october 2002sienna, jl. faure, dapnia/spp in 8th topical seminar on innovative particle and...
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October 2002Sienna, JL. Faure, DAPNIA/SPP Requirements I Photon counting capability In scintillation detection In Cerenkov light detection Pixelisation & Single photon Scintillating fiber Cerenkov counter RICH Low photon Yield (single photon) Gain Speed Large Surface Coverage Harsh Environement Magnetic field Radiation field High Energy Physics Medicine Astro PhysicsTRANSCRIPT
October 2002 Sienna, JL. Faure, DAPNIA/SPP
InIn
8th Topical Seminar on Innovative Particle and 8th Topical Seminar on Innovative Particle and Radiation DetectorsRadiation Detectors
Jean-louis Faure CEA-DAPNIA-SPPJean-louis Faure CEA-DAPNIA-SPP
Progress with Photo-detectors
October 2002 Sienna, JL. Faure, DAPNIA/SPP
Photo-detectorsPhoto-detectors
Vacuum DevicesSolid States DetectorsGaseous Detectors
High Energy PhysicsAstro-PhysicsMedecine
Restriction to Visible Light
October 2002 Sienna, JL. Faure, DAPNIA/SPP
Requirements IRequirements IPhoton counting capability
In scintillation detection In Cerenkov light detection
Pixelisation & Single photonScintillating fiberCerenkov counter RICH
Low photon Yield (single photon)Gain
SpeedLarge Surface CoverageHarsh Environement
Magnetic fieldRadiation field
High Energy Physics
Medicine
Astro Physics
October 2002 Sienna, JL. Faure, DAPNIA/SPP
Requirements II Requirements II Resolution reminderResolution reminder
Nphoto−electron=QuantumEff⋅Ccollected⋅ Nγ_ signal.or.background
σsignal/background= ENF ⋅ Nphoto−electron
ENF =1+ 1δ1
+ 1δ1δ2
+⋅⋅⋅+ 1δ1δ2 ⋅⋅⋅δn
σENC =ENCGain
σE
= σNphoto−electron
= σsignal2 +σBackground
2 +σ ENC2
Npe
October 2002 Sienna, JL. Faure, DAPNIA/SPP
Requirements III Requirements III Resolution reminderResolution reminder
σE
≈ ENFQE⋅Ccol ⋅Nγ
σE
=ENF⋅QuantumEff⋅Ccol ⋅(Nγ _ signal+Nγ _ background)+(ENC/ Gain)2
QuantumEff⋅Ccol ⋅Nγ
G >>ENC or ENC small !!Nbackground << Nsignal
QE as high as possibleENF as close as 1.Ccol as close as 100%
N as large as possible !!!
October 2002 Sienna, JL. Faure, DAPNIA/SPP
Requirements IV Requirements IV Resolution summaryResolution summary
No.of Photons
Ener
gy R
eso l
u ti o
n
0.001
Poisson (statistic) LimitENF=1QE=1Ccol=1
Photo Diode
Avalanche Photo-diode
Hybrid Photo-DiodePMT
0.01
0.1
1
10
10 1 10 2 10 710 3 10 4 10 610 0
October 2002 Sienna, JL. Faure, DAPNIA/SPP
Vacuum DevicesVacuum DevicesVacuum Devices are the ground of Photodetection
since more than 40 years
There are still important progress made and to be made ?
