time resolution of analog sipms techniques and setups
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Time resolution of analog SiPMs: techniques and setups examples Fabio Acerbi (on behalf of the ICASiPM timing group: S Gundacker, S. Brunner, A. Gola, E. Venialgo, E. Popova, T. Ganka, J.F. Pratte, M.V. Nemallapudi, S. Dolinsky, S. Vinogradov)


  1. Time resolution of analog SiPMs: techniques and setups examples Fabio Acerbi (on behalf of the ICASiPM timing group: S Gundacker, S. Brunner, A. Gola, E. Venialgo, E. Popova, T. Ganka, J.F. Pratte, M.V. Nemallapudi, S. Dolinsky, S. Vinogradov)

  2. Introduction • Among others properties, single-photon time resolution (SPTR) is an important characteristic of the SiPMs • Has been studied over the last few years by different groups employing different setups and techniques. • In this contribution  examples and comparison of meas. setups and readout methodologies used by various groups to characterize the SPTR of analog SiPM. • Discussion of some SPTR measurement related aspects such as – Type of laser, attenuation of light, uniformity of the light, reference signal, … – Identification of single photon events. – Practical considerations (TTS, amplifier, state-of-the-art values, etc.) • By examining the SPTR measurement techniques for analog SiPM  we intend to have comparable parameters for the measurements performed by groups across several fields and institutions. 13 June 2018 F. ACERBI - ICASIPM 18 - SPTR meas. with aSiPMs 2

  3. Single-photon time resolution (SPTR) ref Ref [2] Laser signal control unit D T Threshold ref signal SPTR SiPM (FWHM) signal Threshold SiPM signal • Single-photon time resolution (SPTR): • jitter in time between photon arrival on the SiPM and detection by the front-end electronics. • Measurement: 2 signals  SiPM signal & reference (sync) signal  thresholding   SPTR = spread of time difference histogramming 13 June 2018 F. ACERBI - ICASIPM 18 - SPTR meas. with aSiPMs 3

  4. SPTR: from SPAD to SiPM SPAD: aSiPM: (Array of many SPADs in parallel) SPTR depends on: SPTR depends on: • • Single- cell (SPAD) “intrinsic” time -resolution Avalanche build-up spread (highly depend on excess bias  higher E-field, faster build-up times, • Transit time skew (TTS): parasitic and length with less spread) variation of interconnections • diffusion tail • Non-uniformity between SPADs (particularly at high wavelength (e.g. gain or amplitude variation)  diffusion of carrier photogenerated (e.g. breakdown voltage variation  different local excess in neutral region) biases  overall wider timing hist., worse SPTR) • Non-uniformity • ( effect of electronic noise on th. crossing time of electric field  significantly affect measured SPTR, but it is not a in the active area characteristic of the detector ) 𝐾𝑗𝑢𝑢𝑓𝑠 𝑜𝑝𝑗𝑡𝑓 = 𝑊 𝑜𝑝𝑗𝑡𝑓 See ref [1] 𝑒𝑊 𝑒𝑢 ൗ and ref [2] 13 June 2018 F. ACERBI - ICASIPM 18 - SPTR meas. with aSiPMs 4

