A. Lyashenko Alkali-antimonide PCs for GPMPC workshop, Chicago 09 Alkali-antimonide Photocathodes for Gas- Avalanche Photomultipliers Recent review on.

Slides:



Advertisements
Similar presentations
Bialkali Photocathode Development
Advertisements

General Characteristics of Gas Detectors
First observation of electroluminescence in liquid xenon within THGEM holes: towards novel Liquid Hole-Multipliers L. Arazi, A. Breskin, A. Coimbra*,
LECTURE- 5 CONTENTS  PHOTOCONDUCTING MATERIALS  CONSTRUCTION OF PHOTOCONDUCTING MATERIALS  APPLICATIONS OF PHOTOCONDUCTING MATERIALS.
Hiroyuki Sekiya Oct. 4 th 2007 Hamamatsu, JAPAN NNN07 Development of Gaseous Photomultiplier with GEM/μPIC Hiroyuki Sekiya ICRR, University of Tokyo
1 Two-phase and gaseous cryogenic avalanche detectors based on GEMs A. Bondar, A. Buzulutskov, A. Grebenuk, D. Pavlyuchenko, R. Snopkov, Y. Tikhonov Budker.
Hiroyuki Sekiya Jul. 31 st 2008, Philadelphia, ICHEP2008 Development of Gaseous Photomultiplier with GEM/μPIC Hiroyuki Sekiya ICRR, University of Tokyo.
Gas Detector Developments Jin Li. Liquid Xenon case Liquid Xenon can be considered as a gaseous xenon of 520 atm. K.Masuda, S. Takasu, T.Doke et al. (Doke.
1 LAPD Team Meeting 10/14/09 O.H.W. Siegmund, Experimental Astrophysics Group, Space Sciences Laboratory, U. California at Berkeley Bialkali Photocathode.
K 2 CsSb Cathode Development John Smedley Triveni Rao Andrew Burrill BNL ERL needs – 50 mA, 7 mm dia., 1.3 mA/mm 2.
A. BreskinTIPP09 Tsukuba VISIBLE-SENSITIVE GAS-PMs A. Breskin, A. Lyashenko, R. Chechik Weizmann Institute of Science, Rehovot, Israel J.M.F. dos Santos,
The problem: The latest theoretical and experimental results suggest investigating a physics domain for p t higher than the actual one covered by the HMPID.
GaAs and CsKSb Photocathodes for DC Gun
1 st Workshop on Photo-cathodes: nm Klaus Attenkofer, Karen Byrum, Henry Frisch, Oswald Siegmund July 20-21, 2009: University of Chicago.
Transducers Converts one type of energy into another. Light  Electrical (current, voltage, etc.) What characteristics should we look for in a transducer?
Photomultiplier Tube. What is it? Extremely sensitive detector of light in the ultraviolet, visible and near infrared Multiplies the signal produced by.
10 Picosecond Timing Workshop 28 April PLANACON MCP-PMT for use in Ultra-High Speed Applications.
1 Light Collection  Once light is produced in a scintillator it must collected, transported, and coupled to some device that can convert it into an electrical.
Catania VLVnT09 Athens, Greece 1/14 Catania Performances of four super bialkali large area photomultipliers with respect to.
Detector R & D plan Detector Development plan Detector Simulations Conclusion SINP/VECC Meeting High Energy Physics Group, BHU.
C.Shalem et al, IEEE 2004, Rome, October 18 R. Chechik et al. ________________RICH2004_____________ Playa del Carmen, Mexico 1 Thick GEM-like multipliers:
A. Breskin RD51 Amsterdam 4/08 ION BLOCKING & visible-sensitive gas-PMs Efficient ion blocking in gaseous detectors and its application to visible-sensitive.
A. Lyashenko INSTR08 – BINP – Feb ION BLOCKING & visible-sensitive gas-PMs Efficient ion blocking in gaseous detectors and its application to visible-sensitive.
RICH04 Mexico A. Breskin Ion-induced effects in GEM & GEM/MHSP- gaseous photomultipliers for the UV & visible spectral range
Gaseous photomultipliers and liquid hole-multipliers for future noble-liquid detectors L. Arazi [1], A. E. C. Coimbra [1,2], E. Erdal [1], I. Israelashvili.
1 The GEM Readout Alternative for XENON Uwe Oberlack Rice University PMT Readout conversion to UV light and proportional multiplication conversion to charge.
D. Attié CEA Saclay/Irfu RD51 – ALICE Workshop June 18 th, 2014 ILC-TPC Micromegas: Ion Backflow Measurements.
GEM: A new concept for electron amplification in gas detectors Contents 1.Introduction 2.Two-step amplification: MWPC combined with GEM 3.Measurement of.
Sheffield : R. Hollingworth, D. Tovey R.A.L. : R.Luscher Development of Micromegas charge readout for two phase Xenon based Dark Matter detectors Contents:
CsI-TGEM vs. CsI-MWPC photodetector Some part of this work was performed in collaboration between CERN and Breskin group.
Ionization Detectors Basic operation
