monolithic sensors in high-voltage deep-submicron technology
DESCRIPTION
Monolithic sensors in high-voltage deep-submicron technology. Ivan Peric University of Heidelberg, Germany. Introduction to pixel sensors in high voltage CMOS technology Operation principle, advantages and disadvantages Summary of the project results Pixel types - PowerPoint PPT PresentationTRANSCRIPT
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1FEE 2011, Ivan Peric
Monolithic sensors in high-voltage deep-submicron technology
Ivan Peric
University of Heidelberg, Germany
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2FEE 2011, Ivan Peric
• Introduction to pixel sensors in high voltage CMOS technology
• Operation principle, advantages and disadvantages
• Summary of the project results
• Pixel types
• 1) Particle sensitive pixels with complex CMOS electronics– Test chip in 180nm technology
• 2) Integrating pixels with simple “4T” electronics– 4PMOST source follower pixels
– 4PMOST pixels with voltage amplification
– >4T CDS pixels
• Test beam and lab measurements
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3FEE 2011, Ivan Peric
Pixel detector in HV CMOS technology
• Monolithic pixel sensor• 100% fill-factor• In-pixel CMOS signal processing• Good timing properties (theoretically 40 ps signal collection time)
• Radiation hard (tested to 50 MRad (x-rays) and 1015 neq (protons))
• Not expensive (monolithic sensor, no bumping, standard technology used)• 350nm technology: 8 inch wafer run: 90k€ (350nm) • 180nm technology: 120k€ and 1.5k€/wafer (1 wafer ~ 200 cm2)• Allows thinning
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4FEE 2011, Ivan Peric
Detector structure
• The sensor is based on the “deep” n-well in a p-substrate• Main properties: • 1) Charge collection is based on drift• 2) CMOS signal processing electronics
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5FEE 2011, Ivan Peric
Detector structure
Deep n-well
Pixel electronics in the deep n-wellP-substrate
NMOS transistorin its p-well
PMOS transistor
The CMOS signal processing electronics are placed inside the deep-n-well. PMOS are placed directly inside n-well, NMOS transistors are situated in their p-wells that are embedded in the n-well as well.
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6FEE 2011, Ivan Peric
“Smart” diode array - SDA
Deep n-well
Pixel electronics in the deep n-wellP-substrate
NMOS transistorin its p-well
PMOS transistor
Smart diode
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7FEE 2011, Ivan Peric
SDA in high voltage CMOS technology
P-substrate
NMOS transistorin its p-well
PMOS transistor
Particle
E-field
Deep n-well
Pixel electronics in the deep n-well
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8FEE 2011, Ivan Peric
SDA in high voltage CMOS technology
• Although this structure can be implemented in any CMOS technology (see 65nm pixel), the best results are achieved when a standard high voltage CMOS technology with twin well is used.
• A lowly-doped deep n-well can be then used. Such an n-well can be reversely biased with a high voltage.
• In the process we used, we expect a depleted area thickness of 14 μm (20cm substrate resistance -> acceptor density ~ 1015 cm-3)
• We measure a MIP signal of ~ 2000e, ~ 50% probably originates from undepleted bulk.
• The charge generated by ionizing particles in the depleted area is collected by drift. Due to high electric field and small drift path, charge collection is very fast. We estimate ~ 40ps.
• Due to drift based charge collection we have high radiation tolerance
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9FEE 2011, Ivan Peric
Strong points
• 1) Monolithic sensor
• 2) CMOS in-pixel electronics
• 3) Fast signal collection– Theoretically 40ps
• 4) Thinning possible– Since the charge collection is limited to the chip surface, the sensors can be thinned
• 5) Price and technology availability– Standard technology without any adjustment is used
– Many industry relevant applications of HV CMOS technologies assure their long tern availability
– 350nm technology: 8 inch wafer run: 90k€ (350nm)
– 180nm technology: 120k€ and 1.5k€/wafer (1 wafer ~ 200 cm2)
• 6) High tolerance to non-ionizing radiation damage – High drift speed
– Short drift path
• 7) High tolerance to ionizing radiation– Deep submicron technology
– Radiation tolerant design can be used
– PMOS transistors, that are more tolerant to radiation, can be used (in contrast to MAPS with high-resistance substrate)
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10FEE 2011, Ivan Peric
Drawbacks
• 1) Capacitive feedback– We can implement the majority of important pixel circuits in CMOS, like the charge sensitive
amplifier, shaper, tune DAC, SRAM but…
– “Digitally active” CMOS logic gates in pixels should be avoided
– Possibility 1: Current mode logic can be used instead CMOS (drawback – current consumption ~ 1 A / digital gate)
– Possibility 2: Separate digital and analog circuits (drawback – a few per cent of inactive area at the chip edge)
• 2) Relatively large size of the collecting electrode– Typical values for the total n-well capacitance are
– 10fF - small 21x21 m2 pixels and simple pixel electronics (already tested)
– 200fF 55x55 m2 CMOS pixels (already tested)
– 700fF 80x400 m2 CMOS pixels (proposed long pixels for SLHC)
• 3) Lower signals than in the case of fully depleted sensors– The signals do not decrease significantly after irradiation to 1015 neq cm2
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11FEE 2011, Ivan Peric
Results of the Project
• The SDAs have been developed within a small project whose aim was the proof of principle
• CMOS particle sensitive (“intelligent”) pixels in 350nm technology• In pixel hit-detection and binary trigger based readout (similar to ATLAS pixels). Pixel
size is 55x55m2 • Noise of 60e • Direct hit signal - 1800e, leading to a seed pixel SNR of 30 • Signal delay time ~ time resolution of the detector ~ 120ns • Part of the signal originates from the un-depleted bulk and is collected by diffusion –
impact on timing will be investigated on a test chip, probably not an issue • 4-transistor pixels (PM Chip) in 350nm technology• Test beam: • Efficiency 97.5%• MIP cluster signal is 2000e and seed pixel signal 1200e• The noise is about 44e that is twice as large as in lab tests – non-ideal setup• Seed pixel SNR is 27, Cluster Signal/Seed Noise = 47• We measure spatial resolution < 3.8μm
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12FEE 2011, Ivan Peric
„Intelligent“ particle sensitive pixel in 350nm technology
55m
Preamplifier (NMOS part)
Preamplifier (NMOS part)
RC-CR shaper
NMOS based comparator
4-bit threshold DAC
4-bit SRAM
CM NMOS logic
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13FEE 2011, Ivan Peric
„Intelligent“ particle sensitive pixel in 350nm technology
55m
Preamplifier (NMOS part)
Preamplifier (NMOS part)
RC-CR shaper
NMOS based comparator
4-bit threshold DAC
4-bit SRAM
CM NMOS logic
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14FEE 2011, Ivan Peric
4T pixel in 65nm technology
2.5m
Metal-metal coupling capacitor
Here only the standard N-Well has been used, only PMOS electronicsLower signals expected (small depleted volume)We hope to compensate this by lower detector capacitance
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15FEE 2011, Ivan Peric
Radiation tolerance
• In order to test the radiation tolerance we have performed a few irradiations
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16FEE 2011, Ivan Peric
Proton irradiation
• Proton irradiation of continuous readout pixels up to 1015 neq/cm2, which corresponds to a dose of ~300MRad in SiO2.
