A new design of large area MCP-PMT for the next generation neutrino experiments

Similar documents
arxiv: v1 [physics.ins-det] 27 Jun 2017

Direct WIMP Detection in Double-Phase Xenon TPCs

A method to measure transit time spread of photomultiplier tubes with Cherenkov light

Chapter 4 Scintillation Detectors

A Large Liquid Scintillator Detector for Neutrino Mass Hierarchy : RENO-50

ARTICLE IN PRESS. Nuclear Instruments and Methods in Physics Research A

PoS(PhotoDet 2012)010

The Factors That Limit Time Resolution for Photon Detection in Large Cherenkov Detectors

High quantum efficiency S-20 photocathodes for photon counting applications

arxiv:physics/ v1 3 Aug 2006

The Daya Bay Reactor Neutrino Oscillation Experiment

PoS(PD07)031. General performance of the IceCube detector and the calibration results

arxiv: v1 [physics.ins-det] 27 Feb 2014

Shoei NAKAYAMA Kamioka Observatory, Institute for Cosmic Ray Research, The University of Tokyo

PHOTODETECTORS AND SILICON PHOTO MULTIPLIER

hν' Φ e - Gamma spectroscopy - Prelab questions 1. What characteristics distinguish x-rays from gamma rays? Is either more intrinsically dangerous?

Outline. (1) Physics motivations. (2) Project status

The JUNO veto detector system. Haoqi Lu Institute of High Energy physics (On Behalf of the JUNO Collaboration) TIPP2017, May22-26,Beijing

1. Neutrino Oscillations

Radioactivity and Ionizing Radiation

Neutrino Oscillation: Non-Accelerator Experiments

First Beam Profile Measurements Based on Light Radiation of Atoms Excited by the Particle Beam

Cherenkov Detector. Cosmic Rays Cherenkov Detector. Lodovico Lappetito. CherenkovDetector_ENG - 28/04/2016 Pag. 1

Hands on Project: Large Photocathode PMT Characterization

Time-of-Flight PET using Cherenkov Photons Produced in PbF 2

Nuclear Physics Laboratory. Gamma spectroscopy with scintillation detectors. M. Makek Faculty of Science Department of Physics

Proton decay and neutrino astrophysics with the future LENA detector

Scintillator Detectors for Neutrino Physics

KamLAND. Studying Neutrinos from Reactor

Andrey Formozov The University of Milan INFN Milan

Scintillation Detectors

Scintillation Detectors

Neutrino Experiments: Lecture 2 M. Shaevitz Columbia University

Prospects of Reactor ν Oscillation Experiments

DETERMINING FUNDAMENTAL PARAMETERS OF A SINGLE-PHOTOTUBE LIQUID SCINTILLATION COUNTER

Equalisation of the PMT response to charge particles for the Lucid detector of the ATLAS experiment

Next Generation Scintillation Detectors: Development of Quantum Dot Doped Scintillator. Lindley Winslow University of California Los Angeles

Scintillation Detectors

Chung-Yao Chao Fellowship Interview. Marco Grassi

Radionuclide Imaging MII Detection of Nuclear Emission

Energetic particles and their detection in situ (particle detectors) Part II. George Gloeckler

Measurements of Liquid Scintillator Light Yield for Future Neutrino Experiments

PoS(PD07)020. Timing Properties of MCP-PMT. Kenji Inami. Nagoya university, Nagoya, Japan

Synthesis of plastic scintillator. Ildefonso León Monzón Universidad Autónoma de Sinaloa

Guest Lecture PHY 7361: Harnessing Cherenkov Radiation SteveSekula, 13 April 2010 (created 9 April 2010)

PARTICLES REVELATION THROUGH SCINTILLATION COUNTER

THE JUNO EXPERIMENT. A.Meregaglia - IN2P3/CNRS - IPHC Strasbourg on behalf of the JUNO collaboration. 4 th November Paris NNN 2014

PoS(TIPP2014)033. Upgrade of MEG Liquid Xenon Calorimeter. Ryu SAWADA. ICEPP, the University of Tokyo

