Hyper-Kamiokande project and R&D status Hyper-K project Motivation Detector Physics potential study photo-sensor development Summary Kamioka.

Slides:



Advertisements
Similar presentations
Trigger issues for KM3NeT the large scale underwater neutrino telescope the project objectives design aspects from the KM3NeT TDR trigger issues outlook.
Advertisements

NNN02 16 January, 2002 CERN Maury Goodman – Argonne Lab Large Detector workshop Current Status and Prospects of Approved Proton Decay Search Experiments.
Sinergia strategy meeting of Swiss neutrino groups Mark A. Rayner – Université de Genève 10 th July 2014, Bern Hyper-Kamiokande 1 – 2 km detector Hyper-Kamiokande.
PLAN Morning Talk – Long Base Line Neutrino Oscillations – 1) Beam line & brief description of detector 2) Neutrino interaction signal Afternoon talk –
Alain Blondel Detectors UNO (400kton Water Cherenkov) Liquid Ar TPC (~100kton)
Lens ALens B Avg. Angular Resolution Best Angular Resolution (deg) Worst Angular Resolution (deg) Image Surface Area (mm 2 )
A feasibility study for the detection of SuperNova explosions with an Undersea Neutrino Telescope A. Leisos, A. G. Tsirigotis, S. E. Tzamarias Physics.
T2K experiment at J-PARC Epiphany 2010D. Kiełczewska1 For T2K Collaboration Danuta Kiełczewska Warsaw University & Sołtan Institute for Nuclear Studies.
K. Nakamura NNN05, Aussois, April Overview of Hyper-Kamiokande R&D Kenzo NAKAMURA KEK April 7-9, 2005 NNN05 Aussois, Savoie, France.
Latest developments in Hamamatsu Large Format PMTs
T. Sumiyoshi (TMU) 30, Nov del Carmen 1 Development of HPD (HAP D) Photon-detector for the Aerogel RICH Photon-detector for the Aerogel.
1 The Daya Bay Reactor Electron Anti-neutrino Oscillation Experiment Jianglai Liu (for the Daya Bay Collaboration) California Institute of Technology APS.
Peter Križan, Ljubljana March 17, 2006 Super B Workshop, Frascati Peter Križan University of Ljubljana and J. Stefan Institute Aerogel RICH and TOP: summary.
I. Giomataris NOSTOS Neutrino studies with a tritium source Neutrino Oscillations with triton neutrinos The concept of a spherical TPC Measurement of.
KamLAND Experiment Kamioka Liquid scintillator Anti-Neutrino Detector - Largest low-energy anti-neutrino detector built so far - Located at the site of.
1 Max-Planck-Institut fuer Physik, Muenchen, Germany, 2 Humboldt-Universituet Berlin, Germany, 3 Univ. Complutense, Madrid, Spain, 4 ETH, Zurich, Switzerland,
Solar neutrino measurement at Super Kamiokande ICHEP'04 ICRR K.Ishihara for SK collaboration Super Kamiokande detector Result from SK-I Status of SK-II.
Status of the NO ν A Near Detector Prototype Timothy Kutnink Iowa State University For the NOvA Collaboration.
The Earth Matter Effect in the T2KK Experiment Ken-ichi Senda Grad. Univ. for Adv. Studies.
KamLAND : Studying Neutrinos from Reactor Atsuto Suzuki KamLAND Collaboration KEK : High Energy Accelerator Research Organization.
Dec. 13, 2001Yoshihisa OBAYASHI, Neutrino and Anti-Neutrino Cross Sections and CP Phase Measurement Yoshihisa OBAYASHI (KEK-IPNS) NuInt01,
Karsten M. Heeger US Reactor  13 Meeting, March 15, 2004 Comparison of Reactor Sites and  13 Experiments Karsten Heeger LBNL.
Experimental set-up for on the bench tests Abstract Modeling of processes in the MCP PMT Timing and Cross-Talk Properties of BURLE/Photonis Multi-Channel.
TAUP Searches for nucleon decay and n-n oscillation in Super-Kamiokande Jun Kameda (ICRR, Univ. of Tokyo) for Super-Kamiokande collaboration Sep.
1 DISCOVERY OF ATMOSPHERIC MUON NEUTRINO OSCILLATIONS Prologue First Hint in Kamiokande Second Hint in Kamiokande Evidence found in Super-Kamiokande Nov-12.
JHF-Kamioka Neutrino Oscillation Experiment using JHF 50 GeV PS Y.Itow ICRR,Univ.of Tokyo Jul27,2002 Jul27,2002 ICHEP02 Amsterdam Introduction Facility.
1 The JHF-Kamioka Neutrino experiment 1.Introduction 2.Overview of the experiment 3.Physics sensitivity in Phase-I 4.Physics sensitivity in Phase-II 5.Summary.
Development of TOP counter for Super B factory K. Inami (Nagoya university) 2007/10/ th International Workshop on Ring Imaging Cherenkov Counters.
1 水质契仑科夫探测器中的中子识别 张海兵 清华大学 , 南京 First Study of Neutron Tagging with a Water Cherenkov Detector.
Yoshihisa OBAYASHI, Oct. Neutrino Oscillation Experiment between JHF – Super-Kamiokande Yoshihisa OBAYASHI (Kamioka Observatory, ICRR)