• As expected, we measure an increased noise. For example, at 20C we measure 270e. (We had 12e before irradiation.) However, only a light cooling leads to significant noise improvement, a sign that the noise is caused by leakage current. At 10C we have a noise of 77e and at -10 only 40e.
• We have measured the response to 22Na beta particles. SNR at -10C is 93.
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17FEE 2011, Ivan Peric
Irradiation with protons (1015 neq/cm2, 300 MRad)
0.00 0.02 0.04 0.06 0.08 0.100.0
0.2
0.4
0.6
0.8
1.0
~ n
um
be
r o
f sig
na
ls
signal amplitude [V]
RMS Noise 0.5mv (12e)
55Fe 70mV (1660e)Room temperature
0.00 0.02 0.04 0.06 0.08 0.100.0
0.2
0.4
0.6
0.8
1.0
~n
um
be
r o
f sig
na
lssignal amplitude [V]
RMS Noise, 2.8mv (77e)
55Fe, 60mV (1660e)Temperature 10C
Irradiated with protons to 1015neq
55Fe spectrum and RMS noiseNot irradiatedRoom temperature RMS Noise 12 e
55Fe spectrum, RMS noiseIrradiated10C RMS Noise 77 e
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18FEE 2011, Ivan Peric
Irradiation with protons (1015 neq/cm2, 300 MRad)
0.0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.80.0
0.2
0.4
0.6
0.8
1.0
~
nu
mb
er
of
sig
na
ls
signal amplitude [V]
RMS Noise (40e)
55Fe x-ray spectrum (Peak: 1660e)
22Na beta spectrum (Maximum: 3750e)
SNR = 93
-10C
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19FEE 2011, Ivan Peric
Particle sensitive pixels with CMOS electronics and continuous readout
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20FEE 2011, Ivan Peric
Signal detection
ComparatorCR-RC
CSA
N-well
AC coupling
3.3 V
-50 V
P-substrate
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21FEE 2011, Ivan Peric
Signal detection
ComparatorCR-RC
CSA
N-well
AC coupling
3.3 V
-50 V
P-substrate
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22FEE 2011, Ivan Peric
Signal detection
ComparatorCR-RC
CSA
N-well
AC coupling
3.3 V
-50 V
P-substrate
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23FEE 2011, Ivan Peric
Signal detection
ComparatorCR-RC
CSA
N-well
AC coupling
3.3 V
-50 V
P-substrate
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24FEE 2011, Ivan Peric
Signal detection
ComparatorCR-RC
CSA
N-well
AC coupling
3.3 V
-50 V
P-substrate
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25FEE 2011, Ivan Peric
Signal detection
ComparatorCR-RC
CSA
N-well
AC coupling
3.3 V
-50 V
P-substrate
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26FEE 2011, Ivan Peric
Signal detection
ComparatorCR-RC
CSA
N-well
AC coupling
3.3 V
-50 V
P-substrate
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27FEE 2011, Ivan Peric
Signal detection
ComparatorCR-RC
CSA
N-well
AC coupling
3.3 V
-50 V
P-substrate
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28FEE 2011, Ivan Peric
Intelligent particle sensitive pixels – possible application
• Vertex detector for the novel experiment. Goal: search for lepton flavor violating decay -> eee
• Four layers of pixels ~ 80x80m2 size
• Continuous muon beam stopped at target – 109 muon stops/s –> requires time stamping with ~ 100ns resolution
• Energy range of interest: 15-50MeV –> multiple scattering dominates momentum measurement –> ~50 m thin detector
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29FEE 2011, Ivan Peric
Multi-reticle module
Reticle1
Chip1
Pads
Chip to chip connections
Chip to reticle edge distance = 80 um
Chip2
Chip1
Chip2
Reticle2
2.0 cm
Module
Pixel modules with (almost) no insensitive area can be producedReticle-reticle connections can be made easily by wire bondingInstead of wire-bonding, an extra metal layer can be used as well
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30FEE 2011, Ivan Peric
Low-mass detector
Carrier
Module (length. 12 cm, width 1cm, the figure is not scaled)
Pads for power and IO signals
chip to chip connections
Chip (reticle 3)
Interaction region
Large sensitive area without material
Chip (reticle 2)
Very low-mass only silicon module
Wire as support
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31FEE 2011, Ivan Peric
Analog Pixel
CSA
Comparator
N-well
P-substrate
ThresholdDAC
Bias Volt.
