Status and perspectives of solid state photon detectors...High-field region. Poly strip resistor....
Transcript of Status and perspectives of solid state photon detectors...High-field region. Poly strip resistor....
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Status and perspectives of solid state photon detectors
Yu. MusienkoUniversity of Notre Dame (Notre Dame)
&INR RAS (Moscow)
RICH-2016, 6 September 2016, Bled, Slovenia 1
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SSPD talks at previous RICH conferences
Yu. Musienko, RICH-2016 2
Excellent reviews on SSPDs were presented at previous RICH conferences. Description of the principles and physics of operation you can find there…
In my presentation I will concentrate on the most recent developments and perspectives in SSPDs (especially in SiPMs).
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Introduction
Yu. Musienko, RICH-2016 3
At RICH-2013 workshop: excellent review on SiPMs by G. Collazuol: improvedunderstanding of SiPM physics was demonstrated.As a result (2016) significant progress in SiPM developmentGeneral trend : reduce correlated noise (X-talk, afterpulsing), improve PDE,reduce dark noise
Here I will review current (September 2016) status of SSPM development.Possible perspectives of SSPM development will be also discussed.I will use some of results presented at NDIP-14, PD-15, VCI-16, Elba-15, 2ndSiPM Advanced workshop-Geneva-2014
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Silicon photomultipliers (SiPMs)
Yu. Musienko, RICH-2016 4
Structure and principles of operation (briefly)
Al electrodeRquench
n+/p junctions
p-Si substrate
SiO2+Si3N4p-epi layer
300µ
2-4µ
(EDIT-2011, CERN)
Vbias> VBD
GM-APD
Rq
substrate
Al electrodeVout
Q Q
Qtot = 2Q
• SiPM is an array of small cells (SPADs) connected in parallel on a common substrate• Each cell has its own quenching resistor (from 100kΩ to several MΩ)• Common bias is applied to all cells (~10-20% over breakdown voltage)• Cells fire independently• The output signal is a sum of signals produced by individual cellsFor small light pulses (Nγ<<Npixels) SiPM works as an analog photon detector
The very first metall-resitor-smiconductor APD (MRS APD) proposed in 1989 by A. Gasanov, V. Golovin, Z. Sadygov, N. Yusipov (Russian patent #1702831, from 10/11/1989 ). APDs up to 5x5 mm2 were produced by MELZ factory (Moscow).
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SiPMs: Optical cross-talk between cells (direct cross-talk)
Yu. Musienko, RICH-2016 5
Hot-carrier luminescence:105 carriers produces ~3 photons with anwavelength less than 1 µm.Increases with the gain !Optical cross-talk causes adjacent pixels to befired increases gainfluctuations increases noise and excessnoise factor !
(R. Mirzoyan, NDIP08, Aix-les-Bains)
N.Otte, SNIC-2006
Avalanche luminescence
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SiPMs: Optical cross-talk - II
Yu. Musienko, RICH-2016 6
Other effects of cell luminescence:- External cross-talk- Delayed pulses from
light absorbed in non-depleted region (look like after-pulses)
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SiPMs: After-pulses
Yu. Musienko, RICH-2016 7
Carriers trapped during the avalanche discharging and then released trigger a new avalanche during a period of several 100 ns after the breakdown
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Vol
tage
(V)
Events with after-pulse measured on a single micropixel.
y = 0.0067x2 - 0.4218x + 6.639
y = 0.0068x2 - 0.4259x + 6.705
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Afte
rpul
se/p
ulse
Tint = 60nsTint = 100ns
After-pulse probability vs bias
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SiPMs: Geometric factor
Yu. Musienko, RICH-2016 8
20 x 20 pix
“Dead” space between SiPM cells reduces its PDE. It is especially important for the small cell pitch SiPMs
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X-talk reduction
Yu. Musienko, RICH-2016 9
(KETEK – Photodet-2015 (Troitsk))
(HPK: Koei Yamamoto, 2nd SiPMAdvanced Workshop, March 2014)
Metal filledtrench
< 1 µm
(FBK: G. Zappalà, VCI-2016)
25µm 30µm 35µm 40µm
The way to reduce X-talk: trench filled with non-transparent material (tungsten)
X-talk was reduced from 20÷30% to 3÷5% at dVB=4÷5 V
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Afterpulsing and delayed X-talk reduction
Yu. Musienko, RICH-2016 10
25µm 30µm 35µm 40µm
(G. Zappalà, VCI-2016)
(HPK: Koei Yamamoto, 2nd SiPMAdvanced Workshop, March 2014)
After-pulsing and delayed X-talk were reduced from 30% to <1.5% at high overvoltage
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SiPMs: PDE increase
Yu. Musienko, RICH-2016 11
Small X-talk and after-pulsing allow SiPM operation at high over-voltages. As a result maximum PDE increased from 20 ÷ 30% to 50 ÷ 60 % (SiPMs with 43÷50 µm cell pitch).
