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md-NUV PET project meeting

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Presentation on theme: "md-NUV PET project meeting"— Presentation transcript:

1 md-NUV PET project meeting
Influence of SiPM Single Photon Timing Resolution on Coincidence Timing Resolution with Fast Scintillator . 1E. POPOVA, 1,2S. VINOGRADOV, 1D. PHILIPPOV, 1P. BUZHAN, 1A. STIFUTKIN, 1National Research Nuclear University «MEPhI» 2Lebedev Physical Institute RAS 18 April 2018 AQUA EPFL Microcity, Neuchatel

2 Estimate a coincidence time resolution CTR on the basis of known
For the TOF PET ( and another timing applications) we are interested to Estimate a coincidence time resolution CTR on the basis of known photodetector and scintillator parameters. Choosing of the best photodetector Choosing of the best scintillator Chosing of the best photodetector and scintillator * Photodetector – analogue SiPM The goal of our studt – to derive CTR as an analytical function of SiPM and scintillator parameters: single photon time resolution SPTR, pulse shape (single electron response, SER), PDE - SiPM trise and tdecay of scintillator, photon numbers - scintillator 2

3 Before we will talk about analytical model for the CTR,
we have to define SPTR itself Uniform light distribution over the sensitive SiPM area, selection of single photoelectron events Draft Timing group, S.Gundaker We assume that SPTRdetector is important parameter that affects CTR, however we often measure SPTR and CTR for the different electronics conditions (different noise and SER) How we can estimate electronics noise and BW influence on SPTR value in order to perform transition between the different setups? Or how we can estimate for the used electronics the SPTRdetector ?

4 Experimental study of SPTR and MPTR and analytical model for MPTR
The main idea of experiment: Instead of measuring of CTR with annihilation gammas we study MPTR by using light source with variable pulse shape and intensity 4

5 Timing measurements with KETEK SiPM+amplifiers assembly
Experimental setup: picosecond laser (405 nm, FWHM ≈ 40 ps) advanced timing optimized 3x3 mm2 KETEK SiPM chip and specially designed (by S. Ageev) and produced monolithic trans-impedance amplifier(s) (BW 1.5GHz) on PCB assembly External KETEK evaluation kit amplifier thermal chamber with light protection T=-30° C digital oscilloscope LeCroy WaveRunner 620Zi (2GHz, 20GS/s ) PMT-monitor for calibration light intensity into Npe New timing optimized SiPM SiPM + Amplifiers PCB 5

6 Digital signal processing
Linear fit of baseline Time stamp is the moment of crossing threshold with linear fit of rising edge of pulse Charge selection: only 1phe pulses (for SPTR data) LED threshold = 15 mV FWHM ≈ 1 ns DSP: time stamps (Uov = 7.5V) 1_phe pulse shape, Uov = 4.5 V 1_phe pulse shape, Uov = 9.5 V 6 6

7 SPTR measurements LED 15 mV Temperature = -30 С° 3x3 mm2 SiPM,
SPTR = 112 ps Temperature = -30 С° SPTR histogram, Uov = 9.5 V LED 15 mV 7

8 MPTR measurements In order to study MPTR dependence on SPTR we carried out two experiments (T = -30°C, Uov = 4.5V, SPTR = 147 ps): 1) Light source – laser, FWHM = 40 ps, MPTR measurements 2) Light source – laser + WLS-fiber, Tr ≈ 80 ps, Td ≈ 1.8ns, scintillator-simulated experiment 8

9 Timing resolution - analytical model (S.Vinogradov)
Filtered marked point process Analytical model “Amplitude noise” for timing resolution Number of photoelectrons Excess noise factor of SiPM (include DCR, XT, AP) Probability density function of light Probability density function of SiPM SPTR Single-electron response function (SER) Constant threshold at the first photon- no CT, no AP, no dark rate ENF≈1 9

10 Analytical model (laser light)
Gaussian shape of laser pulse and SPTR allows to get CTR dependence on SPTR: in case if SER is a Heaviside step response it has an analytical form: in case if SER is a bi-exponential with rise Tr and fall Tf times it has an analytical form: For typical SiPM pulses (Tr = ns, Tf = 1…100 ns) dependence of CTR on Tr and Tf is rather weak, so it can be approximated as:

11 MPTR experiment – short laser pulse
Analytical model: Tr = 0.5 ns, Tf = 1 ns Experimental Fit Uov = 4.5 V, T = -30 °C SPTR Laser trigger electronic jitter? (not include in model) 11

12 Experiment MPTR with laser+WLS-fiber
MPTR histograms (Tr ≈ 80ps, Td ≈ 1.9ns) : top – Npe ≈ bottom – Npe ≈ 52.3 Experimental Fit MPTR FWHM, ps (CTR with scintillator simulation) vs Light intensity Uov = 4.5 V, T = -30 12

13 Analytical model calculations: MPTR as function of SPTR
for scintillator-simulated pulse Npe = 100 Npe = 10 Npe = 1 Npe = 100, Td = 1.8 ns Npe = 100, Td = 18 ns MPTR has regions with different dependence on SPTR Kind of plateau for smaller SPTR value is connected with WLS rise time (80 ps) 13

14 Summary PCB assembly of 3x3 mm2 KETEK SiPM with amplifier was measured, SPTR of 112 ps was achieved (9.5V OV, -30 °C). The multi-photon timing measurements with different pulse shapes were carried out to show how coincidence timing resolution depends on SPTR. Analytical model of “Amplitude noise” has a good agreement with experiment results for light intensity Npe > 1. MPTR for short light pulse may allow to extract true SPTRdetector (not affected by noise) – should be checked Analytical model shows how MPTR depends on SPTR for long scintillator-like pulses, but it should be checked with more experimental data. 14

15 BACKUP 15

16 Timing measurements with new PCB – multi-photon TR results
N, pixel SPTR, ps 0.168 163 0.288 185.5 0.549 204 1.072 217 1.932 144 3.585 111 7.353 85 12.6 66 39 36.6 59 32.6 95 29,8 112 28,8 140 27,9 212 26,1 Timing resolution vs Light intensity (in fired pixels), Uov = 4.5 V 16

17 Timing measurements with new PCB – CTR simulation experiment – results
N, pixel CTR, ps 0.18 1200 0.46 1501 0.86 1202 1.75 850 3.71 499 6.94 376 17.5 240 26.8 188 41.5 151 52.3 131 Simulated coincidence timing resolution vs Light intensity (in fired pixels), Uov = 4.5 V 17

18 Light intensity calibration: laser & laser + WLS (CTR simulation)
18

19 Analytical model: CTR as function of SPTR and other parameters
Modern analytical approaches: Monte Carlo simulations, Detection event statistics, Order statistics of photoelectron detection time, Cramer-Rao lower bound estimation. 19

20 MPTR (CTR with scintillator simulation) vs Light intensity
0.1 1 10 100 3 Experiment Model Experimental fit Number of photoelectrons per pulse Time resolution (FWHM), ps Uov = 4.5 V, T = -30 ℃ Analytical model: Tr = 0.5 ns, Tf = 1 ns Experimental Fit 20

21 Uov = 4.5 V, T = -30 ℃ Experimental Fit 21


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