  5. Measured SPTR: contributing factors 𝑇𝑄𝑈𝑆 𝑛𝑓𝑏𝑡 = 𝑇𝑄𝑈𝑆 𝑞ℎ𝑝𝑢𝑝𝑡𝑓𝑜𝑡𝑝𝑠  𝐾𝑗𝑢𝑢𝑓𝑠 𝑜𝑝𝑗𝑡𝑓  𝐾𝑗𝑢𝑢𝑓𝑠 𝑡𝑓𝑢𝑣𝑞  Laser_PW  𝐾𝑗𝑢𝑢𝑓𝑠 𝑢𝑠𝑗𝑕𝑕𝑓𝑠 𝐾𝑗𝑢𝑢𝑓𝑠 𝑜𝑝𝑗𝑡𝑓 = 𝑊 𝑜𝑝𝑗𝑡𝑓 LASER contributions: 𝑒𝑊 𝑒𝑢 - optical Pulse Width (PW) ൗ - Electronic-to-optical signal jitter 𝑇𝑄𝑈𝑆 𝑞ℎ𝑝𝑢𝑝𝑡𝑓𝑜𝑡𝑝𝑠 = 𝑇𝑄𝑈𝑆 𝑇𝑄𝐵𝐸(𝑗𝑜𝑢𝑠𝑗𝑜𝑡𝑗𝑑)  𝑈𝑈𝑇  𝑇𝑞𝑏𝑒_𝑢𝑝_𝑇𝑞𝑏𝑒_𝑊𝑏𝑠𝑗𝑏𝑢𝑗𝑝𝑜 SPTR ( l ,V EX ,V th ) 𝑢ℎ )  𝑒𝑗𝑔𝑔𝑣𝑡𝑗𝑝𝑜_𝑢𝑏𝑗𝑚(𝜇)  𝐾𝑗𝑢𝑢𝑓𝑠 𝐹𝑔𝑗𝑓𝑚𝑒_𝑣𝑜𝑗𝑔. (𝑊 𝑇𝑄𝑈𝑆 𝑇𝑄𝐵𝐸 𝑗𝑜𝑢𝑠𝑗𝑜𝑡𝑗𝑑 = 𝐾𝑗𝑢𝑢𝑓𝑠 𝑐𝑣𝑗𝑚𝑒−𝑣𝑞 (𝑊 𝑓𝑦 , 𝑊 𝑓𝑦 ) • The actual SPTR ( l , V EX , V th ) is only the photosensor jitter (SPTR photosensor ) • setup influence, laser PW and jitter should be deconvolved from measured data. • BUT also the measured value have to be reported (since estimations and deconvolutions may be not easy, and may introduce error) • Detector SPTR  considered intrinsic to the detector • SPTR can be given with more insight (e.g. TTS, or focused-light SPTR) 13 June 2018 F. ACERBI - ICASIPM 18 - SPTR meas. with aSiPMs 5

  6. Setup for SPTR measurement front-end Pulsed signals Amplified SiPM signal laser REF (sync) signal Input: Threshold s Pulsed Amplitude SiPM laser REF (sync) signal Timing ASIC Discr. Threshold • Two commonly used techniques to measure timing: – Waveform acquisition  SiPM output is amplified, acquired directly (oscilloscope or digitizer) and the signal analyzed, appl. threshold(s), extracting timing histogram(s). – ASIC readout  the output is either a time stamp or a discriminated signal that can further be digitized by an external TDC. 13 June 2018 F. ACERBI - ICASIPM 18 - SPTR meas. with aSiPMs 6

  7. Important: photon number discrimination Single-photon time resolution  only single photon events ! SPAD (or PMT) SiPM FBK 1x1mm 2 SiPM Th.SiPM www.picoquant.com Ref signal 1 photon Th.ref events SiPM signal 8.9 mV/div 2.0 ns/div D T • For SiPMs  timing histogram & statistics • For SPAD (or PMT)  necessary and altered by 2ph, 3ph, etc. events. sufficient to operate at <5% rate (of laser rep-rate) • Important to consider only 1-ph events.  prob. 2ph triggering same cell negligible • Even if trig rate < 5% (single photon level) optical CT is present. 13 June 2018 F. ACERBI - ICASIPM 18 - SPTR meas. with aSiPMs 7

  8. Important: photon number discrimination FBK 1x1mm 2 SiPM (see ref[3]) Gauss fit Without photon num. discrimination : “irregular” timing histogram shapes, Norm. counts dependent on mean number of photons. lower intensity higher intensity Time 8 13 June 2018 F. ACERBI - ICASIPM 18 - SPTR meas. with aSiPMs

  9. SPTR dependences of aSiPM FBK 1x1mm 2 SiPM (see ref[3]) Excess bias: 8.9 mV/div 2.0 ns/div FBK SiPM 1x1 mm 2 Low threshold: triggering High thresholds: Good (intermediate) on electronic noise and lower signal slope thresholds : baseline fluctuations and sensitive to good signal slope amplitude variations 13 June 2018 F. ACERBI - ICASIPM 18 - SPTR meas. with aSiPMs 9