To digital channel
SRAM
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32FEE 2011, Ivan Peric
Digital Channel
S
R
LERAM
AddrROM
Time Stamp Data BusPriority Out
Priority In
Read
Hit
From Analog Pixel
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33FEE 2011, Ivan Peric
Detector with separated analog and digital pixels
1cm
2cm
~125 pixel rows(80 μm pitch)
250 pixel rows(80 μm pitch)
Digital Channels
Analog Pixels – Sensitive Area
Reticle1
Analog Pixels
Digital Channels
~0.75mm
LVDS OutThe figure shows one reticle
~0.7m
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34FEE 2011, Ivan Peric
Test Chip in 180nm technology
30m
39m
0.7m
2 metal layers
An
alo
g p
ixels
Dig
ital ch
an
ne
ls
1.8mm
42x36 pixels
Analog pixel layout
Pixel is made smaller than neededThis has positive impact on detector capacitance
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35FEE 2011, Ivan Peric
Analog Pixel
CSA
Buffer
N-well
P-substrate
Bias Volt.
To digital channel
The analog pixel is slightly different than required for the final designComparator, tune DAC and SRAM are missing (placed in the digital channel)
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36FEE 2011, Ivan Peric
Digital Channel with tune DAC
Comparator
InTrigger
Reset
In
ThresholdDACLatch
ROEn
HitEn
Base line
Global thr.
Hit bus Data out
The digital channel is slightly different than required for the final designSimilar number of transistors
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37FEE 2011, Ivan Peric
Digital Channel with e-fuse
Comparator
In„1“
Reset
In
ROEn
HitEn
1.8V
3.6V
x
y
Base line
or global thr.
Idea: Strasbourg “MAPS” group (A. Dorokhov)
E-fuse
E-fuse substitutes threshold tune DAC -> smaller layout
E-fuse requires high voltage to be “burned”
This NMOS takes care that the other transistors do not see the high voltage required for “burning” the fuse
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38FEE 2011, Ivan Peric
Digital Channels
12m
39m DAC
Latches
Fuse
Fuse-“addressing“ transistors
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39FEE 2011, Ivan Peric
Time walk - simulation
Power in analog pixel ~ only 8W
6 sigma noise
6000e
1200e
7ns!!!
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40FEE 2011, Ivan Peric
Integrating pixels
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41FEE 2011, Ivan Peric
Integrating pixels with source follower readout
Out
Res Res Sel
3.3V
2V
-60V
Source followerSensordiode
Only PMOS transistors -> no need for P-Well
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42FEE 2011, Ivan Peric
Integrating pixels with source follower readout
Out
Res Res Sel
-60V
3.3V
2V
Reset phase
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43FEE 2011, Ivan Peric
Integrating pixels with source follower readout
Out
Sel
-60V
Signal detection phase
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44FEE 2011, Ivan Peric
Integrating pixels with source follower readout
Out
Sel
-60V
Q
Q/Cdet
Cdet
Signal detection phase
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45FEE 2011, Ivan Peric
Integrating pixels with source follower readout
Out
Res Res Sel
3.3V
2V
-60V
Source follower
Leakage current -> noise, pedestal dispersion
Threshold dispersion -> pedestal dispersion
The main problems:KTC noise -> requires CDSLeakage current (leakage of PMOS switches probably dominates)Leakage current causes noise and pedestal dispersionThreshold dispersion
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46FEE 2011, Ivan Peric
Integrating pixels with voltage amplification
Out
VP
Res
Res Sel
VP
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47FEE 2011, Ivan Peric
Integrating pixels with voltage amplification
Out
VP
Res
Res Sel
VP
Reset phase
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48FEE 2011, Ivan Peric
Integrating pixels with voltage amplification
OutSel
VP
Signal detection phase
Charge sensitive amplifier
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49FEE 2011, Ivan Peric
Integrating pixels with voltage amplification
OutSel
VP
Q
CfQ/Cf
Signal detection phase
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50FEE 2011, Ivan Peric
Integrating pixels with voltage amplification
Out
VP
Res
Res Sel
VP
Leakage current -> noise, pedestal dispersionGets worse with higher reverse biasProbably a kind of back gate effectMore pronounced than in source follower pixels
The main problems:KTC noise -> requires CDSPMOS leakage currentThreshold dispersion is not the issue since its effect is reduced by applied gain
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51FEE 2011, Ivan Peric
Integrating pixels with CDS
Out
VP
Res
Res Sel
VP
Sel
Sample
Sel
~100fF sampling capacitor to store the reset value for duration of one frame
A few NMOS transistors in pixel required -> P-Well is mandatory
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52FEE 2011, Ivan Peric
Integrating pixels with CDS - simulation
Pixel1 Pixel2
Pre signal reset val.
Signal - reset
Post. signal noisy reset val. Noiseless reset
Signal – reset did not change although the new reset value is different
Transient noise simulation
The reset val. Is stored for the duration of one frame
SelSample
Reset
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53FEE 2011, Ivan Peric
PM2 chip (known in Eudet community as „Taki“)2
.7 m
m
ADC channel
Pixel matrix
Pixels with voltage amplification (64x128)
Pixels with SF readout (64x128)
LVDS digital I/Os
Analog pads
2-stage switched capacitor difference amplifier
Single ramp ADC
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54FEE 2011, Ivan PericADC
Row
-contro
l („Sw
itcher“)
Digital output
10000001000
Pixel size: 21 X 21 m Matrix size: 2.69 X 2.69 mm (128 X 128) Possible readout time/matrix (400MHz clock): ~ 40 s (320ns/row) (tested so far 1.28 s/row (2.56 CDS)) ADC: 8 – Bit Analog power: 43mW/chip, 0.33mW/ADC (90μA+10 μA)Digital power: 538mW/chip at 400MHz clock, 160mA Digital power can be reduced to 40mW (factor 14!) by reducing digital supply and improving flip-flop designIn 180nm technology digital power would be only 12mW
8 LVDS
Counter
Amplifier
Comparator
Latch
Ramp gen.
