Light High Precision CMOS Pixel Devices Providing 0(µs) Timestamping for Future Vertex Detectors
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1 Light High Precision CMOS Pixel Devices Providing 0(µs) Timestamping for Future Vertex Detectors M. Winter, on behalf of PICSEL team of IPHC-Strasbourg IEEE/NSS-MIC - Anaheim(CA) Novembre 2012 Contents Reminder: main features of CMOS sensors Architecture developped - state of the art MIMOSA-28 (STAR-PXL, AIDA) Extension towards more demanding experiments speed, radiation tolerance ALICE-ITS (& -MFT) CBM-MVD ILD-VXD SuperB-SVT First test results of a 0.18 µm CMOS technology charged particle detection perfo. for deep P-well & elongated pixels radiation load & T dependence Summary 1
2 CMOS Pixel Sensors: Main Features Prominent features of CMOS pixel sensors: high granularity excellent (micronic) spatial resolution very thin (signal generated in µm thin epitaxial layer) signal processing µ-circuits integrated on sensor substrate impact on downstream electronics and syst. integration ( cost) CMOS pixel sensor technology has the highest potential R&D largely consists in trying to exploit potential at best with accessible industrial processes manufaturing param. not optimised for part. detection: epitaxy characteristics, feature size, N(ML),... Organisation of MIMOSA sensors: manufactured in 0.35 µm OPTO process (until recently) signal sensing and analog processing in pixel array mixed and digital circuitry integrated in chip periphery read-out in rolling shutter mode (pixels grouped in columns read out in //) impact on power consumption 2
3 State-of-the-Art: MIMOSA-28 for the STAR-PXL Main characteristics of ULTIMATE ( MIMOSA-28): 0.35 µm process with high-resistivity epitaxial layer column // architecture with in-pixel cds & amplification end-of-column discrimination & binary charge encoding on-chip zero-suppression active area: 960 colums of 928 pixels ( mm 2 ) pitch: 20.7 µm 0.9 million pixels charge sharing σ sp 3.5 µm JTAG programmable t r.o. 200 µs ( frames/s) suited to >10 6 part./cm 2 /s 2 outputs at 160 MHz 150 mw/cm 2 power consumption Sensors fully evaluated : (50 µm thin) N 15 e ENC at C (as MIMOSA-22AHR) ǫ det, fake & σ sp as expected Rad. tol. validated ( n eq /cm 2 & 150 krad at 30 C) All specifications are met 40 ladders under construction Start of data taking early
4 4
5 Towards Higher Read-Out Speed and Radiation Tolerance Next generation of experiments calls for improved sensor performances : Expt-System σ t σ sp TID Fluence T op STAR-PXL 200 µs 5 µm 150 krad n eq /cm 2 30 C??? ALICE-ITS µs 5 µm 700 krad n eq /cm 2 30 C CBM-MVD µs 5 µm 10 MRad n eq /cm 2 0 C ILD-VXD 10 µs 3 µm O(100) krad O(10 11 ) n eq /cm 2 30 C SuperB-SVT 2 µs 10 µm 5 MRad/yr SF n eq /cm 2 /yr SF 10 C Main improvements required to comply with forthcoming experiments specifications : aim for higher epitaxial layer resistivity reduce nb(pixels) / read-out unit (column) aim for smaller feature size process & more parallelised read-out How to accelerate the pixel read-out elongated pixels less pixels /col. & in-pixel discri. 3-8 faster r.o. read out simultaneously 2 or 4 rows 2-4 faster r.o./side subdivide pixel area in 4-8 sub-arrays read out in // 2-4 faster r.o./side conservative step: 2 discri./col. end (22 µm wide) simult. 2 row r.o. remain inside virtuous circle: spatial resol., power, flex mat. budget, µm process needed instead of currently used 0.35 µm process 5