1 IBF in aligned, misaligned and FLOWER THGEMs The IBF problem Standard THGEM configuration COBRA and extra electrode Misaligned holes FLOWER THGEM solution.
15th RD51 Collaboration Meeting 18 – 20 March 2015 CERN On the way to sub-100ps timing with Micromegas T. Papaevangelou IRFU / CEA Saclay.
R & D at BHU B.K. Singh (On behalf of HEP Group).
1 LAPPD Team meeting 6/10/2010 Ossy Siegmund, Experimental Astrophysics Group, Space Sciences Laboratory, U. California at Berkeley Bialkali Photocathode.
LAPPD Collaboration Review 12/9/2011 Ossy Siegmund, Sharon Jelinsky, Jason McPhate, Joe Tedesco Experimental Astrophysics Group, Space Sciences Laboratory,
THGEM in Ne-mixtures UV-photon detection in RICH & more Weizmann: M. Cortesi, R. Chechik, R. Budnik, CERN: V. Peskov Coimbra & Aveiro: J. Veloso, C. Azevedo,
Techniques for Nuclear and Particle Physics Experiments By W.R. Leo Chapter Eight:
DETECTOR TECHNOLOGIES
6-Aug-02Itzhak Tserruya PHENIX Upgrade mini-Workshop1 Boris Khachaturov, Alexander Kozlov, Ilia Ravinovich and Itzhak Tserruya Weizmann Institute, Israel.
Catania 11 ICATPP october, 2009 Como 1/12 Catania Comparative measurements of the performances of four super bialkali large.
Itzhak Tserruya, BNL, May13, HBD R&D Update: Demonstration of Hadron Blindness A. Kozlov, I. Ravinovich, L. Shekhtman and I. Tserruya Weizmann Institute,
1 Original motivation for first mass-production of MPGDs: Low-background applications (in particular coherent neutrino-nucleus scattering) “Wallpaper”
Lecture 3-Building a Detector (cont’d) George K. Parks Space Sciences Laboratory UC Berkeley, Berkeley, CA.
TCPD test measurement 1 TCPD (TGEM CCC Photon Detector) test measurement ELTE, MTA KFKI RMKI, REGARD Group (Budapest, Hungary): Levente Kovács G. Hamar,
Prospects to Use Silicon Photomultipliers for the Astroparticle Physics Experiments EUSO and MAGIC A. Nepomuk Otte Max-Planck-Institut für Physik München.
Discharge Studies in MPGD: what could be done in the frame of WG-2 collaboration P. Fonte, V. Peskov.
1 Two-phase Ar avalanche detectors based on GEMs A. Bondar, A. Buzulutskov, A. Grebenuk, D. Pavlyuchenko, Y. Tikhonov Budker Institute of Nuclear Physics,
1 HBD R&D: Update Itzhak Tserruya (for A. Kozlov, I. Ravinovich and L. Shekhtman) Weizmann Institute, Rehovot DC meeting Feb. 14, 2003.
Construction and Characterization of a GEM G.Bencivenni, LNF-INFN The lesson is divided in two main parts: 1 - construction of a GEM detector (Marco Pistilli)
Collection of Photoelectrons from a CsI Photocathode in Triple GEM Detectors C. Woody B.Azmuon 1, A Caccavano 1, Z.Citron 2, M.Durham 2, T.Hemmick 2, J.Kamin.
Quality-evaluation of Cesium Iodide photocathodes for the ALICE/High Momentum Particle Identification detector by means of a VUV-Scanner system Herbert.
T. Zerguerras- RD51 WG Meeting- CERN - February Single-electron response and energy resolution of a Micromegas detector T. Zerguerras *, B.
1 A two-phase Ar avalanche detector with CsI photocathode: first results A. Bondar, A. Buzulutskov, A. Grebenuk, D. Pavlyuchenko, R. Snopkov, Y. Tikhonov.
Development of a Single Ion Detector for Radiation Track Structure Studies F. Vasi, M. Casiraghi, R. Schulte, V. Bashkirov.
THGEM Marco Cortesi Weizmann Institute of Science PANIC08 Recent Advances in THGEM Detectors M. Cortesi, A. Breskin, R. Chechik, R. Alon, J. Miyamoto Weizmann.
R&D on Hadron Blind detector, recent results Issues addressed: - gain limits in CF 4 with heavily ionizing particles - operation.
Mg Films Grown by Pulsed Laser Deposition as Photocathodes: QE and surface adsorbates L. Cultrera INFN – National Laboratories of Frascati.
Study of the cryogenic THGEM-GPM for the readout of scintillation light from liquid argon Xie Wenqing( 谢文庆 ), Fu Yidong( 付逸冬 ), Li Yulan( 李玉兰 ) Department.
Amos Breskin Weizmann Institute of Science
Part-V Micropattern gaseous detectors
MPGD 2015 Concise Summary Amos Breskin.
IBF in THGEM-based PHOTON DETECTORS, an update
WG1 Task2 New structures, new designs, new geometries
THGEM: Introduction to discussion on UV-detector parameters for RICH
Production of Cesium Iodide Photocathodes for
PAN-2013: Radiation detectors
E. Erdal(1), L. Arazi(2), A. Breskin(1), S. Shchemelinin(1), A
Presentation transcript:

A. Lyashenko Alkali-antimonide PCs for GPMPC workshop, Chicago 09 Alkali-antimonide Photocathodes for Gas- Avalanche Photomultipliers Recent review on GPMs: Chechik & Breskin NIM A595 (2008) 116 Summary article visible-light GPM: Lyashenko et al. JINST 4 (2009) P07005 A.Lyashenko, R. Chechik and A. Breskin Weizmann Institute of Science, Rehovot, Israel

A. Lyashenko Alkali-antimonide PCs for GPMPC workshop, Chicago 09 UV-exist: ALICE, HADES, COMPASS, J-LAB, PHENIX Visible-in course Motivation: large areas, flat geometry operation in magnetic fields sensitivity to single photons visible spectral range fast (ns range) high localization accuracy (sub-mm range) Gaseous Photo-Multipliers (GPM)

A. Lyashenko Alkali-antimonide PCs for GPMPC workshop, Chicago 09 Principles of GPM operation Photoelectron emission from photocathode Avalanche charge multiplication in gas Signal recording

A. Lyashenko Alkali-antimonide PCs for GPMPC workshop, Chicago 09 Alkali-antimonide pc production (QE nm in vacuum for semi-transparent PC) Hot Indium sealing to => critical for pc Multi-chamber UHV setup

A. Lyashenko Alkali-antimonide PCs for GPMPC workshop, Chicago 09 PC substrate treatment in air PC substrate treatment in vacuum (usually baking at C ) Evaporation of alkali-metals PC sensitivity Long term stability PC fabrication process:

A. Lyashenko Alkali-antimonide PCs for GPMPC workshop, Chicago 09 Photocathodes: Cs 3 Sb Activation steps: 1. Evaporation of Sb at C onto a substrate until it looses ~20% of its transparency 2. Exposure to Cs at C until the maximum of photocurrent is reached. 3. Post-treatment if needed (removing of excess of Cs by baking at ~200 0 C) Activation time: min PC characteristics (typical): Wavelength of max response: λ max = nm Luminous sensitivity: μA/lm Responsivity at λ max : 65-75mA/W QE at λ max : 20-25% Dark emission current at 25 0 C: ≤0.1fA/cm 2 Surface resistance at 25 0 C: 3*10 7 Ohm/square Designation: S-11 Large area: YES Burle

A. Lyashenko Alkali-antimonide PCs for GPMPC workshop, Chicago 09 Photocathodes: K 2 CsSb PC characteristics (typical): Wavelength of max response: λ max = nm Luminous sensitivity: μA/lm Responsivity at λ max : 100mA/W QE at λ max : >30% Dark emission current at 25 0 C: ≤0.01fA/cm 2 Surface resistance at 25 0 C: 6*10 9 Ohm/square Features: Very high surface resistance Activation steps: One possibility: 1. Evaporation of Sb at C onto a substrate until 20% of transparency is lost 2. Exposure to K at C until the maximum of photocurrent is reached (formation of K 3 Sb PC). 3. Repetitive (yo-yo) exposure to Cs & Sb at C until the maximum of photocurrent is reached. Another possibility: So called co evaporation Large area: YES, needs a conductive layer Burle

