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To cite this document: Virmontois, Cédric and Goiffon, Vincent and Magnan, Pierre and

Girard, Sylvain and Inguimbert, Christophe and Petit, Sophie and Rolland, Guy and

Saint-Pé, Olivier Displacement Damage Effect Due to Neutron and Proton Irradiations

on CMOS Image Sensors Manufactured in Deep Sub-Micron Technology. (2010) In:

Nuclear and Space Radiation Effects Conference (NSREC), 19 July 2010 - 23 July 2010

(Denver, United States). (Unpublished)

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rchive

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oulouse

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rchive

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Displacement Damage Effect Due to Neutron and Proton

Irradiations on CMOS Image Sensor

C. Virmontois

1

(cedric.virmontois@isae.fr),

V. Goiffon

1

,S. Girard

2

, C. Inguimbert

3,

O. Saint-Pé

4

,

S. Petit

5

, G. Rolland

5

, P. Magnan

1

1Université de Toulouse, ISAE, 2CEA, DAM, DIF, 3ONERA, DESP, 4EADS Astrium, 5CNES

Test chip :

0.18 µm CMOSCIStechnology

Dedicated photodiodedoping profiles

128 x 128 pixel arrays,3T, 10µm pitch

Larges photodiodes (>104 µm²)

Proton irradiation :

Facilities : KVI, UCL, TRIUMF

Energies :50 to 500 MeV

Fluences : 5 x 109to 1 x 1011H+/cm²

Neutron irradiation : Facilities : CEA Valduc, UCL

Energies :0.8 to 20 MeV

Fluences : 5 x 109to 1 x 1013N/cm²

Experimental

Overview

Goal : Study ofdisplacement damageeffects onCMOS sensorsmanufactured in adeep

sub-microntechnologydedicated to imagingapplications

Test structures :pixel arrays + isolated large photodiodes

Main result :

Main damage due to displacement is dark current increase

Proton displacement effect

Neutron and proton induce equivalent displacement damage

Analytic model, based on damage energy, could predict dark current increase distribution in APS

Defects responsible of dark current increase are intrinsic defectsprobably in the form of cluster

Effects on in-pixel photodiode

Main defectsinducing dark current increasein

photodiode, after γγγγ-ray (1), proton (2) and neutron (3) irradiations :

Ionizationinduces interface statesin Shallow

Trench Isolation (STI)

Displacement induces point defectsand

clusters of defectsin space charge region (SCR)

Bulk defects Interface states

Annealing

0 0,2 0,4 0,6 0,8 1 1,2 0 50 100 150 200 250 300 Annealing temprature (°C) U n a n n e a le d F a c to r PD 2000x5 µm PD 800x800 µm PD 4000x5 µm APS 38 TeV/g APS 183 TeV/g APS 365 TeV/g APS 20000 TeV/g

Unannealed dark current fraction and

DLTS measurements show that defects

inducing dark current increase could be

probably in the form of clusters

Effects on CMOS sensors

No photoresponse degradation, no voltage shift, no gain reduction

No sign of electric

field enhancementat

the Si-STI interface

Neutron induces essentially

Displacement damages Proton induced displacement

damageseffects on mean dark

current arenegligible in front

ofionizing dose 1,E-20 1,E-18 1,E-16 1,E-14 1,E-12

1,E-02 1,E+00 1,E+02 1,E+04

Displacement dose (TeV/g)

Id a rk i n c re a s e ( A ) Experimental results Displacement contributions + 1,E-16 1,E-15 1,E-14 1,E-13

1,E+01 1,E+02 1,E+03 1,E+04

Displacement dose (TeV/g)

Id a rk i n c re a s e ( A ) Experimental results Displacement contributions 0,001 0,01 0,1 1 10 0 0,5 1 1,5 2 2,5 3 3,5 4

Dark current (fA)

R e la ti v e f re q u e n c y Initial 0,4 TeV/g 3,78 TeV/g 37,8 TeV/g 182,5 TeV/g 365 TeV/g

Pixel tail, due to neutron induced displacement,

increases followingdisplacement damage dose

Histogram observations ofdark

current increase due to

neutron irradiationare

compared to estimates based on GEANT 4 calculations of the

recoil spectrum parameters Estimation of dark current increase is calculated usingthe recoil element damage energy

Proportionalitybetween

damage energy anddark

current increase based on

NIEL is used

Analytic model is convolved

withionization fit to obtain proton induced dark current increase distribution. 0,001 0,01 0,1 1 10 100 0 1 2 3 4 5 6 7

Dark current increase (fA)

R e la ti v e f re q u e n c y Measurements 39 TeV/g Measurments 183 TeV/g Measurement 365 TeV/g model 39 TeV/g model 183 TeV/g model 365TeV/g 0,001 0,01 0,1 1 10 0 0,5 1 1,5 2 2,5 3 3,5 4 4,5 5 Dark current increase (fA)

R e la ti v e f re q u e n c y Proton 39 TeV/g Simulation

Dark current at 23°C (fA)

A c ti v a ti o n e n e rg y ( e V )

Dark current at 23°C (fA)

A c ti v a ti o n e n e rg y ( e V )

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