z. li brookhaven national laboratory, upton, ny 11973-5000, usa e. verbitskaya, v. eremin, a. ivanov...
TRANSCRIPT
Z. Li
Brookhaven National Laboratory, Upton, NY 11973-5000, USA
E. Verbitskaya, V. Eremin, A. Ivanov
Ioffe Physico-Technical Institute of Russian Academy of SciencesSt. Petersburg, Russia
J. Härkönen, E.Tuovinen, P. LuukkaHelsinki Institute of Physics, CERN/PH, 1211 Geneva, Switzerland
Initial data on the DRIVE approach: results and analysis
This work has been supported in part by the US Department of Energy, contract No.: DE-AC02-98CH10886, by the grant of the President of Russian Federation # NS-2223.2003.02, by Academy of Finland, and by the EU Intas 03-52-5477 contract; and it is within the framework CERN RD39 and RD50 collaborations
• Introduction• Current/Conventional Approaches
Defect/Impurity/Material Engineering (DIME) Device Structure Engineering (DSE)Device Operational Mode Engineering (DOME)
• New ApproachesDevice Recovery/Improvement Via Elevated
temp annealing (DRIVE)
• Experimental Methods• Results and Discussions• Summary
OUTLINE
• For SLHC, with 1035 cm-2s-1 luminosity, total radiation fluence can be as high as 1016 neq/cm2
• At this highest fluence, detector degrades in many ways:o High leakage current (IL): 4x10-1 A/cm3 at RT!o High full depletion bias (Vfd): 6400 V for 200 m thick STD
FZ detector!o Low charge collection distance due to trapping (CCE(tr)): 20 to 40 m regardless of detector detector thickness and
depletion depth!
• Radiation hard/tolerant Si detectors have to improve with regard to all three problems listed above
• Most conventional approaches may solve only one to two problems
• Need a new, simple/easy approach
Introduction
Name of the approach
R&D group Good for Technology difficulty
Defect/Impurity/Material Engineering
(DIME)
Oxygenation/MCZ Si CERN RD50 Vfd Easy
Diamond/SiC/GaN, etc. CERN RD42, RD50
Vfd Difficult
Device Structure Engineering (DSE)
3d detectors CERN RD50 CCE(tr), Vfd Very difficult
Semi-3d detectors CERN RD50 Vfd Easy
Thin detectors CERN RD50 Vfd Difficult
Device Operational Mode Engineering
(DOME)
Cryogenic Si detectors (LN2 T)
CERN RD39 IL, Vfd Difficult
Cryogenic Si detectors (LHe T)
CERN RD39 IL, Vfd, and
CCE(tr)?
Very difficult
Current/Conventional Approaches
Device Recovery/Improvement Via Elevated temperature annealing (DRIVE)
The DRIVE was first proposed by Z. Li and J. Harkonen on the 5th RD50 Workshop in Florence, Italy, October 14-16, 2004
Preliminary data presented by E. Verbitskaya et al, at the 6th RD50 Workshop, Helsinki, June 2-4, 2005
Thermal annealing of radiation damage has been a conventional way for material/device recovery
It has not been used so far in HE physics detector field for standard FZ and oxygenated FZ Si detectors because :
If the annealing temperature is too high (>450 °C), it will destroy the detector and/or electronics
If the annealing temperature is too low (< 450 °C), the reverse annealing (generation of more negative space charges) will make the detector worse
New Approach
Device Recovery/Improvement Via Elevated temperature annealing (DRIVE) (continues)
However, for high resistivity MCZ Si material/detectors, thermal annealing in the temperature range from 200 °C to 450 °C will generate thermal donor (TD, positive space charge) due to high oxygen concentration [O]