VBD: 25.5 V
(KETEK – Photodet-2015 (Troitsk))
(SensL MicroFJ-SMA-3035-E46, CERN APD Lab)
(T.Kirn, VCI-2016)
SiPM array for LHCb Scintillating Fibre Tracker
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PDE increase: SiPMs with very thin trenches
Yu. Musienko, RICH-2016 12
NUV-HD SiPM
Trench< 2 µm
High-field region
Poly stripresistor
Metal
High-field region
Cell 2Cell 1
~ 4.5 µm
NUV-SiPM
Cell 2 Cell 3Cell 1
NUV High-Density (HD) technology:
Lower dead border region → Higher Fill Factor
Trenches between cells → Lower Cross-Talk
(G. Zappalà(FBK), VCI-2016)
Cherenkov light spectrum in Earth’s atmosphere
NUV-HD 30µm Cell Pitch PDE, 10V OV
30 µm cell pitch SiPMs: GF=77% PDE>50 % !!
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Dark noise reduction
Yu. Musienko, RICH-2016 13
25µm 30µm 35µm 40µm(G. Zappalà(FBK), VCI-2016)
(HPK: Koei Yamamoto, 2nd SiPMAdvanced Workshop, March 2014)
J.Merphy(SensL) 2nd SiPMAdvanced Workshop, March 2014)
Dark Count ~30 kHz/mm2 wasmeasured at dVB=2÷3 V atroom temperature with SiPMsfrom several producers. Now itbecomes a standard!!
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Dark noise at low temperature
Yu. Musienko, RICH-2016 14
Standard field
Low-field
> 7 orders of magnitude !
A 10x10 cm2 SiPM array would have a total DCR < 100 Hz!
A low-electric field NUV-HD version has been developed by FBK to reduce the tunnelling component of the DCR.
(G. Zappalà(FBK), VCI-2016)
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Further GF increase: Metal Film Quenching Resistor
Yu. Musienko, RICH-2016 15
(HPK: Koei Yamamoto, 2nd SiPMAdvanced Workshop, March 2014)
Quenching resistors occupy some of the cell’s sensitive area. They are non-transparent for UV/blue/green light. The loss of sensitivity can be significant (especially for small cells).
Another advantages of MFQ resistors are better uniformity and relatively small temperature coefficient smaller cell recovery time
change with temperature
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SiPMs with Metal Quenching Resistor: PDE increase
Yu. Musienko, RICH-2016 16
Polysilicon resistors MQ resistors
MPPCs developed by HPK for the CMS HCAL Upgrade project
PDE(515 nm)>30% for 15 µm cell pitch MQR MPPCs. It was improved by a factor of >3 in comparison to the 15 µm cell pitch MPPCs with polysilicon quenching resistors.
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The future of SiPMs: UHD SiPMs
Yu. Musienko, RICH-2016 17
During last 3 years very high geometric factors (up to 80%) were achieved with smallcell pitch SiPMs or (Ultra High Density SiPMs). Small cells have many advantages: lowgain smaller X-talk, after-pulsing, recovery time; larger dynamic range, possibility tooperate SiPMs at high over-voltages, better resistance to radiation: smaller darkcurrents of irradiated SiPMs, smaller power dissipation, reduced blocking effects. Smallcells potentially should provide better timing resolution (smaller avalanchedevelopment time)
Previous development: linear array of MAPDs (18x1 mm2 , 15 000 cells/mm2 ) produced by Zecotek for the CMS HCAL Upgrade project.