PM2 chip structure
Pixel matrix
![Page 55: Monolithic sensors in high-voltage deep-submicron technology](https://reader035.vdocument.in/reader035/viewer/2022062801/56814395550346895db01178/html5/thumbnails/55.jpg)
55FEE 2011, Ivan Peric
Integrating pixels with SF readout –experimental results
![Page 56: Monolithic sensors in high-voltage deep-submicron technology](https://reader035.vdocument.in/reader035/viewer/2022062801/56814395550346895db01178/html5/thumbnails/56.jpg)
56FEE 2011, Ivan Peric
Laboratory measurement with radioactive sources
The spectrum has been measured with 22Na beta source at room temperatureMost probable cluster signal: 2905eMost probable single pixel signal ~1660 eNoise: 31eSNR single pixel = 54SNR cluster signal to single pixel noise = 94Integration time 160 s
0 100 200 300 400 5000.0
0.2
0.4
0.6
0.8
1.0
~ n
umbe
r of
sig
nals
ADC
22Na cluster (2905e) 55Fe single pixel (1660e) 22Na single pixel (~1660e) Noise (31e)
![Page 57: Monolithic sensors in high-voltage deep-submicron technology](https://reader035.vdocument.in/reader035/viewer/2022062801/56814395550346895db01178/html5/thumbnails/57.jpg)
57FEE 2011, Ivan Peric
Test beam at CERN (SPS) with Eudet Mimosa 26 telescope
Pixel signals corrected for pedestal distribution (base-line noise)
ADU
num
ber
of s
igna
ls Gaussian fit: sigma = 0.743 (44 e)
Common mode correction(all frames)
ADU
num
ber
of s
igna
ls Gaussian fit: sigma = 0.152 (9 e)
Base line noise – the pixel signals corrected for pedestal distribution, all pixel in one frame are shown
Common mode noise – common mode correction values for all frames and rows
Noise measurement
![Page 58: Monolithic sensors in high-voltage deep-submicron technology](https://reader035.vdocument.in/reader035/viewer/2022062801/56814395550346895db01178/html5/thumbnails/58.jpg)
58FEE 2011, Ivan Peric
Test beam: Signal
Seed pixel 2 MSP 3 MSP
7 MSP
ADU
num
ber
of s
igna
ls
Signal spectra in AD units depending on number of pixels in a cluster
![Page 59: Monolithic sensors in high-voltage deep-submicron technology](https://reader035.vdocument.in/reader035/viewer/2022062801/56814395550346895db01178/html5/thumbnails/59.jpg)
59FEE 2011, Ivan Peric
Test beam: Signal (2)
1 2 3 4 5 6 70
250
500
750
1000
1250
1500
1750
2000
2250
2500
2750
3000
3250
Mo
st p
rob
ab
le s
ign
al [
e]
Number of pixels
55Na
60Co MIPs
High energy particle signals depending on number of pixels in cluster
Single pixel signal1200 e
Cluster signal2000 e
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60FEE 2011, Ivan Peric
Test beam: SNR
Seed pixel SNR
SNR
num
ber
of s
igna
ls
Seed pixel SNR = 27
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61FEE 2011, Ivan Peric
Test beam: SNR
1 2 3 4 5 6 70.0
2.5
5.0
7.5
10.0
12.5
15.0
17.5
20.0
22.5
25.0
27.5
30.0
SN
R
Number of pixels
SNR
Cluster signal to noise ratio (MPX) vs. number of pixels in cluster
Single pixel SNR = 27
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62FEE 2011, Ivan Peric
Test beam: “fake” SNR
SNR as cluster signal over seed pixel noise
SNR
num
ber
of s
igna
ls
Fake SNR spectrum of the clusters. Fake SNR is here defined as the total cluster charge divided by the seed pixel noise.
Fake SNR = 47
![Page 63: Monolithic sensors in high-voltage deep-submicron technology](https://reader035.vdocument.in/reader035/viewer/2022062801/56814395550346895db01178/html5/thumbnails/63.jpg)
63FEE 2011, Ivan Peric
Test Beam: efficiency
Efficiency vs pixel xy-coordinates(Mean value = 0.9761)
X pixel
Y p
ixel
Fig “Efixy”: 2D distribution of the detector efficiency.
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64FEE 2011, Ivan Peric
Test Beam: Spatial Resolution
Spatial resolution in y-directionGaussian fit: sigma = 4.431 m
Y -Y [ m]DUT TEL
num
ber
of h
its
Distribution of the differences between the measured and the fitted y hit-coordinate.
![Page 65: Monolithic sensors in high-voltage deep-submicron technology](https://reader035.vdocument.in/reader035/viewer/2022062801/56814395550346895db01178/html5/thumbnails/65.jpg)
65FEE 2011, Ivan Peric
Test Beam: Spatial Resolution (2)
4.4311
5.36844
4.95608
3.7842
4.84826
4.38728
A B C0
1
2
3
4
5
Sp
atia
l re
solu
tion
in Y
dir
ect
ion
[ m
]
without correction corrected for telescope error
6.31243
7.099016.61151
5.54876
6.42946
5.88677
A B C0
1
2
3
4
5
6
7
Sp
atia
l re
solu
tion
in X
dir
ect
ion
[m
]
without correction corrected for telescope error
Spatial resolution of the DUT in y direction. The black rectangles show the measured and red rectangles the exact spatial resolutions of the DUT corrected for the telescope error. In the cases A and B we used the eta-corrected CoG, and in the case C only the raw CoG corrections. The corrections were calculated only with 3 most significant pixels of a cluster in the case B.