A. Lyashenko Alkali-antimonide PCs for GPMPC workshop, Chicago 09 Photocathodes: Na 2 KSb Activation steps: 1. Evaporation of Sb at C on substrate until it looses 20% of its transparency 2. Exposure to K at C until maximum photocurrent reached (K 3 Sb). 3. Exposure to Na at ~220 0 C until the raise of PC current start slowing down*. 4. Alternating addition of Sb and K at ~ C until maximum photocurrent reached. * Simultaneous evaporation of K and Na is possible PC characteristics (typical): Wavelength of max response: λ max = nm Luminous sensitivity: 65-80μA/lm Responsivity at λ max : 64mA/W QE at λ max : 19-21% Dark emission current at 25 0 C: ≤0.0001fA/cm 2 Surface resistance at 25 0 C: 2*10 6 Ohm/square Features: Outstanding temperature stability (up to C), lowest dark current Large area: YES, but production is rather complicated, QE< other Bi-alkali. Burle

A. Lyashenko Alkali-antimonide PCs for GPMPC workshop, Chicago 09 PC characterization

A. Lyashenko Alkali-antimonide PCs for GPMPC workshop, Chicago 09 QE of alkali-antimonide photocathodes QE~48% RECENT PHOTOCATHODES

A. Lyashenko Alkali-antimonide PCs for GPMPC workshop, Chicago 09 Photoelectron extraction from bi-alkali PC into gas Optimal field for GPM Higher transmission in other gases, e.g. CH4

A. Lyashenko Alkali-antimonide PCs for GPMPC workshop, Chicago 09 PC is stable in gas in the large vacuum chamber Expected even better stability for sealed devices Long-term photocathode stability in gas

A. Lyashenko Alkali-antimonide PCs for GPMPC workshop, Chicago 09 Secondary effects in visible-sensitive GPMs Gaseous Photo-Multiplier (GPM) Main problem: Ions & photons   secondary e emission  ion/photon feedback pulses  gain & performance limitations Photon feedback is largely reduced PC masked by electrode *GEM: Gas Electron Multiplier - Sauli, NIM A 386, (1997) 531. GEM* 70μm 50μm

A. Lyashenko Alkali-antimonide PCs for GPMPC workshop, Chicago 09 IBF: Ion Back-Flow Fraction  Major efforts to limit ion backflow 1. GATING  operation in “gated-mode”  deadtime, trigger NEW e - - MULTIPLIERS  operation in continuous mode (cascaded-GEM, MICROMEGAS…&: OTHERS)  Challenge: BLOCK IONS WITHOUT AFFECTING ELECTRON COLLECTION IBF: The average fraction of avalanche-generated ions back-flowing to the photocathode

A. Lyashenko Alkali-antimonide PCs for GPMPC workshop, Chicago 09 Visible-sensitive GPM: Ion-feedback development Visible-sensitive gas photomultiplier review: M. Balcerzyk et al., IEEE Trans. Nucl. Sci. Vol. 50 no. 4 (2003) 847  stable operation of visible sensitive GPMif CsI K-Cs-Sb K-Cs-Sb, Na-K-Sb, Cs-Sb : Current deviates from exponential Max Gain ~ few 100, IBF~10% G~10 5, γ + eff - ?, IBF - ?

A. Lyashenko Alkali-antimonide PCs for GPMPC workshop, Chicago 09 Calculation of ion induced secondary emission probability from bi-alkali PCs γ + eff = γ + ·ε extr Auger neutralization + Backscattering PCK-Cs-SbNa-K-Sb γ + eff PC GAS A.Lyashenko et al., J. Appl. Phys. (2009) accepted, arXiv: Most gases

A. Lyashenko Alkali-antimonide PCs for GPMPC workshop, Chicago 09 Measurements of γ + eff = γ + ·ε extr PCK-Cs-SbNa-K-Sb γ + eff (experiment)0.03± ±0.006 CsI K-Cs-Sb

