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To cite this document: Goiffon, Vincent and Virmontois, Cédric and Magnan, Pierre and Girard, Sylvain and Paillet, Philippe Analysis of Total Dose Induced Dark Current in

CMOS Image Sensors from Interface State and Trapped Charge Density Measurements.

(2010) In: IEEE Nuclear and Space Radiation Effects Conference (NSREC 2010), 19 July 2010 - 23 July 2010 (Denver, United States). (Unpublished)

Open Archive Toulouse Archive Ouverte (OATAO)

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This is an author-deposited version published in: http://oatao.univ-toulouse.fr/

Eprints ID: 11394

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(2)

Vincent Goiffon

1

, Cédric Virmontois

1

, Pierre Magnan

1

,

Sylvain Girard

2

and Philippe Paillet

2

2010 IEEE Nuclear and Space Radiation Effects Conference 20 July 2010, Denver, Colorado

1

Institut Supérieur de l’Aéronautique et de l’Espace (ISAE)

Image Sensor Research Team, Toulouse University, France

(3)

20 July 2010 NSREC2010 - V. Goiffon 2

Context / Motivations

Dark current increases in CIS are

often reported

but

Its variation with TID has not been explained in detail so far The annealing behavior is not fully understood

Radiation hard photodiode structures compatible with the majority of commercial deep sub-micrometer CMOS process is still missing

Purpose of this work:

Precise the role of TID induced trapped charge and interface states

in the generation of dark current in CIS

Dark current

increase is the main issue in

CMOS Image

Sensors

(

CIS

) exposed to ionizing radiations in:

Space / Military / Scientific / Medical applications

Dark current (

IDARK)

Parasitic current when the sensor is not illuminated

Reduces the useful voltage swing and brings shot noise

(4)

20 July 2010 NSREC2010 - V. Goiffon 3

Talk Outline

Experimental details

Results & Discussion

Nature of TID induced dark current

Role of trapped charges

(5)

20 July 2010 NSREC2010 - V. Goiffon

Photodiode environment

in pixel arrays

As can be seen on the 3x3 pixel array illustration

photodiodes (PN junctions) are

surrounded by Shallow

Trench Isolations

(

STI

) in CMOS image sensors

The

depleted region ends

at the bottom

STI interface

(6)

20 July 2010 NSREC2010 - V. Goiffon

Photodiode environment

in pixel arrays

As can be seen on the 3x3 pixel array illustration

photodiodes (PN junctions) are

surrounded by Shallow

Trench Isolations

(

STI

) in CMOS image sensors

The

depleted region ends

at the bottom

STI interface

3x3 pixel array

Photodiode STI Photodiode

(7)

20 July 2010 NSREC2010 - V. Goiffon

Photodiode environment

in pixel arrays

As can be seen on the 3x3 pixel array illustration

photodiodes (PN junctions) are

surrounded by Shallow

Trench Isolations

(

STI

) in CMOS image sensors

The

depleted region ends

at the bottom

STI interface

3x3 pixel array

Photodiode STI Photodiode

2 adjacent pixel cross section

Space charge region

(8)

Test structures

The following

test structures

have been used in this

work to

study the dark current

:

(9)

Test structures

CIS photodiode

The following

test structures

have been used in this

work to

study the dark current

:

CIS photodiode:

(10)

Test structures

FOXFET

CIS photodiode

The following

test structures

have been used in this

work to

study the dark current

:

CIS photodiode:

To measure the dark current

FOXFET:

To estimate the defect densities around the photodiode

Drain/Source = CIS photodiode

(11)

20 July 2010 NSREC2010 - V. Goiffon 10

Test chip & Irradiation

Test structures : Photodiodes

Arranged in arrays of 300 diodes in parallel Junction size: 2 µm x 5 µm

Test structures : FOXFETs

To extract the defect densities at the photodiode vicinity

Several W/L ratios : from 300/0.7 to 300/100

Manufactured

On the same die

By using a commercial 0.18µm CMOS process dedicated to imagers

Irradiated at CEA DIF by

10 keV X-rays

Up to 1 Mrad(SiO2) At ~0.5 krad/s

(12)