Current Results from Reactor Neutrino Experiments

QUASAR-370 Hybrid Phototube as a prototype of a photodetector for the next generation of deep underwater neutrino telescopes

Daya Bay and joint reactor neutrino analysis

arxiv: v1 [physics.ins-det] 3 Feb 2011

Factors Affecting Detector Performance Goals and Alternative Photo-detectors

Lecture 16 Light transmission and optical detectors

Daya Bay Neutrino Experiment

XENON Dark Matter Search. Juliette Alimena Columbia University REU August 2 nd 2007

Introduction to Radiation Monitoring

LENA. Investigation of Optical Scintillation Properties and the Detection of Supernovae Relic Neutrinos. M. Wurm. January 18, 2006 LENA. M.

Studies of Hadron Calorimeter

Neutrinos and the Universe

XMASS 1.5, the next step of the XMASS experiment

The Daya Bay Reactor Neutrino Experiment

Lecture 9. PMTs and Laser Noise. Lecture 9. Photon Counting. Photomultiplier Tubes (PMTs) Laser Phase Noise. Relative Intensity

SIDIS Gas CherenkovS. S. Malace, H. Gao et al.

Quantum Efficiency Measurements of Dark Matter PMT

Seminar. Large Area Single Photon Detectors

The Hyper-Kamiodande Project A New Adventure in n Physics

Neutrino Experiments with Reactors

Xenon Compton Telescopes at Columbia: the post LXeGRIT phase. E.Aprile. Columbia University

CMS Note Mailing address: CMS CERN, CH-1211 GENEVA 23, Switzerland

Neutrino Physics. Neutron Detector in the Aberdeen Tunnel Underground Laboratory. The Daya Bay Experiment. Significance of θ 13

Recent Results from RENO & Future Project RENO-50

The Double Chooz reactor neutrino experiment

Dark Matter Detection and PMT Base Optimization

Scintillators General Characteristics

Neutrino oscillation physics potential of Hyper-Kamiokande

Study of absorption and re-emission processes in a ternary liquid scintillation system *

PANDA-?? A New Detector for Dark Matter Search

Neutrino Experiment. Wei Wang NEPPSR09, Aug 14, 2009


PHYS 3446 Lecture #12

An Underground Laboratory for a Multi-Detector Experiment. Karsten Heeger Lawrence Berkeley National Laboratory

Performance of the MCP-PMT for the Belle II TOP counter

A RICH Photon Detector Module with G-APDs

Survey of the performance of scintillation materials at low temperatures

Neutrino Oscillations and the Matter Effect

Physics of Neutrino Oscillation Experiments. in the near future

Solar and atmospheric ν s

Solar Neutrinos: Status and Prospects. Marianne Göger-Neff

- Future Prospects in Oscillation Physics -

David B. Cassidy. Department of Physics and Astronomy, University of California, Riverside, USA. Varenna, July 09

Particle Detectors Tools of High Energy and Nuclear Physics Detection of Individual Elementary Particles

Neutrinos: Yesterday, Today and Tomorrow. Stanley Wojcicki SLAC Summer Institute 2010 August 13, 2010

PMT Signal Attenuation and Baryon Number Violation Background Studies. By: Nadine Ayoub Nevis Laboratories, Columbia University August 5, 2011

Dual readout with tiles for calorimetry.

Measurement of the transverse diffusion coefficient of charge in liquid xenon

Research and Development of Large-Aperture Hybrid Photo-Detectors for Hyper-Kamiokande. Yusuke Suda Department of Physics, University of Tokyo

Future Reactor Expts. The Challenge. DoubleChooz. In France. Stanley Wojcicki. Far Detector m ~50 events/day

Directional Measurement of Anti-Neutrinos with KamLAND

Daniele Vivolo INFN Sec/on of Naples

Transcription:

A new design of large area MCP-PMT for the next generation neutrino experiments Sen. Qian Institute of High energy Physics, Chinese Academy of Science qians@ihep.ac.cn On Behalf of the Workgroup

Outline 1. Motivation: 2. The Design of the new MCP-PMT: 3. The progress of the MCP-PMT R&D. 4. Summary.