A. Lyashenko Alkali-antimonide PCs for GPMPC workshop, Chicago 09 Effective IISEE from K-Cs-Sb and Na-K-Sb PCs PCK-Cs-SbNa-K-Sb IonCH 4 + γ + eff (exp) 0.03± ±0.006 γ + eff (theory) ~0.03 PC Ar/CH 4 (95/5), γ eff + ~0.03, Gain ~ 10 5 => IBF < 3.3*10 -4  stable operation of visible sensitive GPMif

A. Lyashenko Alkali-antimonide PCs for GPMPC workshop, Chicago 09 The Microhole & Strip plate (MHSP) Two multiplication stages on a single, double-sided, foil R&D: Weizmann/Coimbra Veloso et al. Rev. Sci. Inst. A 71 (2000) times lower IBF than with cascaded GEMs Strips: multiply charges

A. Lyashenko Alkali-antimonide PCs for GPMPC workshop, Chicago 09 Reverse-biased MHSP (R-MHSP) concept Flipped-R-MHSP R-MHSP Can trap its own ions Ions are trapped by negatively biased cathode strips Lyashenko et al., JINST (2006) 1 P10004 Lyashenko et al., JINST (2007) 2 P08004 Roth, NIM A535 (2004) 330 Breskin et al. NIM A553 (2005) 46 Veloso et al. NIM A548 (2005) 375 Can trap only ions from successive stages Strips: collect ions

A. Lyashenko Alkali-antimonide PCs for GPMPC workshop, Chicago 09 Lyashenko et al., JINST (2007) 2 P08004 IBF measured with 100% e-collection efficiency IBF=3*10 Gain=10 5 is 100 times lower than with 3GEMs 1st R-MHSP or F-R-MHSP: ion defocusing (no gain!) Mid GEMs: gain Last MHSP: extra gain & ion blocking BEST ION BLOCKING: “COMPOSITE” CASCADED MULTIPLIERS: IBF=3*10 -4

A. Lyashenko Alkali-antimonide PCs for GPMPC workshop, Chicago 09 20% QE 2 μC/mm 2 ion charge on photocathode: only ~ 4 x faster drop compared to thin ST CsI (~8 μ C/mm 2 ) K-Sb-Cs PC ageing in avalanche mode Real conditions: gain=10 5 ; IBF=3* % QE drop 46 5kHz/mm 2 ph. same conditions with a MWPC (IBF~0.5)  3000 times shorter lifetime: ~5 days! A. Breskin al. NIM A553 (2005) 46

A. Lyashenko Alkali-antimonide PCs for GPMPC workshop, Chicago 09 Sealed detector Test detector setup Visible-sensitive GPM UHV compatible materials Bi-alkali photocathode cascaded multiplier GEM/MHSP M. Balcerzyk et al., IEEE Trans. Nucl. Sci. Vol. 50 no. 4 (2003) 847

A. Lyashenko Alkali-antimonide PCs for GPMPC workshop, Chicago 09 Continuous operation of F-R-MHSP/GEM/MHSP with K-Cs-Sb photocathode with K-Cs-Sb photocathode Gain ~10 5 at full photoelectron collection efficiency First evidence of continuous high gain operation of visible-sensitive GPM K-Cs-Sb CsI Lyashenko et al., JINST (2009) 4 P07005

A. Lyashenko Alkali-antimonide PCs for GPMPC workshop, Chicago 09 Short-term GPM stability Rate: 12kHz/mm 2 photons Gain: 10 5 Total anode charge ~125μC

A. Lyashenko Alkali-antimonide PCs for GPMPC workshop, Chicago 09 Visible-sensitive GPM features Single photon sensitivity No ion-feedback Fast ns pulses 19 ns 100 photoelectrons

A. Lyashenko Alkali-antimonide PCs for GPMPC workshop, Chicago 09 Summary Alkali-antimonide PCs for GPMs High (>40%) QE values reached Stability in gas verified Probability of IISEE evaluated  Required IBF estimated MHSP/GEM-based CASCADED MULTIPLIERS 100 times lower IBF than with cascaded GEMs with full efficiency for collecting primary electrons! Gain ~10 5 reached with visible-sensitive K-Cs-Sb PC Demonstrated stable GPM operation at a gain 10 5 Atmospheric pressure operation  Many potential applications in large-area photon detectors: Particle Physics, Medical Imaging, Astroparticle, Military, Bio First evidence of high-gain continuous operation of visible-sensitive GPM