Presentation is loading. Please wait.

Presentation is loading. Please wait.

Scintillation Detectors in High Energy Physics

Similar presentations


Presentation on theme: "Scintillation Detectors in High Energy Physics"— Presentation transcript:

1 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

2 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

3 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

4 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

5 Properties of Organic Scintillators
Used in large area detection requirement: Sampling EM component in air showers, Hadron Calorimeter, Muon time tagging in accelerator experiment

6 Scintillation Light Transport
Scintillation light comes out from all surfaces …..Needs to be navigated to photodetector GRAPES3 Scintillator

7 Light transport in fibers

8 Scintillating fiber tracker
UA2 experiment

9 Detection of scintillation photon (photo detector)
Photo electron Photo sensitive material (photocathod) Epe = Eγ - W

10

11 Quantum Efficiency of Photo cathode

12 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

13 PMT Signal Resolution GRAPES3 PMT

14 Photo Detectors

15 Hybrid Photo Diode HPDs are used in CMS experiment for HCAL detector

16 Si-Photo Multiplier

17 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

18 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

19 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

20 Shashi Dugad, WAPP, Ooty, 18 Dec 2012
IV Characteristic of SiPM Shashi Dugad, WAPP, Ooty, 18 Dec 2012

21 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

22 Shashi Dugad, WAPP, Ooty, 18 Dec 2012
Noise Rate and LED Response Shashi Dugad, WAPP, Ooty, 18 Dec 2012

23 Shashi Dugad, WAPP, Ooty, 18 Dec 2012
LED Test Results for Pixel 01 Shashi Dugad, WAPP, Ooty, 18 Dec 2012

24 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

25 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

26 Shashi Dugad, WAPP, Ooty, 18 Dec 2012
CMS Detector HF HO HB HE Shashi Dugad, WAPP, Ooty, 18 Dec 2012

27 Shashi Dugad, WAPP, Ooty, 18 Dec 2012
TB2009: HB Setup Shashi Dugad, WAPP, Ooty, 18 Dec 2012

28 Shashi Dugad, WAPP, Ooty, 18 Dec 2012
Application of SiPM in CMS Detector Fibers from Scintillator tiles Shashi Dugad, WAPP, Ooty, 18 Dec 2012

29 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

30 Shashi Dugad, WAPP, Ooty, 18 Dec 2012
SiPM Control Board 160 boards fabricated indigenously by GRAPES3, Ooty Shashi Dugad, WAPP, Ooty, 18 Dec 2012

31 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

32 HO Calibration with 150 GeV Muons
Shashi Dugad, WAPP, Ooty, 18 Dec 2012

33 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

34 Zecotek response to 300 GeV Pions in HO at Eta=7 Phi=4
Shashi Dugad, WAPP, Ooty, 18 Dec 2012

35 Zecotek/Hamamatsu response to 300 GeV Pions in HO at Eta=7
Shashi Dugad, WAPP, Ooty, 18 Dec 2012

36 Shashi Dugad, WAPP, Ooty, 18 Dec 2012
Relative Weight Factor for HB/HO Shashi Dugad, WAPP, Ooty, 18 Dec 2012

37 Shashi Dugad, WAPP, Ooty, 18 Dec 2012
Resolution of HB+HO O Shashi Dugad, WAPP, Ooty, 18 Dec 2012

38 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


Download ppt "Scintillation Detectors in High Energy Physics"

Similar presentations


Ads by Google