Figure „ResAllx“: Spatial resolution of the DUT in x direction.
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66FEE 2011, Ivan Peric
Integrating pixels with voltage amplification –experimental results
![Page 67: Monolithic sensors in high-voltage deep-submicron technology](https://reader035.vdocument.in/reader035/viewer/2022062801/56814395550346895db01178/html5/thumbnails/67.jpg)
67FEE 2011, Ivan Peric
Noise measurement and 55Fe spectrum
50 60 70 80 90 100 110 120 130 140 150 160 1700.0
0.2
0.4
0.6
0.8
1.0
~
nu
mb
er o
f sig
na
ls
ADU
55Fe, 1 pixel, 76 ADU, (1660e) Noise 1.1 ADU (24e)
Noise: 24eDKS used
55Fe1660e
Sensor has been cooled with a small Peltier cooler: T ~ (?) 10C
![Page 68: Monolithic sensors in high-voltage deep-submicron technology](https://reader035.vdocument.in/reader035/viewer/2022062801/56814395550346895db01178/html5/thumbnails/68.jpg)
68FEE 2011, Ivan Peric
High-energy beta spectra
0 1000 2000 3000 4000 5000 6000 7000 80000.0
0.2
0.4
0.6
0.8
1.0
~n
um
be
r o
f sig
na
ls
signal amplitude [e]
Noise, 1 pixel (21e)
60Co, 1 pixel (1700e)
60Co, 2 pixels (1800e)
60Co, 3 pixels (1900e)
60Co, 4 pixels (2250e)
0 1000 2000 3000 4000 5000 6000 7000 80000.0
0.2
0.4
0.6
0.8
1.0
~n
um
be
r o
f sig
na
lssignal amplitude [e]
Noise, 1 pixel (21e)
22Na, 1 pixels (1900e)
22Na, 2 pixels (2200e)
22Na, 3 pixels (2500e)
22Na, 9 pixels (3300e)
60Co betas (about 10% higher signals than MIPs)Seed signal: 1700eCluster signal: 2250eNoise: 21eSeed SNR: 81Cluster signal/seed noise: 107
55Na betasSeed signal: 1900eCluster signal: 3300eNoise: 21eSeed SNR: 90Cluster signal/seed noise: 157
Estimated MIP seed pixel SNR: 57Cluster signal/seed noise: 95
![Page 69: Monolithic sensors in high-voltage deep-submicron technology](https://reader035.vdocument.in/reader035/viewer/2022062801/56814395550346895db01178/html5/thumbnails/69.jpg)
69FEE 2011, Ivan Peric
Long module
6 cm
1 cm
Half module size 1x6cm Pixel size 40x40μm Pixels 250x1500 RO time 80μs/matrix Resolution 7(!) bit/pixel (count up to 125) – if CDS pixels are used, we need probably only 6 bits Power 960mW/module (150mW/cm2 (80 analog + 70 digital)) Data output width 7x12 = 84 bits @ 400Mbit180nm Technology:Power 210mW/module (35mW/cm2 (14 analog + 21 digital))20μs/matrix possible – power 140mW/cm2
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70FEE 2011, Ivan Peric
Summary
• We have developed a new pixel sensor structure (smart diode array) for high energy physics that can be implemented in a high voltage CMOS technology.
• The sensor has 100% fill-factor and can have in-pixel electronics implemented with p- and n-channel transistors.
• We have tested the sensor structure in various variants:• 1) Sensor with in-pixel hit detection and sparse readout, • 2) Sensor with fast rolling-shutter readout and simple pixel electronics• We have done three test-beam measurements with good results.
– Detection efficiency 98%– Seed Pixel SNR ~ 27– Cluster Signal/Seed Pixel Noise ~ 47– Spatial resolution ~ 3.8 m
• We have irradiated the chips with neutrons, protons and x-rays to test radiation tolerance.
• After irradiation with protons up to very high fluence 1015 neq/cm2 and dose 300MRad, we have still very large SNR (>40) for high energy beta particles at nearly room temperatures (10C).
• We have submitted a new test-chip in 180nm technology• We are planning an engineering run either in 350nm or in 180nm technology,
probably with two detectors, one for muon experiment (CMOS pixels) and one for electron microscopy (integrating pixels)
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71FEE 2011, Ivan Peric
• Thank you!