Current and Future Neutrino Experiments Large Format PMTs for the Neutrino Experiments Hamamatsu PMT Atmospheric neutrino exp. SuperK (Japan), HyperK/UNO,INO,TITAND, Solar neutrino exp. SNO (Canada), GALLEX/SAGE, Borexino, XMASS, Accelerator neutrino exp. T2K (Japan ), Nova (American), Minos, OPERA, MiniBooNE, Reactor neutrino exp. KamLAND (Japan), Daya Bay (China), Double Chooz (France) Reno (Korea), The Future neutrino exp. Low Energy Neutrino Astrophysics LAGUNA-LBNO (European) Daya Bay II (China),

KamLAND: an Example of Reactor Neutrino Experiment KamLAND Detector Current benchmark: Liquid Scintillator (LS) The Mass of LS: ~1kt Attenuation length of LS: ~15m Light yield of LS: ~~ 8000 photons/mev ~~ PPO% ~ 1.5g/l 1 kt LS Photon Detector (PMT) Hamamatsu PMT:~~17 inch and 20 inch Quantum Efficiency (QE): ~20% Collection efficiency of first dynode (CE): ~70% Photon detection efficiency (PDE): ~14% Photocathode coverage : ~34% 20 PMT 17 PMT Light Yield of the Whole Detector: 250 p.e / Million electron volts energy (MeV) The number of the detected p.e per neutrino reaction

Next generation Neutrino Experiment in China 60 km from Daya Bay and Haifeng Daya Bay II The Main Scientific goals: Mass Hierarchy Mixing matrix elements Supernovae Haifeng geo-neutrinos Daya Bay Measuring Mass Hierarchy Huge Detector : LS + PMT Baseline: 60 km from the Reactor Energy resolution ~ 2%/ E L. Zhan, et. al., Phys.Rev.D 78:111103,2008 L. Zhan, et. al., Phys.Rev.D 79:073007,2009 sin 2 (2θ13) ~( 1-2 ) %

KamLAND Daya Bay II Detector ~1 kt Liquid Scintillator > 10 kt Liquid Scintillator Energy Resolution 6%/ E 2%/ E Light yield 250 p.e./mev 2500 p.e./mev How? 10 Ongoing R&D: Highly transparent LS: Attenuation length 2.5 ; KamLAND: 15m Daya Bay II : 25m; High light yield LS: PPO% 3?? 30% 45%; KamLAND: 1.5g/l Daya Bay II : 5g/l; Photocathode coverage : 2 KamLAND: 34% Daya Bay II : ~ 80% High PDE PMT: Photon detection efficiency 2; 20 UBA/SBA photocathode PMT from Hamamatzu? QE > 40% New large area PMT? QE > 40%?

Conventional PMT Glass shell Photoelectron Photocathode Aluminum mirror coating Glass Joint Dynode The first PMT in the world in 1933 Kubetsky s tube Anode Signal Base Photomultipliers are constructed from a glass envelope with a high vacuum inside, which houses a photocathode, several dynodes, and an anode.

The Quantum Efficiency of PMT The QE of 20 PMT-R3600 The QE of SBA/UBA High QE PMTs: SBA (35%) and UBA (43%) QE of photocathode ~ 20% are only available in small format (< 3" diameter?) CE of first dynode is ~ 70% PDE ~14% Hamamatsu 20" PMT Can we improve the Quantum Efficiency of Photocathode or Photon Detection Efficiency for the large area 20 PMT?

The new design of a large area PMT High photon detection efficiency + Single photoelectron Detection + Low cost 1) Using two sets of Microchannel plates (MCPs) to replace the dynode chain 2) Using transmission photocathode (front hemisphere) ~ 4π viewing angle!! and reflective photocathode (back hemisphere) QE Transmission cathode: 20% Reflection cathode: 40% MCP CE: 60% PDE 20% * 60% = 12% 70% * 40% * 60% = 17% Total Photon Detection Efficiency: ~30% Photon Detection Efficiency: 14% 30% ; ~2 at least!

