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 (Unpublished)
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Vincent Goiffon
1, Cédric Virmontois
1, Pierre Magnan
1,
Sylvain Girard
2and Philippe Paillet
22010 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
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
20 July 2010 NSREC2010 - V. Goiffon 3
Talk Outline
Experimental details
Results & Discussion
Nature of TID induced dark current
Role of trapped charges
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
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
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
Test structures
The following
test structures
have been used in this
work to
study the dark current
:
Test structures
CIS photodiode
The following
test structures
have been used in this
work to
study the dark current
:
CIS photodiode:
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
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
20 July 2010 NSREC2010 - V. Goiffon 11
Talk Outline
Experimental details
Results & Discussion
Nature of TID induced dark current
Role of trapped charges
Irradiated FOXFET I-V characteristics
I
DScorresponds to the dark current for zero FOXFET gate
voltage:
I
DS≈
≈ I
≈
≈
DARKfor
V
GS= 0V
-20 0 20 40 60 10-14 10-12 10-10 10-8 10-6 10-4 10-2Gate 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
20 July 2010 NSREC2010 - V. Goiffon 13
Irradiated FOXFET I-V characteristics
I
DScorresponds to the dark current for zero FOXFET gate
voltage:
I
DS≈
≈ I
≈
≈
DARKfor
V
GS= 0V
-20 0 20 40 60 10-14 10-12 10-10 10-8 10-6 10-4 10-2Gate 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
20 July 2010 NSREC2010 - V. Goiffon 14
Irradiated FOXFET I-V characteristics
I
DScorresponds to the dark current for zero FOXFET gate
voltage:
I
DS≈
≈ I
≈
≈
DARKfor
V
GS= 0V
-20 0 20 40 60 10-14 10-12 10-10 10-8 10-6 10-4 10-2Gate 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
20 July 2010 NSREC2010 - V. Goiffon 15
Irradiated FOXFET I-V characteristics
I
DScorresponds to the dark current for zero FOXFET gate
voltage:
I
DS≈
≈ I
≈
≈
DARKfor
V
GS= 0V
-20 0 20 40 60 10-14 10-12 10-10 10-8 10-6 10-4 10-2Gate 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
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
RNegligible 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)
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
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 interface20 July 2010 NSREC2010 - V. Goiffon 19
Talk Outline
Experimental details
Results & Discussion
Nature of TID induced dark current
Role of trapped charges
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
DARKshould be proportional
to the
interface density increase
∆
∆D
∆
∆
it)
(
)
(
TID
K
P
W
D
TID
I
dark=
×
J×
dep×
∆
it20 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
DARKshould be proportional
to the
interface density increase
∆
∆D
∆
∆
it1011 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×
∆
it20 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
DEPon TID
is taken into account:
)
(
)
(
)
(
TID
K
W
TID
D
TID
I
dark=
×
dep×
it[
it it]
ot dep it ot darkN
D
K
W
N
D
D
I
(
∆
,
∆
)
=
×
(
∆
)
×
0+
∆
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
DEPon 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 depD
D
D
N
I
K
N
W
∆
+
∆
∆
×
=
∆
0)
,
(
1
)
(
i th eff Jv
k
Tn
qP
K
=
σ
π
K
=
K
'
×
σ
effKnown constant
[
it it]
ot dep it ot darkN
D
K
W
N
D
D
I
(
∆
,
∆
)
=
×
(
∆
)
×
0+
∆
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
DEPon TID
is taken into account:
Function to plot to observe the depletion width evolution:
)
(
)
(
)
(
TID
K
W
TID
D
TID
I
dark=
×
dep×
itUnknown parameters
i th eff Jv
k
Tn
qP
K
=
σ
π
K
=
K
'
×
σ
effKnown constant
it it it ot dark ot depD
D
D
N
I
K
N
W
∆
+
∆
∆
×
=
∆
0)
,
(
1
)
(
[
it it]
ot dep it ot darkN
D
K
W
N
D
D
I
(
∆
,
∆
)
=
×
(
∆
)
×
0+
∆
20 July 2010 NSREC2010 - V. Goiffon 25
Influence of trapped charges
on dark current (2)
1011 1012 0 0.5 1 1.5 2 2.5Trapped 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
∆
+
×
=
∆
01
)
(
2 16cm
10
2
×
− −≈
effσ
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 −≈
itD
W
DEPincreases
much with N
ot(and so with TID)
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 sources20 July 2010 NSREC2010 - V. Goiffon 27
TCAD simulation: N
ot= 10
11cm
-20 krad
N
ot
= 10
11
cm
-2
~ 7 krad
W
1W
2Depletion region
extension at the STI
interface
(W2 > W1)
20 July 2010 NSREC2010 - V. Goiffon 28
TCAD simulation: Not = 3x10
11cm
-2N
ot
= 3x10
11
cm
-2
~ 25 krad
0 krad
W
1W
2Depletion region
extension at the STI
interface
(W2 ≈
≈
≈ 3xW1)
≈
20 July 2010 NSREC2010 - V. Goiffon 29
TCAD Simulation: Not = 10
12cm
-2N
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
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 TCADThe same effect can be
observed on both curves
Discrepancies are acceptable considering the simplifying assumption used
20 July 2010 NSREC2010 - V. Goiffon 31
Talk Outline
Experimental details
Results & Discussion
Nature of TID induced dark current
Role of trapped charges
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 )
20 July 2010 NSREC2010 - V. Goiffon 33