By playing the annealing T and time, and [O] (n-type or p-type MCZ Si), one may adjust the TD creation rate in such a way to cancel the reverse annealing effect, and even better, to compensate the original (as-irradiated) negative space charges, which may bring the full depletion voltage down to a manageable range
Elevated temperature annealing (ETA) will also anneal out/down the detector leakage current, and improve detector CCE by annealing out shallow trapping centers
The DRIVE approach may therefore offer a technology to improve all three areas:
IL, Vfd, CCE (tr)
The degree of difficulty may vary depending on the annealing techniques
New Approach
1.0E+09
1.0E+10
1.0E+11
1.0E+12
1.0E+13
1.0E+14
0 10 20 30 40 50 60 70
Heating time @ 430C
Ne
ff
1 ppma
4,5 ppma
10 ppma
p-type MCZ
n-type MCZ
n-type oxygenated FZ
TD generation in different Si with different [O]
1.0E+09
1.0E+10
1.0E+11
1.0E+12
1.0E+13
1.0E+14
0 10 20 30 40 50 60 70
Heating time @ 430C
Ne
ff
10 ppma
One can reach >1014 /cm3 in TD concentration in one hour!Might be enough to cancel – SC generated in irradiation and during reverse
anneal
TD generation at 450 °C in p-type MCZ
Experimental
Detectors: p+-n-n+ pad structures with multiple GRs from n-type MCZ Si with a resistivity of 1 kOhmcm, p+-p-n+ pad structures with multiple GRs, from p-type MCZ Si with a resistivity of 3 kOhmcm
all processed at HIP Irradiation :
P352-18 (p) 9.00E+13 C1-3 (n) 5.90E+13P352-59 (p) 3.60E+14 D2-3 (n) 1.20E+14P352-48 (p) 5.00E+14
protons 20 MeVprotons 24 GeV/c
Annealings
multistep process with a variable time T: 150-450C tann: variable, 10 min up to 120 min/step nitrogen flow fast cooling (~10 min)
Ep protons 24 GeV/c protons 20 MeV # P352-18 P352-59 P352-48 C1-3 D2-3
Fp (cm-2) 91013 3.61014 51014 5.91013 1.21014 annealing
steps 8 12 13 8 10
T (C) 150-450 300-450 450 430-450 430-450
All as-irradiated detectors (p or n-type) have negative space charges before annealingThis means, for n-type detector, the space charge sign inversion (SCSI) occurred
Experimental techniques
Measurements:
After each annealing step (at BNL):
I-V and C-V dependences current pulse response using TCT with a laser pulse generation of non-equilibrium carriers
After final detector annealing (at Ioffe Institute):
Spectra of deep levels (C-DLTS)
Experimental resultsExperimental results
Three stages of the changes of detector characteristics
irrespective to Ep and Fp:
1. Reverse annealing: Irev , Vfd , negative Neff , W TCT signal from the detector p+ side disappears
2. Recovery of reverse current Irev and the signal from p+ side
3. SCSI from negative to positive
Annealing of detectors irradiated by 24 GeV/c protonsAnnealing of detectors irradiated by 24 GeV/c protons
Compensation of acceptor-type radiation induced defects:Thermal Donors areintroduced at 430-450C
Reverse annealing
Recovery of reverse current
24 GeV protons, P352-18, Fp = 91013 cm-2
P352-18, 24 GeV/c protons, Fp = 9e13 cm-2
0.1
1
10
100
1000
1 10 100 1000V (Volt)
I (
A)
before anneal
1: 150 C, 10 min
2: 200 C, 10 min
3: 300 C, 10 min
4: 430 C, 15 min
5: 430 C, 20 min
6: 450 C, 30 min
7: 450 C, 2 h
8: 450 C, 1 h
GRG
2 h
150-300C – Irev is still saturated
Leakage current decreasedby more than one order of magnitude.
24 GeV protons, P352-48, Fp = 51014 cm-2T = 450C
P352-48, 24 GeV/c protons, Fp = 5e14 cm-2
1.0E-02
1.0E-01
1.0E+00
1.0E+01
1.0E+02
1.0E+03
1 10 100 1000V (Volt)
I (u
A)
no anneal
8: 20 min, t_s = 245 min