20 July 2010 NSREC2010 - V. Goiffon 11

Talk Outline

Experimental details

Results & Discussion

Nature of TID induced dark current

Role of trapped charges

(13)

Irradiated FOXFET I-V characteristics

I

DS

corresponds to the dark current for zero FOXFET gate

voltage:

I

DS

≈ I

DARK

for

V

GS

= 0V

-20 0 20 40 60 10-14 10-12 10-10 10-8 10-6 10-4 10-2

Gate to source voltage (V)

D ra in c u rr e n t (A ) 0 krad 3 krad 10 krad 30 krad 100 krad 300 krad 1 Mrad VDS = 3.3V W/L = 300/0.7

(14)

20 July 2010 NSREC2010 - V. Goiffon 13

Irradiated FOXFET I-V characteristics

I

DS

corresponds to the dark current for zero FOXFET gate

voltage:

I

DS

≈ I

DARK

for

V

GS

= 0V

-20 0 20 40 60 10-14 10-12 10-10 10-8 10-6 10-4 10-2

Gate to source voltage (V)

D ra in c u rr e n t (A ) 0 krad 3 krad 10 krad 30 krad 100 krad 300 krad 1 Mrad VDS = 3.3V W/L = 300/0.7

No sign of gate induced - tunneling effect

- electric field enhancement

No subthreshold conduction up to 100 krad

(15)

20 July 2010 NSREC2010 - V. Goiffon 14

Irradiated FOXFET I-V characteristics

I

DS

corresponds to the dark current for zero FOXFET gate

voltage:

I

DS

≈ I

DARK

for

V

GS

= 0V

-20 0 20 40 60 10-14 10-12 10-10 10-8 10-6 10-4 10-2

Gate to source voltage (V)

D ra in c u rr e n t (A ) 0 krad 3 krad 10 krad 30 krad 100 krad 300 krad 1 Mrad VDS = 3.3V W/L = 300/0.7

No sign of gate induced - tunneling effect

- electric field enhancement

No subthreshold conduction up to 100 krad

Above 100 krad,

subthreshold current dominates

(16)

20 July 2010 NSREC2010 - V. Goiffon 15

Irradiated FOXFET I-V characteristics

I

DS

corresponds to the dark current for zero FOXFET gate

voltage:

I

DS

≈ I

DARK

for

V

GS

= 0V

-20 0 20 40 60 10-14 10-12 10-10 10-8 10-6 10-4 10-2

Gate to source voltage (V)

D ra in c u rr e n t (A ) 0 krad 3 krad 10 krad 30 krad 100 krad 300 krad 1 Mrad VDS = 3.3V W/L = 300/0.7

No sign of gate induced - tunneling effect

- electric field enhancement

No subthreshold conduction up to 100 krad

Above 100 krad,

subthreshold current dominates

(inter device leakage)

100 101 102 103 1010 1011 1012 TID (krad) ∆N o t (c m -2 ) a n d ∆D it ( c m -2 ⋅ e V -1 ) ∆D it ∆Not Extracted defect densities

(17)

20 July 2010 NSREC2010 - V. Goiffon 16

Irradiated photodiode dark current

0 0.5 1 1.5 2 2.5 3 10-15 10-14 10-13 10-12 10-11 10-10 Reverse voltage (V) R e v e rs e c u rr e n t (A ) fresh 3 krad 10 krad 30 krad 100 krad 300 krad 1 Mrad

Slow dark current (I

DARK

) increase with reverse voltage V

R

Negligible diffusion contribution

No sign of tunneling effect / electric field enhancement

Negligible subthreshold conduction (because here W/L is more than 10 time smaller than the FOXFET one)

(18)

20 July 2010 NSREC2010 - V. Goiffon 17

Dark current source location

Previous work showed that radiation induced dark current

was directly

proportional

to the photodiode junction

perimeter P

J

(also confirmed in this work)