NuMI Off-Axis Experiment Alfons Weber University of Oxford & Rutherford Appleton Laboratory EPS2003, Aachen July 19, 2003.
Development of Multi-Pixel Photon Counters(MPPC) Makoto Taguchi Kyoto University.
NuFact02, July 2002, London Takaaki Kajita, ICRR, U.Tokyo For the K2K collab. and JHF-Kamioka WG.
Neutrino Oscillations at Homestake from Chlorine to the Megadetector Ancient Origins of the Question ~1860 Darwin publishes “On The Origin of Species”-
Road Map of Neutrino Physics in Japan Largely my personal view Don’t take too seriously K. Nakamura KEK NuFact04 July 30, 2004.
Multipixel Geiger mode photo-sensors (MRS APD’s) Yury Kudenko ISS meeting, KEK, 25 January 2006 INR, Moscow.
Jun Cao Jan. 18, 2004 Daya Bay neutrino experiment workshop (Beijing) Detector Module Simulation and Baseline Optimization ● Determine module geometric.
Daya Bay Reactor Neutrino Experiment On behalf of the DayaBay collaboration Virginia Polytechnic Institute and State University Joseph ykHor YuenKeung,
1/27/2016Katsushi Arisaka 1 University of California, Los Angeles Department of Physics and Astronomy Katsushi Arisaka XAX 10.
Neutrino Oscillations at Super-Kamiokande Soo-Bong Kim (Seoul National University)
Takaaki Kajita ICRR, Univ. of Tokyo Nufact05, Frascati, June 2005 Based on reports at NNN05 Next generation of Nucleon decay and Neutrino detectors
1 Muon Veto System and Expected Backgrounds at Dayabay Hongshan (Kevin) Zhang, BNL DayaBay Collaboration DNP08, Oakland.
1 Constraining ME Flux Using ν + e Elastic Scattering Wenting Tan Hampton University Jaewon Park University of Rochester.
October 2002Sienna, JL. Faure, DAPNIA/SPP In 8th Topical Seminar on Innovative Particle and Radiation Detectors Jean-louis Faure CEA-DAPNIA-SPP Progress.
Current status of XMASS experiment 11 th International Workshop on Low Temperature Detectors (LTD-11) Takeda Hall, University of Tokyo, JAPAN 8/1, 2005.
Water Cherenkov detector - brief status report - Kenji Kaneyuki Research Center for Cosmic Neutrinos, ICRR, Univ. of Tokyo.
1 Limitations in the use of RICH counters to detect tau-neutrino appearance Tord Ekelöf /Uppsala University Roger Forty /CERN Christian Hansen This talk.
Cherenkov Tracking Calorimeters D. Casper University of California, Irvine.
NUMI NUMI/MINOS Status J. Musser for the MINOS Collatoration 2002 FNAL Users Meeting.
September 10, 2002M. Fechner1 Energy reconstruction in quasi elastic events unfolding physics and detector effects M. Fechner, Ecole Normale Supérieure.
PAC questions and Simulations Peter Litchfield, August 27 th Extent to which MIPP/MINER A can help estimate far detector backgrounds by extrapolation.
Review of experimental results on atmospheric neutrinos Introduction Super-Kamiokande MACRO Soudan 2 Summary Univ. of Tokyo, Kamioka Observatory.
Hiroyuki Sekiya ICHEP2012 Jul 5 The Hyper-Kamiokande Experiment -Neutrino Physics Potentials- ICHEP2012 July Hiroyuki Sekiya ICRR,
Development of UV-sensitive MPPC for upgrade of liquid xenon detector in MEG experiment Daisuke Kaneko, on behalf of the MEG Collaboration µ γ Liquid xenon.
Status of the NO A Experiment Kirk Bays (Caltech) on behalf of the NO A collaboration Lake Louise Winter Institute Saturday, Feb 22, 2014.
BSM Group Activities DUNE Collaboration Meeting –ND Physics Jan. 14, 2016 Jae Yu Univ. of Texas at Arlington.
Observation Gamma rays from neutral current quasi-elastic in the T2K experiment Huang Kunxian for half of T2K collaboration Mar. 24, Univ.
Open and Hidden Beauty Production in 920 GeV p-N interactions Presented by Mauro Villa for the Hera-B collaboration 2002/3 data taking:
23/11/05BENE meeting at CERN1 (22-25 November 2005) L. Mosca (CEA-Saclay) The MEMPHYS project MEgaton Mass PHYSics in a Large International Underground.
The XXII International Conference on Neutrino Physics and Astrophysics in Santa Fe, New Mexico, June 13-19, 2006 The T2K 2KM Water Cherenkov Detector M.
The dynamic range extension system for the LHAASO-WCDA experiment
J. Musser for the MINOS Collatoration 2002 FNAL Users Meeting
Physics with the ICARUS T1800 detector
Chris Smith California Institute of Technology EPS Conference 2003
The Hyper-Kamiodande Project A New Adventure in n Physics
R&D status of a large HAPD
Recent Progress in Large Format PMTs
Daya Bay Neutrino Experiment
Development of hybrid photomultiplier for Hyper-Kamiokande
Ultra-high energy upward going muons in Super-Kamiokande II
Presentation transcript:

Hyper-Kamiokande project and R&D status Hyper-K project Motivation Detector Physics potential study photo-sensor development Summary Kamioka Observatory Masato Shiozawa For JHF-Kamioka νworking group

Super-K has not found nucleon decays in 3.5 years data τ/B(p→e + π 0 ) > 5.0 × years (90% CL) τ/B(p→ν K + ) > 1.9 × years (90% CL) Predicted lifetime of nucleon 4 fermion interactions 2 fermion – 2 sfermion interactions (SUSY models) One or two order of extension of Super- Kamiokande would reveal new physics!!! Next generation proton decay detector g 4 m p 4 Γ = : τ(p→e + π 0 ) = 10 35±1 years M X 4 h 4 m p 4 ____ Γ = : τ(p→K + ν) = years M Hx 2 M X 2

Same baseline with Super-K (295km) Enable higher statistics physics (22.5 kton  ~ 1000 kton) improved sensitivity for θ 13 measurement CP phase measurement in lepton sector test of the unitarity triangle Detector requirement good e/π 0 separation capability at low energy No magnetic field is needed Hyper-K as a far detector of 2 nd JHF ν

R&D Items for Hyper-K cavity design and assessment rock stress analysis excavation cost, time, optimization physics potential study optimization of photo-coverage, detector volume sensitivity for p  epi0, nuK+, background estimation SN, atmospheric nu, and others long baseline experiment(JHF), pi0 rejection etc. photo-sensor development low cost, high sensitivity mass production rate  automated production high pressure resistant other detector improvement longer light attenuation length? reducing reflection light?