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72FEE 2011, Ivan Peric
• Backup slides
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73FEE 2011, Ivan Peric
Integrating pixels with source follower readout
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74FEE 2011, Ivan Peric
ResetB
ResetNWB SelB
Out
VN
N-Well
P-Substrate
VP
Out
Pixels with SF RO – signal detection phase
VPVNResNWB SelB
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75FEE 2011, Ivan Peric
ResetB
ResetNWB SelB
Out
VN
Out
Hit
VPVNResNWB SelB
VP
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76FEE 2011, Ivan Peric
ResetB
ResetNWB SelB
Out
VN
Out
Charge collection
VPVNResNWB SelB
VP
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77FEE 2011, Ivan Peric
ResetB
ResetNWB SelB
Out
VN
Out
Readout phase
VPVNResNWB SelB
VP
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78FEE 2011, Ivan Peric
ResetB
ResetNWB SelB
Out
VN
Out
Readout phase
VPVNResNWB SelB
VP Signal
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79FEE 2011, Ivan Peric
ResetB
ResetNWB SelB
Out
VN
Out
Reset
VPVNResNWB SelB
VP Signal
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80FEE 2011, Ivan Peric
ResetB
ResetNWB SelB
Out
VN
Out
Reset
VPVNResNWB SelB
VP Signal
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81FEE 2011, Ivan Peric
ResetB
ResetNWB SelB
Out
VN
Out
Reset + offset readout
VPVNResNWB SelB
VP
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82FEE 2011, Ivan Peric
ResetB
ResetNWB SelB
Out
VN
Out
End of readout
VPVNResNWB SelB
VP
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83FEE 2011, Ivan Peric
Integrating pixels with voltage amplification
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84FEE 2011, Ivan Peric
ResetB
ResetNWB
SelB
VP
Pixel with volt. amplification – signal detection phase
VP
VPResNWB SelBVP
Out
Pixel
Out
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85FEE 2011, Ivan Peric
ResetB
ResetNWB
SelB
VP
Hit
VPOut
VPResNWB SelBVP
Out
Pixel
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86FEE 2011, Ivan Peric
ResetB
ResetNWB
SelB
VP
Charge collection
VPOut
VPResNWB SelBVP
Out
Pixel
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87FEE 2011, Ivan Peric
ResetB
ResetNWB
SelB
VP
Readout phase
VPOut
VPResNWB SelBVP
Out
Pixel
![Page 88: Monolithic sensors in high-voltage deep-submicron technology](https://reader035.vdocument.in/reader035/viewer/2022062801/56814395550346895db01178/html5/thumbnails/88.jpg)
88FEE 2011, Ivan Peric
ResetB
ResetNWB
SelB
VP
Readout phase
VPOut
VPResNWB SelBVP
Out
Pixel
![Page 89: Monolithic sensors in high-voltage deep-submicron technology](https://reader035.vdocument.in/reader035/viewer/2022062801/56814395550346895db01178/html5/thumbnails/89.jpg)
89FEE 2011, Ivan Peric
ResetB
ResetNWB
SelB
VP
Readout – voltage amplification
VP
Out
VPResNWB SelBVP
Out
Pixel
Amplified Signal
![Page 90: Monolithic sensors in high-voltage deep-submicron technology](https://reader035.vdocument.in/reader035/viewer/2022062801/56814395550346895db01178/html5/thumbnails/90.jpg)
90FEE 2011, Ivan Peric
ResetB
ResetNWB
SelB
VP
Readout – voltage amplification
VP
VPResNWB SelBVP
Pixel
Out
Amplified Signal
Out
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91FEE 2011, Ivan Peric
ResetB
ResetNWB
SelB
VP
Reset
VP
VPResNWB SelBVP
Pixel
Out
Amplified Signal
Out
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92FEE 2011, Ivan Peric
ResetB
ResetNWB
SelB
VP
Reset + offset readout
VPOut
VPResNWB SelBVP
Out
Pixel
Out
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93FEE 2011, Ivan Peric
ResetB
ResetNWB
SelB
VP
End of readout
VPOut
VPResNWB SelBVP
Out
Pixel
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94FEE 2011, Ivan Peric
Pixel Electronics for SLHC
• The pixel electronics could include a charge sensitive amplifier (CSA), leakage current compensation, continuous feedback, comparator and threshold tune DAC.
• The digital circuits inside pixel should be as simple as possible• The idea:• The addresses of all hit pixels are transmitted out of the sensor within next bunch
crossing• No hit buffering• No trigger data reduction• Assumption: occupancy is low enough so that we do not have not more than one hit
per pixel column in one bunch crossing. This holds for R ~ 30 - 50cm
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95FEE 2011, Ivan Peric
Capacitance of long pixels
N-well
P-substrate
P-well
400um60um
~200fF
~500fF (C_area = 0.014fF/um2)
Total 700fF
![Page 96: Monolithic sensors in high-voltage deep-submicron technology](https://reader035.vdocument.in/reader035/viewer/2022062801/56814395550346895db01178/html5/thumbnails/96.jpg)
96FEE 2011, Ivan Peric
Pixel Electronics for SLHC
CSA
Comparator
N-well
P-substrate
ThresholdDAC
Bias Volt.
ADDRROM
100MHz
In
In
„1“
![Page 97: Monolithic sensors in high-voltage deep-submicron technology](https://reader035.vdocument.in/reader035/viewer/2022062801/56814395550346895db01178/html5/thumbnails/97.jpg)
97FEE 2011, Ivan Peric
Pixel Electronics for SLHC
ADDRROM
In
In
„1“
ADDRROM
In
In
„1“
Hit in Pixel A
Address „A“ on the data line
Time signal 1
Hit in Pixel B
Address „B“ on the data line
Time signal 2
![Page 98: Monolithic sensors in high-voltage deep-submicron technology](https://reader035.vdocument.in/reader035/viewer/2022062801/56814395550346895db01178/html5/thumbnails/98.jpg)
98FEE 2011, Ivan Peric
Sensor Chip Architecture for SLHC
2cm
250 pixel rows(80 μm pitch)
50 pixel rows(400 μm pitch)
Reticle
1. Sensor reticule
2. Pixel column
Normal pixels
Readout pixel
Signal path
GBit fast shift register
Digital readout chipperforms digital data processing
GBit Pads
Power 30 μW/pixel375mW / reticle94mW / cm2
Current 288mA / reticle
Hit
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99FEE 2011, Ivan Peric
4-Reticle Module for SLHC
Power lines on the sensor chip
Reticle-reticle connections
Digital readout chip
Signal lines on the sensor chip
4cm
Capton PCB
Signals
Power
Pixel orientation
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100FEE 2011, Ivan Peric
Double-Layer Modules
Digital readout chips receive the hits from both detector layers Generation of trigger possible?