6 MIMOSA-32 : Prototyping a 0.18 µm Process 0.18 µm imaging technology options used : Epitaxial layer: High-Resistivity (1-5 kω cm) & 18 µm thick SNR, rad. tol.,... Quadruple well: deep P-type skin embedding N-well hosting P-MOS transistors compactness, power,... MIM capacitors 6 Metal Layers etc. Prototype sub-divided in several blocks : Sensing elements and in-pixel amplifiers : pixel dimensions : 20 20/40/80 µm 2 2 different types of sensing elements : diodes of 9 15 µm 2 N-MOS and P-MOS transistor based amplifiers Discriminators : Col. // pixel array ended with 1 discriminator/col. (2 variants) Pixel array with in-pixel discriminator (16 80 µm 2 pixels) Total surface 43 mm 2 Mimosa-32 fabricated in Q4/2011 tests since April 12 6
7 MIMOSA-32 Tests Prominent test purposes : Validate epitaxial layer characteristics (behaviour) Study charge collection properties of sensing node 2T Validate technology radiation tol. for ALICE-ITS (T=30 C) Study sensing performances of elongated vs square pixels Study sensing performances of deep P-well pixels Estimate necessity of ELT design Beam tests at CERN-SPS in Summer 2012 : MIMOSA-32 chips mounted on beam telescope beams of GeV charged particles 3T test results based on 50,000 tracks reconstructed in BT and DUT effect of combined radiation load: 1 MRad n eq /cm 2 T coolant = 15 C & 30 C RESULTS ARE STILL PRELIMINARY! 7
8 Observed Charge Sensing Properties MIMOSA-32 lab tests ( 55 Fe source) of pixel matrix with analog output Read-out time of each sub-matrix = 32 µs Observed CCE (20 20 µm 2 pixels) : seed pixel : % 2 2 pixel cluster : nearly 100 % confirms Epi. layer 1-5 kω cm No parasitic charge coll. seen with Deep P-well CCE of µm 2 pixels seed 30 %; with 1st crown % Noise 20e ENC at 20 C, unchanged at 35 C Irradiation: 0.4/1/3 MRad no effect up to 35 C (tbc!) Beam tests : Deep P-well Rect. 1D Cluster multiplicity for 60 & 120 GeV charged particles Radiation 20 20µm µm 2 Load 2T 3T Deep P 1D-3T 2D-3T (1.4) (1.3) (1.2) (1.9) (1.2) 1 MRad and n eq /cm 2 (1.2) (1.1) (1.1) (1.5) (1.2) High resistivity of epitaxial layer confirmed 8 Cluster multiplicity S/N> hmult_sn_5 Entries 2639 Mean RMS Cluster multiplicity S/N> hmult_sn_5 Entries 3211 Mean RMS 1.798
9 Beam Tests of 20x20 µm 2 Deep P-Well (3T) Pixel Pros and cons of deep P-well: Pros: allows use of P-mos transistors reduced in-pixel µcircuit footprint and/or more in-pixel functionnalities Cons: potential parasitic charge collection (esp. after ionising irradiation) and increased noise Signal/Noise ratio for P9 Signal/Noise ratio for P9 Events MPV=19.29± MPV=22.6±0.4 Events Mrad+10 - MPV=19.29± MPV=22.6±0.4 REF@30C - MPV=29.7±0.4 REF@15C - MPV=30.85± REF@30C - MPV=29.7± REF@15C - MPV=30.85± Signal/Noise Signal/Noise SNR (MPV) and detection efficiency (stat. uncertainty only): Radiation SNR (MPV) Detection efficiency [%] Load 15 C 30 C 15 C 30 C ± ± ± ± MRad & n eq /cm ± ± ± ±
10 Beam tests of 20x40 µm 2 (1 Sensing Diode) Pixel Trade-off to be found for each application: read-out time reduction spatial resolution degradation NI radiation tolerance degradation (SNR ց) depends on t int, T, epitaxy, diodes (size, Nb),... Signal/Noise ratio for L4_1 Signal/Noise ratio for L4_1 Events Mrad+10 - MPV=10.94± MPV=13.34±0.31 Events MPV=10.94± MPV=13.34±0.31 REF@30C - MPV=21.76± REF@30C - MPV=21.76±0.25 REF@15C - MPV=22.6± REF@15C - MPV=22.6± Signal/Noise Signal/Noise SNR (MPV) and detection efficiency (stat. uncertainty only): Radiation SNR (MPV) Detection efficiency [%] Load 15 C 30 C 15 C 30 C ± ± ± ± MRad & n eq /cm ± ± ± ±
