Shashi Dugad, WAPP, Ooty, 18 Dec 2012
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Analysis procedure …contd
Subtract pedestal from signal and normalise by with muon calibration constant Number of MIPS nMIPs Take nMIPs(i) sum for all 9 towers at each depth of HB and HO Pion Energy = Constant*[A*nMIPs(1) + B*nMIPs(2) + C*nMIPs(3) + D*nMIPs(4) + E*nMIPsHO] Natural Relative Weights: A=0 B=C=1 D=6 E ~ 3.1 Estimation of Weights Pion data at 300 GeV at eta=7 and phi=3 used to estimate weights for each depth of HB and one layer of HO Vary one of the weights by fixing other weights to natural values and obtain RMS/Mean as function of that weight EGeV=0.247*(1.05*nMIPs(2) *nMIPs(3) *nMIPs(4) *nMIPsHO) Shashi Dugad, WAPP, Ooty, 18 Dec 2012
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Zecotek response to 300 GeV Pions in HO at Eta=7 Phi=4
Shashi Dugad, WAPP, Ooty, 18 Dec 2012
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Zecotek/Hamamatsu response to 300 GeV Pions in HO at Eta=7
Shashi Dugad, WAPP, Ooty, 18 Dec 2012
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Shashi Dugad, WAPP, Ooty, 18 Dec 2012
Relative Weight Factor for HB/HO Shashi Dugad, WAPP, Ooty, 18 Dec 2012
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Shashi Dugad, WAPP, Ooty, 18 Dec 2012
Resolution of HB+HO O Shashi Dugad, WAPP, Ooty, 18 Dec 2012
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Shashi Dugad, WAPP, Ooty, 18 Dec 2012
Summary SiPM is photo-readout element of 21st century Being used in large high energy physics experiments GRAPES-3 collaboration have completed HO-upgrade (~2800 channels) for CMS experiment Potential candidate in medical industry for imaging Several groups within country are working on this device Shashi Dugad, WAPP, Ooty, 18 Dec 2012
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