Project team and Collaborators Institute of High Energy Physics, CAS R&D effort by Yifang Wang; & Tianchi Zhao; Jun Cao; Yukun Heng, Sen Qian; et al Collaborators Xi an Institute of Optics and Precision Mechanics of CAS; JInshou Tian; Xiangyan Xu; Huling Liu; Xibing Cao; Nanjing Electronic Devices Institute; Huirui Li; Jun Shentu; Xiaoyun Wang; Deling Liu; Wenjin Zhao; Nanjing University; Ming Qi;

The R&D plan of the MCP-PMT Design 5 (8 ) prototype transmission 5 (8 ) prototype Transmission +Reflection 20 prototype Transmission +Reflection Photocathode MCP vacuum equipment Prototype PreAMP & Base SPE Photomultiplier Glass

Photomultiplier design ------ Simulation!! The possibility of the 20 spherical MCP-PMT; The properties of MCP-PMT (8, 12, 20 ); Photocathode ------ large area!! Try to produce the alkali metal dispensers (AMD) to control the quality; Glass ------ large and low radiation background!! Superb water-resistance characteristics; Low radioactive background glass; MCP ------ low cost!! The Progress of the R&D currently Try to find MCPs for SPE detection with lost cost (~ hundreds ); Base ------ added with preamplifier!! The gain of the 2-piece MCP-multiplier is about 10 5 ; To detect the SPE, the Pre-amplifier is needed! These Progress will be detailed discussed in the following Parts!

The Simulation work 20 MCP-PMT 1. Simulate the possibility of the 20 spherical MCP-PMT --Electron Multiplier: small size MCP (φ=18mm) large Dynode chain ; --photocathode area: transmission+ reflection, nearly 4π effective area ; --Could the small MCP collect all the photoelectron from the photoelectron? Photocathode MCP Electron Multiplier MCP Anode --Yes! Nearly all the photoelectrons could be collected by the small MCP!

The Simulation work properties of MCP-PMT Hit position of the photoelectron in the MCP Transit Time Spread(T.T.S) Electric field intensity distribution electric potential distribution Effective diameter of MCP is 18mm; Working voltage: V cathode =-2500V; V focus electrode =-2000V; V MCP =-2000V; V anode =0V;

spherical symmetry glass shell photoelectron produced from photocathode photoelectron collected by MCP the performance of different MCP-PMT without the geomagnetic field (GM) Transmission photocathode Reflection photocathode size Width of Blind Ring Collection efficiency Transit Time Spread (T.T.S) Hit position In MCP Collection efficiency Transit Time Spread (T.T.S) Hit position In MCP inch mm % ns mm % ns mm 8 10 97.5 1 < 12 95.4 4.8 < 12 10 13 97.4 2.3 < 12 96.2 5.1 < 12 12 14 97.7 3.3 < 14 96.8 8.5 < 16 20 36 96.4 7.1 < 16 96.1 10.1 < 18

Large area photocathode & Glass 1.Why we need the alkali metal dispensers (AMD)? To achieve 20 large photocathode, the standard alkali metal dispensers could control the quality of the PMTs during the production process. Getter K Cs Glass bulb for the MCP-PMT 1. superb water-resistance characteristics; --to be submerged in liquid for long time in the experiment. 2. low radioactive background; AMD used in a PMT --to reduce the background rates Table: The background test of different types of electric vacuum glass (unit: ppb) Project Glass U 238 Th 232 K 40 Daya Bay I? 153±25 335±90 16.5±4.5 KamLAND HARIO -32# 150 240 10 Daya Bay II CN-2# (OLD Data) 24.4 27.5 7.7 CN-2# (NEW Data) On testing!