  10. SPTR dependences of aSiPM ref [4] Excess bias: SPTR values ref [4] FBK SiPM Ref [3] 1x1 mm 2 • Measured SPTR value is highly affected by: – the choice of the excess bias Very important to – the voltage discriminating threshold (on SiPM signal) specify the values – Laser wavelength (diffusion tail) used in the measurement ! – Temperature (e.g. DCR influence on SPTR meas , or second order effects.) – Repetition rate of laser (dead time?) – Front-end circuit (input capacitance) 13 June 2018 F. ACERBI - ICASIPM 18 - SPTR meas. with aSiPMs 10

  11. SPTR: state of the art results FBK SiPMs: single cell, 1x1 mm 2 , 3x3 mm 2 Ref [5] Several different SiPMs - tested with NINO ASIC FBK RGB 50µm single cell: SPTR=50 ps FWHM FBK RGB 1x1mm 2 (50µm cell): SPTR=75 ps FWHM FBK RGB 3x3mm 2 (50µm cell): SPTR=180 ps FWHM Ref [3] FBK SiPMs: 1x1 mm 2 std and HD technology Recent results: 3x3 mm 2 SiPMs - with NEW Capacitance compensation circuit FBK NUV 3x3mm 2 (40µm cell) NINO ASIC: SPTR=175ps FWHM new circuit: SPTR=100ps FWHM HPK 3x3mm 2 (50µm cell): NINO ASIC: SPTR=220ps FWHM new circuit: SPTR=144ps FWHM Ref [7] Ref [12] SensL-J 3x3mm 2 (35µm cell): NINO ASIC: SPTR=290ps FWHM new circuit: SPTR=150ps FWHM FBK single SPADs (square and circular) SiPMs 3x3 mm 2 SiPMs 1x1 mm 2 or 1.3x1.3 mm 2 Ref [11] Ref [8] ~60 ÷ 70 ps 13 June 2018 F. ACERBI - ICASIPM 18 - SPTR meas. with aSiPMs 11

  12. Practical considerations Laser ? Laser type Producer Model Pulse width Rep rate Cost Features range • Picoquant Picosecond 40-100 ps * Adjustable Electrical trig-out available (but Pulsed (e.g. 1Hz ÷100MHz) few tens ps jitter ?) • Semiconductor Sources Several different laser heads + (different l ) lasers ALS PiL XXX 40-80 ps * From pulse-on-demand up • Secondary peaks or tails ** to 120 MHz • Compact, fiber coupled. • Spectra Mai Tai ~100 fs 80 MHz High stability, short pulses • physics Tunable wavelength, limited range (e.g. 690 – 1040 nm) Pulse Oscillators +++ Coherent Vitara < 20 fs 80 MHz • Accessories: pulse picker, SHG, etc. • Bulky, typ. Free space. • Toptica FemtoFErb ~ 90 fs 100 MHz Chirped very short pulses • 780 Fiber coupled, compact Femtosecond ++ • Only 1 wavelength, (plus SHG) Fiber Lasers 50 – 100 MHz MENLO ELMO 780 < 100 fs In this table only very few examples reported – with the only purpose of comparing the general features of the different types of laser solutions. Data taken from the relative website. * From general description of product or considering only the visible range ** See plot below. www.picoquant.com 13 June 2018 F. ACERBI - ICASIPM 18 - SPTR meas. with aSiPMs 12

  13. Practical considerations Laser ref. signal 1) With electrical trigger out signal from laser 2) With reference signal from secondary detector • Reference signal: – Electrical-optical jitter can be an issue (up to few tens of picoseconds) – maybe not relevant when measuring SPTR of 100ps, or when laser PW is ~70ps, but can be eliminated using reference signal from secondary detector . (with much higher light intensity, to decrease the jitter to the minimum). 13 June 2018 F. ACERBI - ICASIPM 18 - SPTR meas. with aSiPMs 13

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