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Large dynamic range SiPMs for the CMS HE HCAL Upgrade
Yu. Musienko, RICH-2016 18
PDE(
515
nm) [
%]
SiPM, T=23.2 C 45 40 HPK-array-10003-ch5 35 30 25 20 15 10
5 0
0 1 2 3 4 5 6 7 V-VB [V]
8-ch. SiPM array for the CMS HE HCAL Upgrade project: Ø2.8 mm SiPMs, 15 µm cell pitch
05
1015202530354045
350 400 450 500 550 600 650 700 750 800
PDE
[%]
Wavelength [nm]
dVB=4.0 V
Glass widow with special filter was designed by HPK to cut off UV light which can be produced by muons and hadrons in plastic fibers
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Ampl
itude
[V]
Time [s]
Yu. Musienko, PD-15
SiPM laser response
Recovery time 7-8 ns
1400 SiPM arrays have beendelivered to CERN during this year
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FBK UHD2 SiPMs
Yu. Musienko, RICH-2016 19
RGB-UHDL < 1um
RGB-HD
RGB
(Alberto Gola – PhotoDet 2015, Troitsk)
L (um) Fill Factor
0.75 57.1%
1 48.8%
1.25 40.3%
1.5 32.6%
Fill Factor vs. trench widthCell sensitive area vs. trench width
Finished 10 µm cell pitch SiPM
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UHD2 SiPM parameters
Yu. Musienko, RICH-2016 20
3.4 ns
Laser response Recovery time
(Alberto Gola – PhotoDet-2015 , Troitsk)
12.5 um cellOV = 5.7 V
7.5 um cellOV = 4.6 V
L = 0.75 umT = 24 °C
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SiPM timing
Yu. Musienko, RICH-2016 21
Single-photon time resolution for 3 SiPM area, measured at different biases for 425 nm light. Larger area SiPMs have slower signal rise-time. Factors limiting SPTR are signal rise-time, signal electron resolution and correlated noise (X-talk and delayed pulses). The latest is especially important for multi-photon events. The result which is shown here is among the best measured so far.
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Vacuum ultra violet (VUV) SiPMs
Yu. Musienko, RICH-2016 22
SiPMs sensitive to VUV light (<150 nm) were recently developed by HPK for detection LAr (T=-186 °C) scintillation light (λ = 128 nm).
(NIM A833 (2016) 239–244)
The PDE(128 nm) wasmeasured ~8% for 50υm pitch SiPMs and~13% for 100 µm pitchSiPM at dVB=3 V
Am-241, E=5.5 MeV
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SiPM: radiation hardness
Yu. Musienko, RICH-2016 23
Radiation may cause:
• Fatal SiPMs damage (SiPMs can’t be used after certain absorbed dose)• Dark current and dark count increase (silicon …)• Change of the gain and PDE vs. voltage dependence (SiPMs blocking effects due to high induced dark carriers generation-recombination rate)• Breakdown voltage change
SiPMs with high cell density and fast recovery time can operate up to 3*1012 neutrons/cm2 (gain change is< 25%).
Relative response to LED pulse vs. exposure to neutrons (Eeq~1 MeV) for different SiPMs
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Dark current vs. exposure to neutrons (Eeq~1 MeV) for different SiPMs
Yu. Musienko, RICH-2016 24
High energy neutrons/protons produce silicon defects which cause an increase in dark count and leakage current in SiPMs:
Id~α*Φ*V*M*k,
α – dark current damage constant [A/cm];Φ – particle flux [1/cm2];V – silicon active volume [cm3]M – SiPM gaink – NIEL coefficient
αSi ~4*10-17 A*cm after 80 min annealing at T=60 C (measured at T=20 C)
V~S*Gf*deff, S - areaGf - geometric factordeff - effective thickness
Thickness of the epi-layer for most of SiPMs is in the range of 1-3 µm, however deff ~ 5 ÷ 50 µm for different SiPMs. High electric field effects (such as tunneling and field enhanced generation) play significant role in the origin of SiPM’s dark noise.
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Dependence of the SiPM dark current on the temperature (after irradiation)
Yu. Musienko, RICH-2016 25
It was observed a rather weak dependence of theSiPM’s dark current decrease with temperature onthe dVB value. SiPM dark currents at low voltage(5V) behave similar with temperature to that of thePIN diode. However we observed significantdifference of this dependence for differenet SiPMtypes when they operate over breakdown! Generaltrend is that SiPMs with high VB value have fasterdark current reduction with the temperature.
(Yu.Musienko, NDIP-2014)
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SiPM irradiated up to 2.2*1014 n /cm2
Yu. Musienko, RICH-2016 26
Can SiPM survive very high neutron fluences expected at high luminosity LHC? FBK SiPM (1 mm2, 12 µm cell pitch was irradiated with 62 MeV protons up to 2.2*1014 n /cm2 (1 MeV equivalent).
(A.Heering et al., NIM A824 (2016) 111)
We found:- Increase of VB: ~0.5 V- Drop of the amplitude (~2 times)- Reduction of PDE (from 10% to 7.5 %)- Increase of the current (up to ~1mA at
dVB=1.5 V- ENC(50 ns gate, dVB=1.5V)~80 e, rmsThe main result is that SiPM survived this dose of irradiation and can be used as photon detector!