The dark current SRH source is located at the STI/depletion

region interface

(19)

20 July 2010 NSREC2010 - V. Goiffon 18

Dark current Arrhenius plot

The dark current activation energy is close to Eg/2

Due to Shockley-Read-Hall generation (even @ 1 Mrad) Dark current simplified expression:

-50 -48 -46 -44 -42 -40 -38 10-15 10-14 10-13 10-12 10-11 10-10 -q/kT (eV-1) I da rk ( A ) 30 krad 100 krad 1 Mrad

it

dep

dark

K

W

D

I

=

×

×

Slope

≈ Eg/2

Depletion width at the STI interface

(20)

20 July 2010 NSREC2010 - V. Goiffon 19

Talk Outline

Experimental details

Results & Discussion

Nature of TID induced dark current

Role of trapped charges

(21)

20 July 2010 NSREC2010 - V. Goiffon 20

Comparison dark current /

interface state density

First, if only the effect of

interface states is considered

:

The dark current increase

∆I

DARK

should be proportional

to the

interface density increase

∆D

it

)

(

)

(

TID

K

P

W

D

TID

I

dark

=

×

J

×

dep

×

it

(22)

20 July 2010 NSREC2010 - V. Goiffon 21

Comparison dark current /

interface state density

If only the effect of

interface states is considered

:

The dark current increase

∆I

DARK

should be proportional

to the

interface density increase

∆D

it

1011 1012 10-13

10-12 10-11

Interface state density increase (cm-2/eV)

D a rk c u rr e n t in c re a s e ( A ) Delta I dark y=a⋅x

No

proportionality

Interface states can not explain by themselves the

observed dark current increase

)

(

)

(

TID

K

W

D

TID

I

dark

=

×

dep

×

it

(23)

20 July 2010 NSREC2010 - V. Goiffon 22

Influence of trapped charges

on dark current (1)

The trapped charge can

change the electrostatic equilibrium

at

the STI interface

Depletion width (WDEP)variation with TID

If the dependence of

W

DEP

on TID

is taken into account:

)

(

)

(

)

(

TID

K

W

TID

D

TID

I

dark

=

×

dep

×

it

[

it it

]

ot dep it ot dark

N

D

K

W

N

D

D

I

(

,

)

=

×

(

)

×

0

+

(24)

20 July 2010 NSREC2010 - V. Goiffon 23

Influence of trapped charges

on dark current (1)

The trapped charge can

change the electrostatic equilibrium

at

the STI interface

Depletion width (WDEP)variation with TID

If the dependence of

W

DEP

on TID

is taken into account:

Function to plot to observe the depletion width evolution:

)

(

)

(

)

(

TID

K

W

TID

D

TID

I

dark

=

×

dep

×

it it it it ot dark ot dep

D

D

D

N

I

K

N

W

+

×

=

0

)

,

(

1

)

(

i th eff J

v

k

Tn

qP

K

=

σ

π

K

=

K

'

×

σ

eff

Known constant

[

it it

]

ot dep it ot dark

N

D

K

W

N

D

D

I

(

,

)

=

×

(

)

×

0

+

(25)

20 July 2010 NSREC2010 - V. Goiffon 24

Influence of trapped charges

on dark current (1)

The trapped charge can

change the electrostatic equilibrium

at

the STI interface

Depletion width (WDEP)variation with TID

If the dependence of

W

DEP

on TID

is taken into account:

Function to plot to observe the depletion width evolution:

)

(

)

(

)

(

TID

K

W

TID

D

TID

I

dark

=

×

dep

×

it

Unknown parameters

i th eff J

v

k

Tn

qP

K

=

σ

π

K

=

K

'

×

σ

eff

Known constant

it it it ot dark ot dep

D

D

D

N

I

K

N

W

+

×

=

0

)

,

(

1

)