The low cost MCP ~ 1 mm MCP Why the cost of the MCP is usually high? ----Low production yield! ~ 20% ----MCP mainly used for optoelectronic imaging device MCP-PMT Operation Principle Channels cost disqualified MCP for Imaging device 1 asymmetrical surface; 2 Blind channels; 3 Non-uniform gain of the channels ; 4 emission flash Acceptable MCP for SPE detection cost North Night Vision Technology Limited Company (NNVT), our partner has over 20 years of experience in MCP production. Could supply us the MCP used in 18mm with low cost.

The size of the glass joint The size of the joint of the glass will affected electric potential distribution 1. Better Mechanical strength big size; Less distorted electric field small size; 2. The size of the MCP for 20 inch PMT : Diameter of area: ~ 25 mm; 3. The diameter of the glass joint ~ 80 mm; 4. All the prototypes with different inch (5~20) ; using the same size glass joint ~ 2 inch

The Base with preamplifier The electron multiplier consists of two conventional MCP, ~ 10 5 gains Current-sensitive preamplifier Equivalent noise charge Unity-Gain bandwidth Rise time < 2000 electron 300 MHz 1~2 ns Amplification 20 ~ 50 Output impedance Signal polarity 50 Ω negative

Prototypes 5 MCP-PMT transmission photocathode MCP 2 MCP-PMT

Performance of the 5 -prototype Rise time:~ 2ns; Fall time: ~3ns; Signal amplitude ~7mV; Spectral Response Peek wavelength Anode Dark Current Cathode luminous sensitivity 300~ 750 nm 370 nm < 50 na > 50 ua/lm Gain > 1.0*10 5

The single photoelectron spectrum and the multi-photoelectron spectrum of the PMT The photoelectron spectrum of the XP2020 PMT 5 MCP-PMT XP2020 SPE vs the Voltage of the PMT pedestal SPE SPE vs the luminance of the LED light **--adjust the working voltage of the LED to adjust the luminance of the LED light.

The photoelectron spectrum of a prototype: 5 IHEP-MCP-PMT XP2020 5 MCP-PMT SPE vs the Voltage of the PMT pedestal MPE MPE vs the luminance of the LED light **--adjust the working voltage of the LED to adjust the luminance of the LED light.

8 ellipse MCP-PMT 8 prototype transmission --Electron Multiplier: small size MCP (φ=18mm) --photocathode area: transmission + reflection photocathode The photoelectron collected by the electron multiplier MCP d? The overview of the prototype The hit position of the photoelectron in MCP was affected by the distance between the MCP and the center of the ellipse. Whit is the best position for the better collection efficiency?

Summary 1. A new type of MCP-PMT is designed for the next generation neutrino exp. Large ares: ~ 20 ; High photon detection efficiency: ~30%, al least 2 than normal PMT; Low coat: ~ low cost MCPs; 2. The R&D process is composing with 3 step. 1 5 (8 ) prototype with transmission photocathode; 2 5 (8 ) prototype with transmission and reflection photocathode; 3 20 prototype with transmission and reflection photocathode; 3. The R&D work is divided into 6 Parts to product the prototype to detect SPE: 1Photocathode; 2MCP; 3Glass; 4Photomultiplier; 5vacuum equipment; 6PreAMP & Base; There are lots of work to do!

The end! 谢谢! Thanks for your attention!

Characteristics unit 13# 16# 22# 25# Test voltage v V -2000-2000 -1970-2020 Cathode current I K na -1.2-3.46-10.56-31 Cathode luminous sensitivity S K ua/lm 4.5 12.9 39.5 117 Anode Current I A na 12.5 42 35.7 70 Anode Dark Current I D na 0.7 16.7 2.39 18 Anode luminous sensitivity S A A/lm 2.57 5.5 7.22 9.15 Gain G - 5.7*10 5 4.2*10 5 1.8*10 5 1.01*10 5 S k = I k ϕ k S A = I A ϕ A I D G = S S A k luminous flux: ϕ k ϕ A = 2.67*10-4 lm = 4.59*10-9 lm