Pads
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101FEE 2011, Ivan Peric
Time Resolution
• Time resolution is limited by time walk (can be improved by ToT correction!)• Time resolution is proportional to preamplifier bias current and power consumption• Time resolution is inversely proportional to detector capacitance
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102FEE 2011, Ivan Peric
Time walk for 24μW pixel amplifier and 700fF detector capacitance - simulation
22ns time walk
6 sigma noise (24mV)
100.0n 150.0n 200.0n 250.0n 300.0n0.00
0.02
0.04
0.06
0.08
0.10
0.12
0.14
0.16
Out
put
Vol
tage
[V
]
Time
1500e 2625e 3750e 4875e 6000e
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103FEE 2011, Ivan Peric
Time Resolution with HV1
0 10 20 30 40 50 6048
50
52
54
56
58
60
62
Response timeThreshold: 720 eSignal: 1110 e
Noise
DAC setting
No
ise
/e
100
110
120
130
140
150
160
Re
spon
se tim
e/n
s1 2 3 4 5 6 7 8 9
20
40
60
80
100
120 Separated diodeRegular pixel
Inpu
t no
ise/
eAmplifier bias / A
Response time ~ time resolution
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104FEE 2011, Ivan Peric
Irradiation with neutrons (1014 neq/cm2) – signal
0 1 2 3 4 5 60
200
400
600
800
1000
1200
1400
1600
1800
2000
2200
2400 60Co Irradiated chip (1014 n
eq)
Not irradiated
Sig
nal [
e]
Number of pixels in cluster
IrradiatedNot irradiated
Increase of the detector leakage current from 350fA to 130pA per pixelSeed pixel signal decrease from 1300e to 1000e. The measurement has been performed at 0C
0 1000 2000 3000 4000 5000 60000
50
100
150
200
250
300
350
Num
ber
of h
itsSignal [e]
1 MSP 2 MSP 3 MSP 4 MSP 5 MSP 6 MSP
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105FEE 2011, Ivan Peric
Irradiation with neutrons (1014 neq/cm2) – noise
0.00 0.05 0.10 0.150.0
0.2
0.4
0.6
0.8
1.0
~n
um
be
r o
f sig
na
ls
signal amplitude [V]
noise amplitude 3 = 3mv (3 = 50e)
55Fe 100mv (1660e)
Irradiated with neutrons to 1014 neq
Room temperature
0.00 0.02 0.04 0.06 0.08 0.100.0
0.2
0.4
0.6
0.8
1.0
~ n
um
be
r o
f sig
na
ls
signal amplitude [V]
RMS Noise 0.5mv (12e)
55Fe 70mV (1660e)Room temperature
55Fe spectrum and RMS noiseNot irradiatedRoom temperature RMS Noise 12 e
55Fe spectrum and noise amplitudeIrradiated with neutrons (1014 neq)Room temperature Noise amplitude (~3 sigma) ~ 50 e
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106FEE 2011, Ivan Peric
Irradiation with protons (1015 neq/cm2, 300 MRad)
0.00 0.02 0.04 0.06 0.08 0.100.0
0.2
0.4
0.6
0.8
1.0
~
nu
mb
er
of s
ign
als
signal amplitude [V]
RMS Noise 0.5mv (12e)
55Fe 70mV (1660e)Room temperature
0.00 0.02 0.04 0.06 0.08 0.10 0.120.0
0.2
0.4
0.6
0.8
1.0
~n
um
be
r o
f sig
na
ls
signal amplitude [V]
RMS Noise, 13mv (270e)
55Fe, 80mV (1660e)Temperature 20C
Irradiated with protons to 1015neq
0.00 0.02 0.04 0.06 0.08 0.100.0
0.2
0.4
0.6
0.8
1.0
~n
um
be
r o
f sig
na
ls
signal amplitude [V]
RMS Noise, 2.8mv (77e)
55Fe, 60mV (1660e)Temperature 10C
Irradiated with protons to 1015neq
0.00 0.02 0.04 0.06 0.08 0.10 0.12 0.14 0.160.0
0.2
0.4
0.6
0.8
1.0
~n
um
be
r o
f sig
na
ls
signal amplitude [V]
RMS Noise, 2.4mv (40e)
55Fe, 100mV (1660e)Temperature -10C
Irradiated with protons to 1015neq
55Fe spectrum and RMS noiseNot irradiatedRoom temperature RMS Noise 12 e
55Fe spectrum and RMS noiseIrradiated20C RMS Noise 270 e
55Fe spectrum, RMS noiseIrradiated-10C RMS Noise 40 e
55Fe spectrum, RMS noiseIrradiated10C RMS Noise 77 e
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107FEE 2011, Ivan Peric
Irradiation with protons (1015 neq/cm2, 300 MRad)
0.0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.80.0
0.2
0.4
0.6
0.8
1.0
~
nu
mb
er
of s
ign
als
signal amplitude [V]
22Na - 0V bias (0.075V or 1250e)
22Na - 30V bias (0.18V or 3125e)
22Na - 60V bias (0.22V or 3750e)
55Fe - 60V bias (100mV or 1660e) RMS Noise (2.4mV or 40e)
Temperature: - 10C
Irradiated with protons to 1015neq
55Na spectra, -10C
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108FEE 2011, Ivan Peric
Irradiation with protons (1015 neq/cm2, 300 MRad)
0.0 0.2 0.4 0.6 0.80.0
0.2
0.4
0.6
0.8
1.0
~n
um
be
r o
f sig
na
ls
signal amplitude [V]
RMS Noise, 2.4mv (40e)
55Fe, 100mV (1660e)
55Na, 220mV (3750e)Temperature -10C
Irradiated with protons to 1015neq
0.0 0.2 0.4 0.6 0.80.0
0.2
0.4
0.6
0.8
1.0
~n
um
be
r o
f sig
na
ls