Last years a lot of efforts on “Compactness” Flat PMT“Pixelization” Multi-anode PMT“Hybridation” Hybrid Photo-diode
October 2002 Sienna, JL. Faure, DAPNIA/SPP
FLAT PMT HamamatsuFLAT PMT Hamamatsu
64 Pixels
Metal Channel dynode
RICH2002 J. Va’vra (SLAC)
October 2002 Sienna, JL. Faure, DAPNIA/SPP
Delft Electronic Products B.V. HPDs
LHCb
19 x 5.5mm
73 x 2.75mm
CMS HCAL
Photon Countingpossibility
October 2002 Sienna, JL. Faure, DAPNIA/SPP
MultiAnode PMTMultiAnode PMT
Hamamatsu R7600-M16/M64
EUSO Focal Plane 2.5 m diameter250.000 pixels
Hamamatsu R5900 seriesM64 (64 anodes – metal dynode chains)
Enhancing the actual active surfaceFrom 38 % to 85 %
From RICH2002 Workshop: Franz Muheim (U.of Edinburgh)
October 2002 Sienna, JL. Faure, DAPNIA/SPP
””Large” PMT ExamplesLarge” PMT Examples
1 km
10 TeV Muon Event
Photomultiplier
ICECUBE(Amanda II)60 PMTs/string80 strings4800PMTs
AUGER1600 water tanks 3 PMTs≈ 4800 PMT of 9”
Photonis XP1805/D1
October 2002 Sienna, JL. Faure, DAPNIA/SPP
Quantum Quantum EfficiencyEfficiency
October 2002 Sienna, JL. Faure, DAPNIA/SPP
MCP R&DMCP R&D
Photoelectron
photonFaceplate
Photocathode !V ~ 300V
Dual MCP !V ~ 3000V
6 !V ~ 300V
Anode
Gain ~ 106
BurlePlanacom™
Micro Channel PlateMCP-PMTs
SiliconMicro Channel Plate
Silicon MCP are made by photolithography5 m pores Potential large surfaceStrip readout (X and Y) pixel nb reduction
From O.Siegmund SSL UCB
October 2002 Sienna, JL. Faure, DAPNIA/SPP
APDsAPDs
Si3N4, SiO2, contactp++photon conversionp e- accelerationn e- multiplication
n-e- drift
n++e- collection
contact
Not to scale
APD are grown by epitaxy on n++ wafer
5 mm
Active area 5x5 mm2
Operating voltage (Vr) ~380 VCapacitance 70 pFSerial resistance 3 ΩDark Current <10 nAQuantu efficien cy ∼72% @ 420 n
CMS ECALDouble APD
October 2002 Sienna, JL. Faure, DAPNIA/SPP
APDs con’t APDs con’t
1
3
5
7
9
11
13
15
0 500 1000 1500 2000
Gain
Excess Noise Factor
0
10
20
30
40
50
60
70
80
90
100
300 400 500 600 700 800 900 1000Wavelength [nm]
Quantum Efficiency [%]
dMdV
× 1M
=3%/V dMdT
× 1M
=−2%/0C
ENF =k ×G+ 2−1G( )×(1−k)k is the hole / elec velocity ratioG the gain
ENF≥2
October 2002 Sienna, JL. Faure, DAPNIA/SPP
APDs R&DAPDs R&DHow to overcome the ENF versus Gain issue
=How to operate at high gain without increasing ENF
Run at low temperature
Reverse APDs
LAAPD Large Array APD
Build a HAPDHPMT using an APD instead of an PIN diode
October 2002 Sienna, JL. Faure, DAPNIA/SPP
Silicon PMSilicon PMby P. Buzhan, B. Dolgoshein et. al.
G= 2x106
ENF≈1QE≈10%Sensitive area 1.5x1.5 mm
October 2002 Sienna, JL. Faure, DAPNIA/SPP
Gaseous Photo DetectorGaseous Photo Detector
• fast signals [1-10 ns] • high gain [>105] • sensitivity to single photoelectrons• operation in noble gases (mixtures) • high 2D precision
Multi-GEM GMPTs
From Breskin et al.CsI Quantum Efficiency
CsI photo-cathode mature technologyIs well adpated to RICH
How to work in visible light ?A possible solution for very large surface detector
October 2002 Sienna, JL. Faure, DAPNIA/SPP
SummarySummaryHuge progress in small pixel photodetectors
Hybid devices [HPD, MaPMT,….] Solid states arrays [PiN, APD,….]
R&DHybrid improvement (HAPD)Promising use of nano-technology Silicon MCP
Very Large surface (volume) coverageVacuum devices today only solution ?R&D needs
Dream no vacuumLarge area photo-cathode
High Energy Physics&
Medicine
Astro Particule&
Astrophysics