9: 60 min, t_s = 305 min
10: 30 min, t_s = 335 min
11: 40 min, t_s =375 min
12: 20 min, t_s = 395 min
13: 10 min, t_s = 405 min
Annealing at 450 C
GRG
1 h
• Bulk current decreases after 1st anneal, but the leakage arises at high biases• tann = 305 min: Irev becomes saturated• After final anneal, leakage current decreased by more than 2 orders of magnitude
P352-48, 24 GeV/c protons, Fp = 5e14 cm-2
0.1
1
10
100
1000
1 10 100 1000V (Volt)
I (
A)
no anneal, RTA28 days
1: 60 min
2: 15 min, t_s =75 min
3: 15 min, t_s =90 min
4: 15 min, t_s =105 min
5: 60 min, t_s =165 min
6: 30 min, t_s =195 min
7: 30 min, t_s =225 min
8: 20 min, t_s=245 min
GRG
Annealing at 450 C
Changes of TCT signal: Fp = = 91013 cm-2, P352-18
P352-18, 24 GeV/c protons, Fp = 9e13 cm-2, p+ side
-1.0E-03
0.0E+00
1.0E-03
2.0E-03
3.0E-03
4.0E-03
5.0E-03
6.0E-03
7.0E-03
8.0E-03
9.0E-03
1.0E-02
7.0E-08 7.5E-08 8.0E-08 8.5E-08 9.0E-08 9.5E-08 1.0E-07
t (s)
V (
Vo
lt)
37
47
56
66
76
86
96
106
116
146
167
196
216
247
297
346
before anneal
V (Volt): P352-18, 24 GeV/c protons, Fp = 9e13 cm-2, n+ side
-1.0E-03
0.0E+00
1.0E-03
2.0E-03
3.0E-03
4.0E-03
5.0E-03
6.0E-03
3.5E-08 4.0E-08 4.5E-08 5.0E-08 5.5E-08 6.0E-08 6.5E-08 7.0E-08 7.5E-08
t (s)
V (
Vo
lt)
27
47
56
76
86
96
106
116
146
176
196
196
246
345
395
before anneal
V (Volt):
SC (-)p+/p/n+ structureHigh field on the n+ side
SCSI: SCSI: tann(450 C) = 210 min
P352-18, 24 GeV/c protons, Fp = 9e13 cm-2, p+ side
-0.005
0
0.005
0.01
0.015
0.02
0.025
0.03
1.50E-08 2.00E-08 2.50E-08 3.00E-08 3.50E-08 4.00E-08
t (s)
V (
Vo
lt)
20
40
60
80
100
120
140
160
180
200
220
240
260
300
400
500
600
after 8th anneal450 C, 60 min
t_s(450) = 210 min
V (Volt):
P352-18, 24 GeV/c protons, Fp = 9e13 cm-2, n+ side
-0.002
0
0.002
0.004
0.006
0.008
0.01
0.012
2.00E-08 2.50E-08 3.00E-08 3.50E-08 4.00E-08 4.50E-08 5.00E-08
t (s)
V (
Vo
lt)
250
300
350
400
450
500
550
600
650
700
750
800
850
900
950
1000
V (Volt):
after 8th anneal450 C, 60 min
t_s(450) = 210 min
SC (+)
p+/n/n+ structureHigh field on the p+ side
Neff evolutionNeff derived from TCT measurements
Reverseannealing
Neff recoveryup to SCSI
Neff evolution
P352-18, 24 GeV/c, 9e13 cm-2
-4.0E+13
-3.0E+13
-2.0E+13
-1.0E+13
0.0E+00
0 100 200 300 400 500
T (C)
Ne
ff (
cm
-3)
t_ann =15 min
t_ann = 10 min
Range of reverse annealing
Neff vs. tann, 24 GeV/c protons
-7.0E+13
-6.0E+13
-5.0E+13
-4.0E+13
-3.0E+13
-2.0E+13
-1.0E+13
0.0E+00
1.0E+13
2.0E+13
0 50 100 150 200 250 300 350 400 450
t (min)
Nef
f (c
m-3
)
P352-18, 9e13 cm-2 P352-59, 3.6e14 cm-2 P352-48, 5e14 cm-2
Tann = 450 C
Range of TD introduction
Finally
Fp (cm-2) Vfd (Volt) Neff (cm-3)
9.00E+13 250 3.6E+123.60E+14 460 6.7E+125.00E+14 500 7.3E+12
All positive space charge
Since these are all initially p-type wafers withless than 1011/cm3 donors, the positive spacecharge has to be thermal donor
+SC
-SC
-SC
Annealing of detectors irradiated by 20 MeV protonsAnnealing of detectors irradiated by 20 MeV protons
Compensation of acceptor-type radiation induced defects:Thermal Donors areintroduced at 430-450C
n-type detectors before irradiation,initially (+SC)
All positive space chargeafter annealing (+SC)
After irradiation, space charge signinverted to negative (“p”) (-SC)
Recovery of reverse current
C1-3, 20 MeV protons, Fp = 5.9e13 cm-2
0.01
0.1
1
10
100
1000
1 10 100 1000V (Volt)
I (
A)
1: 430 C,20 min+RTA2: 450 C,60 min
3: 450 C,15 min
4: 450 C,15 min
