Development of CMOS pixel sensors for tracking and vertexing in high energy physics experiments

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PICSEL group Development of CMOS pixel sensors for tracking and vertexing in high energy physics experiments Serhiy Senyukov (IPHC-CNRS Strasbourg) on behalf of the PICSEL group 7th October 2013 IPRD13, 7-10 October 2013, Siena, Italy 1

Outline CMOS Pixel Sensors (CPS): Principle of operation Advantages vs. limitations State of the art Future projects Current developments in IPHC Prototype test results (preliminary) Conclusions & outlook 7th October 2013 IPRD13, 7-10 October 2013, Siena, Italy 2

CPS principle of operation, advantages vs. limitations Sensitive volume and readout chain in a single silicon die: High granularity (pitch ~ 20 µm) Low material budget (50 µm of Si ~ 0.3% X 0 per layer) Low production cost (large scale commercial providers and no bump bonding needed) Optimal choice for the low-p T tracking and vertexing (i.e. heavy flavors) Radiation hardness and readout speed are determined by the CMOS process parameters i.e.: feature size TID hardness epi-layer resistivity NIEL hardness Sensitive layer substrate 20 µm ~50 µm 7th October 2013 IPRD13, 7-10 October 2013, Siena, Italy 3

State of the art: Ultimate-2 for STAR-PXL First CPS in the HEP experiment: AMS 0.35 µm process Pixel pitch: 20.7 µm (960 928 pixels) Rolling shutter readout Integration time: < 200 µs TID: 150 krad NIEL: 3 10 12 n eq /cm 2 @ 35 C Chip thickness: 50 µm 0.37 % X 0 per layer 3 out of 10 sectors installed on 8 th May 2013 Commissioning with pp and light ion collisions in May June 2013. More details in the talk by M. Szelezniak on Wed. 9 th October 7th October 2013 IPRD13, 7-10 October 2013, Siena, Italy 4

New projects new challenges Spatial resolution [µm] Integration time (µs) TID (MRad) NIEL (n eq /cm 2 ) STAR-PXL ~5 200 0.15 3 10 12 35 Temp ( C) ALICE-ITS ~5 10-30 0.7 10 13 30 CBM-MVD ~5 10-30 10 10 14 <0 ILD-VXD ~3 10 ~0.1 ~10 11 30 AMS 0.35 µm process cannot satisfy the requirements of the future projects Another CMOS process is needed with Smaller feature size to Increase TID hardness (thinner gate oxide) Allow more sophisticated and faster readout Higher resistivity of the epitaxial layer to Increase NIEL hardness (more depletion, less sensitive to the charge traps) 7th October 2013 IPRD13, 7-10 October 2013, Siena, Italy 5

TowerJazz CMOS process NMOS PMOS P-well N-well P-well N-well P-well Deep P-well P - epitaxial layer P ++ substrate Feature size: 0.18 µm Thick epitaxial layer: 18-40 µm, 1 < ρ < 6 kω*cm Six metal layers Deep P-well option (P-layer underneath N-well protecting from parasitic charge collection) allows usage of PMOS transistors Stitching option 7th October 2013 IPRD13, 7-10 October 2013, Siena, Italy 6

2012: first validation of the process 2 prototypes tested in the lab and at CERN-SPS Radiation hardness of the process proven: Det. efficiency ~98% @30 C after 1 MRad + 10 13 n eq /cm 2 arxiv:1305.0531 Main issue: Non-gaussian tail of the noise distribution due to the Random Telegraphic Signal (RTS) 7th October 2013 IPRD13, 7-10 October 2013, Siena, Italy 7

Development of the full scale chips In-pixel CDS MISTRAL Column-level discriminator Rolling shutter readout 2 rows read out in parallel Integration time: 30 µs In-pixel CDS ASTRAL In-pixel discriminator Rolling shutter readout 2 rows read out in parallel Integration time: 15 µs Power: < 200 mw/cm 2 Power: 100 mw/cm 2 + common zero suppression logic (SUZE 02) 2D Cluster search Encoding of 4 5 pixels windows Output data rate ~ 1 Gbit/s 7th October 2013 IPRD13, 7-10 October 2013, Siena, Italy 8

March 2013 engineering run Joint effort in collaboration with CERN and RAL (UK) 6 most important chips: MIMOSA 22THR(A1/A2/B): RTS noise mitigation 2-row readout validation AROM-0: ASTRAL in-pixel circuitry validation SUZE 02: zero suppression MIMOSA 34: optimization of pixel size and design, epitaxial layer thickness and resistivity 7th October 2013 IPRD13, 7-10 October 2013, Siena, Italy 9

Laboratory tests: noise L/W = 0.18/1 µm L/W = 0.36/1 µm L/W = 0.36/2 µm MIMOSA 22 THR-A RTS noise mitigation through the gate size of the input transistor RTS noise tail is suppressed (TN 17 e - ) MIMOSA 22 THR-B double row readout via end-of-column discriminators FPN increase due to the coupling (3 5 e - ENC) FPN: single row (M22THRA) vs. double row readout (M22THRB) 7th October 2013 IPRD13, 7-10 October 2013, Siena, Italy 10

Beam tests: Detection efficiency & fake hit rate MIMOSA 22THR-A1 tested with the ~5 GeV/c electron beam at DESY in Aug 2013 Result: in the threshold range of (5-8) σ noise Detection efficiency ε det 99.5% Fake rate ~10-5 for the pixels with RTS mitigation (S1, S2) To be confirmed after irradiation 7th October 2013 IPRD13, 7-10 October 2013, Siena, Italy 11

Spatial resolution vs. pixel pitch Measurement was performed with MIMOSA 34 chip at DESY electron beam Pixels sizes tested: 22 30, 22 33, 22 44, 22 66 µm 2 Analog resolution via 12-bit signal encoding: ~2.5 µm for 22 33 µm 2 ~3.5 µm for 22 66 µm 2 Binary resolution after conversion to 1-bit clusters: < 5 µm for 22 33 µm 2 < 7 µm for 22 66 µm 2 Results compatible with previous chips. 7th October 2013 IPRD13, 7-10 October 2013, Siena, Italy 12

AROM-0: in-pixel discriminators 3 versions of the in-pixel discriminator 4 32 32 pixel matrices with single row readout 2 16 16 pixel matrices with double row readout Chip tested in the lab Noise estimated from the transfer function (S-curve) 16 16 matrix Double row readout TN = 1.52 mv FPN = 0.45 mv X1.5 higher than target To be improved 7th October 2013 IPRD13, 7-10 October 2013, Siena, Italy 13

Conclusions & outlook TowerJazz 0.18 µm CMOS process is chosen for the on-going CPS developments for ALICE ITS upgrade and CBM-MVD Upstream and downstream parts of the final architectures (MISTRAL/ASTRAL) will be validated in 2013 2014-15 production of the first full scale (~1 cm 2 ) prototypes 2015-16 production of the final chips for ALICE-ITS and CBM-MVD 2017-19 adaptation to the ILD requirements 7th October 2013 IPRD13, 7-10 October 2013, Siena, Italy 14

Thank you for your attention 7th October 2013 IPRD13, 7-10 October 2013, Siena, Italy 15

Cluster multiplicity 7th October 2013 IPRD13, 7-10 October 2013, Siena, Italy 16