(

[

it it

]

ot dep it ot dark

N

D

K

W

N

D

D

I

(

,

)

=

×

(

)

×

0

+

(26)

20 July 2010 NSREC2010 - V. Goiffon 25

Influence of trapped charges

on dark current (2)

1011 1012 0 0.5 1 1.5 2 2.5

Trapped charge density increase ∆Not (cm-2)

In te rf a c e d e p le ti o n w id th ( µ m ) it it dark ot dep

D

D

I

K

N

W

+

×

=

0

1

)

(

2 16

cm

10

2

×

− −

eff

σ

The unknown parameters are chosen to yield realistic depletion

width values (they have a very small influence on the curve shape)

The

depletion width extension

with TID

explains

the observed dark

current evolution

eV

/

cm

10

10 2 0 −

it

D

W

DEP

increases

much with N

ot

(and so with TID)

(27)

20 July 2010 NSREC2010 - V. Goiffon 26

TCAD simulations

Qualitative Sentaurus TCAD simulations based on SIMS

measurements

2 photodiodes separated by 5 µm of STI (as in the studied photodiodes)

Simulation purpose:

Confirm the trapped charge influence on the depletion width at the STI interface

0 krad

N

N

P

Space charge region Space charge region Dark current sources

(28)

20 July 2010 NSREC2010 - V. Goiffon 27

TCAD simulation: N

ot

= 10

11

cm

-2

0 krad

N

ot

= 10

11

cm

-2

~ 7 krad

W

1

W

2

Depletion region

extension at the STI

interface

(W2 > W1)

(29)

20 July 2010 NSREC2010 - V. Goiffon 28

TCAD simulation: Not = 3x10

11

cm

-2

N

ot

= 3x10

11

cm

-2

~ 25 krad

0 krad

W

1

W

2

Depletion region

extension at the STI

interface

(W2 ≈

≈ 3xW1)

(30)

20 July 2010 NSREC2010 - V. Goiffon 29

TCAD Simulation: Not = 10

12

cm

-2

N

ot

= 10

12

cm

-2

~ 160 krad

0 krad

The STI interface is

completely depleted

:

Enhances strongly the generation rate

Can lead to inter device leakage if Not is large enough Adjacent photodiode are biased at different potentials

(31)

20 July 2010 30

Comparison TCAD/measurements

1011 1012 0 0.5 1 1.5 2 2.5 ∆Not (cm-2) W d e p ( µ m ) Experimental data TCAD

The same effect can be

observed on both curves

Discrepancies are acceptable considering the simplifying assumption used

(32)

20 July 2010 NSREC2010 - V. Goiffon 31

Talk Outline

Experimental details

Results & Discussion

Nature of TID induced dark current

Role of trapped charges

(33)

20 July 2010 NSREC2010 - V. Goiffon 32

Summary

After X-ray exposure (up to 1 Mrad(SiO

2

)),

the CIS photodiode

dark current

Increased

quickly with TID

Due to

Shockley-Read-Hall

generation

at the

STI

/depleted region

interface

The

role

of TID induced

defects

was

clarified

:

Interface states

contribute directly to the dark current by

increasing the number of

generation centers

in the depleted

region

Trapped charges

enhance the dark current by

extending the

depleted region

at the STI interface (confirmed by TCAD

simulations)

At

high TID

(above ~300krad), the

STI interface is completely

depleted, and

inter-device leakage

can become an issue

100 101 102 103 10-14 10-13 10-12 10-11 10-10 10-9 TID (krad) D a rk c u rr e n t in c re a s e ( A / µ m )

(34)

20 July 2010 NSREC2010 - V. Goiffon 33

On going and future work

Radiation hardening of CIS photodiodes

Based on this work conclusions

By reducing the effect of trapped charge

Several test structures are being characterized

Find generic

radiation hardened photodiode

designs that can

be used in

any commercial DSM CIS process

Address other type of device

Extend

the study to CIS

pinned photodiode

Address other radiation effects:

(35)

Thank you

for your attention!

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