5: 450 C,15 min
6: 450 C,60 min
7: 450 C,30 min
8: 450 C,15 min
GRG
1 h
D2-3, 20 MeV protons, Fp = 1.2e14 cm-2
0.01
0.1
1
10
100
1000
1 10 100 1000V (Volt)
I (
A)
1: 430 C, 20 min+RTA 6 mns2: 450 C, 60 min
3: 450 C, 15 min
4: 450 C, 15 min
5: 450 C, 15 min
6: 450 C, 30 min
7: 450 C, 20 min
8: 450 C, 1 h
9: 450 C, 30 min
10: 450 C, 20 mint_s = 265 min
GRG
Leakage is observed in I-V curves
Annealing time at 450 C for SCSI vs. Fp
0
50
100
150
200
250
300
350
400
450
0.0E+00 1.0E+14 2.0E+14 3.0E+14 4.0E+14 5.0E+14 6.0E+14
Fp (cm-2)
t_a
nn
(m
in)
24 GeV/c protons
20 MeV protons
T = 450 C
Annealing time at 450C required for SCSI
Defect spectra after SCSIDefect spectra after SCSI
-6.5
-4.5
-2.5
-0.5
1.5
50 100 150 200 250 300
Temperature (K)
DLT
S s
ign
al (
pF
)
C1_3
P352-18
P352-48
P204-I-A3-7
Ci-OiRD2
with injection
C-DLTS spectra
Reference spectra:P204-I-A3-7:24 GeV/cFp = 1.51011 cm-2
-0.1
0.4
0.9
1.4
50 100 150 200 250 300Temperature (K)
DLT
S s
ign
al (
pF
)
C1_3
P352-18
P352-48
P204-I-A3-7
V-O VV-
VV--
Continuous defect spectra Increase of tann
is favorable(for P352-48 tann is maximal)
-0.2
0
0.2
0.4
0.6
0.8
1
1.2
1.4
50 100 150 200 250 300
Temperature ([K)
DLT
S s
ign
al (
pF
)
experim. fit E1 E2 E3
E5 E4 E6 E7 E8
E1
E3E4
E6
E2
E5
E7
E8Electron traps
P352-1824 GeV/c, 91013 cm-
2
Hole traps
-6.5
-5.5
-4.5
-3.5
-2.5
-1.5
-0.5 50 100 150 200 250 300
Temperature (K)
DLT
S s
ign
al (
pF
)
experim. fit H1 H2 H4 H3 H5
H4
H1H3
H2H5
Defect parameters
Electron traps
DL H1 H2 H3 H4 H5
E (eV) Ev + 0.203 Ev + 0.28 Ev + 0.3 Ev + 0.37 Ev + 0.545 (cm2) 1.0E-16 1.0E-15 3.0E-16 4.0E-16 1.0E-15N (cm-3) 1.5E+12 1.6E+12 7.0E+11 5.4E+12 1.3E+12
Hole traps
DL E1 E2 E3 E4 E5 E6 E7 E8
E (eV) Ec – 0.18 Ec – 0.196 Ec – 0.26 Ec – 0.25 Ec – 0.37 Ec – 0.41 Ec – 0.515 Ec – 0.6 (cm2) 3.0E-15 7.0E-16 2.0E-15 3.0E-17 3.0E-15 1.0E-15 5.0E-15 2.0E-15N (cm-3) 1.0E+12 4.5E+11 2.0E+11 2.8E+11 6.9E+11 7.2E+11 4.5E+11 2.6E+11
P352-1824 GeV/c, 91013 cm-2
Defects detected after annealing are presumably products of RDs decay Concentrations of defects after annealing are <10% of as-irradiated RD concentrations Minimal concentrations correspond to the maximal annealing time (P352-48)
Ways of ETAWays of ETA
May be different:
1) localized laser anneal; 2) localized anneal using a lamp; 3) annealing using pre-built-in external heating resistors; 4) annealing using leakage current of the detector itself;5) RT annealing using ultrasonic power
4) and 5) may be the easiest and most practical method
Multiple annealing steps at smaller doses maybe favorable
Fine tuning of the annealing time is required for precise manipulation of thermal donor introduction and resulting Neff
– further studies are needed
o The conventional approaches may not solved all the radiation induced problems
o The new approach, DRIVE, could offer a perfect solution to radiation induced problems, especially at high fluences for SLHC
o Recovery of the positive space charge and detector reverse current is realized by ETA at 450C
o By changing annealing temp, time, one may get a perfect receipt for different fluences
o P-type MCZ Si may be the best material due to its higher [O] than that of n-type MCZ o Different annealing techniques may be used for DRIVE depending on the experiment conditions
o Further studies on detector CCE, on FZ Si, and effect of radiation/annealing cycles are underway
ConclusionsConclusions