11 Spatial Resolution Beam test (analog) data used to simulate binary charge encoding : Apply common SNR cut on all pixels using <N> simulate effect of final sensor discriminators Evaluate single point resolution (charge sharing) and detection efficiency vs discriminator threshold for 20x20 µm 2 pixels and 20x40 µm 2 staggered pixels (1 sensing diode) Comparison of 0.18 µm technology (> 1 kω cm) with 0.35 µm technology (< 1 kω cm) (pitch values: 20.0 µm and 20.7 µm) σ bin sp 3.2 ± 0.1 µm (20X20 µm 2 ) AND 5.4 ± 0.1 µm (20X40 µm 2 ) Mimosa 28 - epi 20 um - 30 C Efficiency (%) MIMOSA 28 - epi 20 um MIMOSA 32 - REF - 15C 20x20 um^2 MIMOSA 32 - REF - 15C 20x40 um^2 PRELIMINARY Threshold / noise Resolution (µm) 11
12 SUMMARY CPS have a very high potential for high precision/low power tracking and vertexing devices 1st vertex detector based on CPS (STAR-PXL) close to commissionning CMOS industry fabrication parametres make it difficult to fully exploit this potential e.g µm technology far from optimal A newly available 0.18 µm imaging technology with thick high-resitivity epitaxial layer is being explored, which pushes the limits of state-of-the-art sensors : - match the requirements of ALICE-ITS (up to 10 m 2 pixellated tracker) Next steps : - opens possibilities for other applications: CBM-MVD, ILC-1TeV, SuperB-SVT, submission: pixel array with peripheral discri. and 2-row simultaneous r.o. zero-suppression circuitry prototype 2013 submission: Q1/Q2: pixel array with in-pixel discriminators 2-4 faster r.o. Q4: complete 1 cm 2 sensor with peripheral discri. (30 µs) full scale proto. (MISTRAL) subm. in 2014 Final goal: ASTRAL ( 10 µs) 12
13 Next Steps of 0.18µm Architecture Prototyping 1st step : MISTRAL MIMOSA FOR THE INNER SILICON TRACKER OF ALICE MIMOSA-22THR ( Upstream part of sensor) : Col. // pixel array with in-pixel ampli + pedestral subtraction (cds) Each of 128 columns ended with discriminator + 8 columns without discri. Pixel array sub-divided in sub-arrays featuring different pixel designs (22 22/33 µm 2 ) 2 options submission in Decembre 12 : sgle end of column discriminator translation of MIMOSA-22AHR (0.35 techno.) simultaneous 2-row encoding & 2 discriminators/column twice faster AROM-1 (Accelerated Read-Out Mimosa) ASTRAL (2nd step) in-pixel discri. & simultaneous 4-row encoding 8 times faster than MIMOSA-22THR submission of 1st prototype in Q1-Q2/2013 SUZE-02 ( Downstream part of sensor) : Ø µ-circuits & output buffers (extension of SUZE-01 with 4 rows simult. encoding) encode windows of 4 rows 5 columns signal transmission at 320 MHz/cm submission in Decembre 12 13
14 R&D Plans towards Final Sensor FSBB (Full Scale Basic Block) : combining upstream and downstream chain elements Composition: Pixel array with final pixel design ( 1 cm 2 ) Final r.o. circuitry (Ø, filtering, data transmission,...) Variants: ALICE baseline (MISTRAL): 30 µs, µm 2 pixels, subm. Q4/2013 ALICE fast sensor (ASTRAL): 15 µs (can be < 4 µs), same pixels, subm. Q4/2015 AIDA-BT:??? Final sensors for ALICE, CBM, AIDA,...: Composition : 3 adjacent FSBB (1-sided read-out) or 2 rows of 3 FSBB (stitching, 2-sided r.o.) Complemented with serial r.o. circuitry Submissions: MISTRAL: 30 µs (15µs possible), subm. Q4/2014 ASTRAL: 15 µs ( 2 µs possible) subm. Q4/2016 AIDA-BT: subm (?) 14
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