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Radiation hardness study of the Philips Digital Photon Counter with proton beam
Yu. Musienko, RICH-2016 27(M.Barnyakov et al., Elba-2015)
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SiC SSPM
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(S.Dolinsky, GE, NDIP-2014)
Dark current vs. temperature
Potentially can be more radiation hard than silicon
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GaAs SSPM
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Wide bandgap (1.42 eV): potentially can be moreradiation hard than silicon. Timing with GaAs SSPM canbe also better (high mobility of electrons and holes, fastavalanche development – direct semiconductor)
LightSpin Photomultiplier Chip™
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Position-Sensitive SiPMs: PS-SiPM RMD
Yu. Musienko, RICH-2016 30
RMD had designed a 5x5 mm2 position-sensitive solid-state photomultiplier (PS-SSPM) using a CMOS process that provides imaging capability on the micro-pixel level. The PS-SSPM has 11,664 micro-pixels total, with each having a micro-pixel pitch of 44.3 micron.
A basic schematics showing the design layout and pattern for PS-SSPM resistive network. Each square represents a micro-pixel. The network resistors are 246.5 Ohm each.
Anger logic:
A plot of the X–Y spatial resolution (FWHM) as a function of the incident beam spot light intensity. Spot size was ~30 micron.
An image of a 66 LYSO array having 0.5 mm pixels uniformly irradiated with 22Na.
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PS SiPM - NDL
Yu. Musienko, RICH-2016 31
Schematic cross-section of the PS-SiPMwith bulk quenching resistor
Top view of tetra-lateral type electrodes of the PS-SiPM with 4 anodes
The device takes advantages of the sheet N+ layer as the intrinsic continuous cap resistor for charge division, the same way adopted in PIN or APD PSD
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PS-SiPM – NDL (II)
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Reconstruction of nine positions of light spots from optical fiber tested in the central part of the device
The device, with an active area of 2.2 mm × 2.2 mm, demonstrated spatial resolution of 78–97 μm, gain of 1.4 × 105
and 46-ps time jitter of transmission delay for 210–230 photons.
IEEE TRANSACTIONS ON ELECTRON DEVICES, VOL. 61, NO. 9, SEPTEMBER 2014
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SiPMs with Bandpass Dichroic Filters
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(M.Mazillo et al., to be published in Sensors)
PDE measured at 515 nm vs bias on n-on-p SiPM with and without BP filter
Optical microscopepicture of the STMicroSiPM (548 cells, 67.4%geometrical factor)
PDE spectral shape measured at 24 °C and dVB=3 V on n-on-p SiPM with and without BP filter
Green bandpath filterwith 5x5 mm area and1.1 mm thickness
Such a photo-sensor can be very used inapplications where protection of the detector fromunwanted light background (ambient light forexample) is required.
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TSV technology (no bonding wire)
Yu. Musienko, RICH-2016 34
TSV Technology:Further improved geometrical efficiency for arrays ,
(KETEK – Photodet-2015 (Troitsk))
(HPK: Koei Yamamoto, 2nd SiPMAdvanced Workshop, March 2014)
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Summary
Yu. Musienko, RICH-2016 35
Significant progress in development of SSPMs over last 3 years by several developers:
• High PDE: ~50-60% for blue-green light
• SiPMs with good sensitivity (PDE>10%) for VUV light have been developed
• Dark count at room temperature was reduced: ~30 kHz/mm2
• Low optical cross-talk: <1-5% for high OV
• Fast timing: SPTR~75 ps (FWHM)
• Large dynamic range: >10 000 pixels/mm2 (with high PDE>30%)
• Very fast cell recovery time: ~4 ns
• Large area: 6x6 mm2 and more
• TSV technology was introduced to build very compact SiPM arrays
• Position-sensitive SiPMs with good position resolution: <100 µm
• SiPMs demonstrated their rad. tolerance up to 2.2*1014 n/cm2
• SiC, GaAs, InGaP SSPMs were successfully developed
• . . .
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SSPM perspectives (3-5 years)
Yu. Musienko, RICH-2016 36
My point of view:
• Further work to reduce correlated noise (this is one of the limiting factors for many applications)
• Small cell pitch (5 µm), large dynamic range SIPMs
• DUV SiPMs with good sensitivity (PDE>30%) for VUV light
• Dark count at room temperature can be reduced: <10 kHz/mm2
• Development of SiPMs for fast timing: SPTR<50 ps (FWHM)
• Fast cell recovery time: 2-3 ns
• Large area: 10x10 mm2 and more
• PS SiPMs with position resolution: <50 µm for single photons
• SiPMs with rad. tolerance up to 5*1014 n/cm2
• Further development of SiC, GaAs, InGaP SSPMs.
• Price will go down (for large quantities) <10 CHF/cm2....
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Acknowledgments
Yu. Musienko, RICH-2016 37
Work supported by RF Ministry of education and science in frame of the Agreement on 17 October 2014 No 14.610.21.0004 ID No RFMEFI61014X0004.