Possible Design of Hyper-Kamiokande Super-K 40m

Possible Design of Hyper-Kamiokande (2) PMT Wall 45m  45m  2 planes  16 modules = 64,800 m 2 45m  46m  4 planes  4 modules = 33,120 m 2 45m  47m  4 planes  12 modules = 101,520 m 2 Total 199,440 m 2   200,000 PMTs if 1 PMT/m 2 Fiducial Volume 41m  41m  42m  4 modules = 282,408 m 3 41m  41m  43m  12 modules = 867,396 m 3 Total 1,149,804 m m 2 m 3 m 45m  45m  46m 41m  41m  42m 45m  45m  47m 41m  41m  43m Total 800m 16 compartments

Possible Design of Hyper-Kamiokande (3) #compartmen ts Total volume Fiducial volume PMT density #PMT Case1 8 1Mton0.57Mton 1PMT/m 2 100k Case2 8 1Mton0.57Mton 2PMT/m 2 200k Case3 16 2Mton1.15Mton 1PMT/m 2 200k Case4 16 2Mton1.15Mton 2PMT/m 2 400k PMT density should be optimized by gamma tagging in nuK+ search, pi0 rejection in long baseline experiment detector volume should be optimized by physics goals site, stable cavity design excavation cost, construction time photo-sensor cost, production time

Detector site candidate Super-K KAMLAND Mozumi site Tochibora site Super-K

Analysis for discovery of p → e + π 0 Tight momentum cut ⇒ target is mainly free protons efficiency=17.4%, 0.15BG/Mtyr No Fermi momentum No binding energy No nuclear effect Small systematic uncertainty of efficiency High detection efficiency Perfectly known proton mass and momentum free protonbound proton

Lifetime sensitivity with tight cut With 3σ(99.73%) level 1Mton ×20 years → ~ 1×10 35 years lifetime

How the signal looks like τ p /B(p→e + π 0 ) = 1×10 35 years S/N = 4 for 1×10 35 years ↓ S/N = 1 for 4×10 35 years τ p /B(p→e + π 0 ) = several×10 35 yrs is reachable by a large water Cherenkov detector Proton mass peak can be observed !

2. K + production by atmν νN → νN* ΛK + ~ 1 events/Mtyr (after pdecay cut) Backgrounds in p → νK + searches 1. prompt γ ~ 6 events/Mtyr most are misfitted vertex events μ spectram 2100 events/Mtyr (single-ring μ,π,proton) π + π 0 ~ 22 events/Mtyr we should reject them by improved vertex fitter very serious backgrounds if both Λ and K + are invisible K.Kobayashi 3. other unknown background?

Lifetime sensitivity with reduced BG With 3σ(99.73%) level 1Mton ×20 years → ~ 3×10 34 years lifetime Prompt γ tagging is essential

Photo-sensor development improving QE optimizing cathode materials, production methods larger (30-40inch) PMTs glass valve production is a key hybrid photo-detector (HPD) photo-cathode + AD(avalanche diode) simple structure  hopefully low cost good timing resolution ( ~ 1ns) good single p.e. separation

5 inch HPD prototype 5inch sensitive area 80mmφ e APD 3mmφ, GND bias voltage 150V photo-cathode – 8kV 100% coll. efficiency cathode 80mmφ mm cathode 120mmφ >10mm need higher voltage larger AD spherical cathode electron bombarded gain 1000 ×avalanche gain 50 = 50,000

5 inch HPD prototype (2) measured quantum efficiencytime response

5 inch HPD prototype (3) pulse height distribution (dark current) good single p.e. peak dark rate is 24kHz

5 inch HPD prototype (4) (a) cathode uniformity (b) anode uniformity geomagnetic effect is seen need higher voltage and/or larger AD

Spherical HPD glass photocathode reflector diode-1 diode-2 light photoelectrons Lead and support high efficiency simple structure  low cost  high production rate pressure resistant

to do list for the new photo-sensor gain up 1000(E.B.gain)×50(Av. gain)= 5×10 4  1×10 7 good focusing  higher voltage, spherical shape good control of AD position operation of AD in positive high voltage keep low dark rate pressure resistant (spherical shape) larger size

Summary of Hyper-K Rich physics potential τ p /B(p → e + π 0 ) ~ 1×10 35 years (3σ CL with 20Mtyr) τ p /B(p → ν K + ) ~ 3×10 34 years (3σ CL with 20Mtyr) Atmospheric, Supernova other physics 2 nd phase of JHF-Kamioka neutrino experiment R&D ’ s are in progress new photo-sensor