signal amplitude [V]
RMS Noise, 2.8mv (77e)
55Fe, 60mV (1660e)
55Na, 180mV (4980e)Temperature 10C
Irradiated with protons to 1015neq
0.0 0.2 0.4 0.6 0.80.0
0.2
0.4
0.6
0.8
1.0
~n
um
be
r o
f sig
na
ls
signal amplitude [V]
RMS Noise, 13mv (270e)
55Fe, 80mV (1660e)
55Na, 200mV (4150e)Temperature 20C
Irradiated with protons to 1015neq
55Fe and 22Na spectrum, RMS noiseIrradiatedTemperature 20CRMS Noise 270 eSNR = 15
55Fe and 22Na spectrum, RMS noiseIrradiatedTemperature 10CRMS Noise 77 eSNR = 64
55Fe and 22Na spectrum, RMS noiseIrradiatedTemperature -10CRMS Noise 40 eSNR = 93
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109FEE 2011, Ivan Peric
Irradiation x-rays (50 MRad)
600 700 800 900 1000 11000.0
0.2
0.4
0.6
0.8
1.0
resp
on
se p
rob
ab
ility
signal amplitude [e]
Response probabilityfit: sgma = 72e, mean = 750eNot irradiatedRoom temperature
500 600 700 800 900 10000.0
0.2
0.4
0.6
0.8
1.0
resp
on
se p
rob
ab
lility
signal amplitude [e]
Response probabilityfit: sgma = 83e, mean = 610eIrradiated with x-rays to 60MRadTemperature 5CNoise
Before irradiationRoom TemperatureNoise 72e
NoiseAfter irradiationTemperature 5CNoise 83e
0 20 40 60 80 100 1200
50
100
150
200
250
300
350
400
NoiseRoom temperature annealiingday 0: irradiation with x-rays to 60MRadday 5: 24 hours at 80C
no
ise
[e]
annealing time [days]
Noise at room TemperatureVs. annealing time
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110FEE 2011, Ivan Peric
Irradiation x-rays (50 MRad)
0 25 50 750
20
40
60
80
100
120
140
~n
um
be
r o
f sig
na
ls
signal duration [clock periodes]
55Feirradiated with x-rays to 60MRadTemeperature 5C
0 1000 2000 3000 4000 5000 6000 7000 8000 9000 100000
250
500
750
1000
~N
um
be
r o
f hits
Singnal/e
55Na beta signalIrradiated with x-rays to 60MRadTemperature 5C
0 25 50 75 100 125 150 175 200 225 250
0.0
0.2
0.4
0.6
0.8
1.0
~
sig
na
l pro
ba
bili
ty
signal duraion [clock periodes]
Not irradiated (room T) Irradiated with x-rays to 60MRad (5C)
22Na spectrum
22Na spectrum
22Fe spectrum
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111FEE 2011, Ivan Peric
Project overview
First chip – CMOS pixelsHit detection in pixels
Binary ROPixel size 55x55μm
Noise: 60eMIP seed pixel signal 1800 e
Time resolution 200ns
CCPD1 ChipBumpless hybrid detector
Based on capacitive chip to chipsignal transfer
Pixel size 78x60μmRO type: capacitive
Noise: 80eMIP signal 1800e
CCPD2 ChipEdgeless CCPD
Pixel size 50x50μmNoise: 30-40e
Time resolution 300nsSNR 45-60
PM1 ChipPixel size 21x21μm
Frame mode readout4 PMOS pixel electronics
128 on chip ADCsNoise: 90e
Test-beam: MIP signal 2200e/1300eEfficiency > 85% (timing problem)
Spatial resolution 7μmUniform detection
PM2 ChipNoise: 21e (lab) - 44e (test beam)
Test beam: Detection efficiency 98%Seed Pixel SNR ~ 27
Cluster Signal/Seed Pixel Noise ~ 47Spatial resolution ~ 3.8 m
Irradiations of test pixels60MRad – SNR 22 at 10C (CCPD1)
1015neq SNR 50 at 10C (CCPD2)
Frame readout - monolithicBumpless hybrid detector
1.5 mm
Readout chip (CAPPIX)
Sensor chip (CAPSENSE)
Power supplyand cont. signalsfor the sensor
Power supplyand cont. signalsfor the readout chip
Testbeam DESY
Testbeam CERN
EUDET telescope
DUT
DUT
0 5 10 15 20 25 30 35 40 45 500
100
200
300
400
500
600
700
800
seed p ix e l3 M S P
w h o le c lu s te r
S N R
coun
t
MIP spectrum (CERN SpS - 120GeV protons)
Testchip
PCB
PCB with PPGA and analog supply voltage regulators/DACs
60V bias voltage (3 batteries)
Trigger ID
USB connector
2.5 3.5 4.5 5.5 6.5 7.5 8.5 9.5 10.5 11.5T
T^ 4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0 8.5
10%
20%
30%
40%
50%
60%
70%
80%
90%
100%
Efficiency
Purity
0
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0.8
0.9
1
0 20 40 60 80 100 1200
10
20
30
40
50
60
effic iencyeffic iency
pixel coordinate x
pix
el
coo
rdin
ate
yEfficiency
Seed and cluster cut [SNR]
2.7
mm
ADC channel
Pixel matrix
ComparatorCR-RC
CSA
N-well
AC coupling
3.3 V
-50 V
P-substrate
0 100 200 300 400 500 600 700 8000
20
40
60
80
100
120
140
160
180
200
220Sr-90, Regular pixel, 55V
Num
ber
of h
its
ToT/Clk
MIP Signal: 2000e/1.17 = 1710 eLow energy peak:1.080 e
a)b)
0 100 200 300 400 500 600 700 8000,0
0,1
0,2
0,3
0,4
0,5
0,6
0,7
0,8
0,9
1,0
1,1
Regular pixel, 55V
Fe-55 Sr-90
~hi
t pr
obab
ility
ToT/Clk
Sensor pixels
Readout electrodes
Pads for power and signals