Deep Underground Large Water Cerenkov Detectors Two types have been proposed. 1) Horizontal cylinders ~60 m diameter by 180 m long – UNO & HyperKamiokande.

Slides:

Advertisements

Similar presentations

UNO R&D and  UNO Possible early use of Henderson Upper Campus UNO collaboration has submitted an R&D proposal covering Excavation R&D of large caverns.

Advertisements

Status of the XMASS experiment S. Moriyama for the XMASS collaboration Kamioka observatory, Institute for Cosmic Ray Research, Univ. of Tokyo, July 27,

11/05/06GDR-Neutrino à Orsay (LAL)1 GDR-Neutrino (10-11 mai 2006) L. Mosca (CEA-Saclay) The MEMPHYS project (Laboratory excavation) MEgaton Mass PHYSics.

DMSAG 14/8/06 Mark Boulay Towards Dark Matter with DEAP at SNOLAB Mark Boulay Canada Research Chair in Particle Astrophysics Queen’s University DEAP-1:

Prospects for 7 Be Solar Neutrino Detection with KamLAND Stanford University Department of Physics Kazumi Ishii.

Liquid Xenon Gamma Screening Luiz de Viveiros Brown University.

February 8 th, 2001 Status Report: SciFi for MICE Edward McKigney Imperial College London.

1 Evidence of Neutrino Oscillation from Super-Kamiokande and K2K Neutrino physics at Super-Kamiokande –Detector overview –Atmospheric neutrinos –Solar.

PLAN Morning Talk – Long Base Line Neutrino Oscillations – 1) Beam line & brief description of detector 2) Neutrino interaction signal Afternoon talk –

The XENON Project A 1 tonne Liquid Xenon experiment for a sensitive Dark Matter Search Elena Aprile Columbia University.

Underground Neutrino Observatory The proposed next-generation underground water Čerenkov detector to probe physics beyond the sensitivity of the highly.

MICE Collaboration Meeting March 29 - April 1, CERN MICE alignment, tolerances and supports Tuesday March 30 Room Edgar Black/IIT March17-

Special Issues on Neutrino Telescopy Apostolos G. Tsirigotis Hellenic Open University School of Science & Technology Particle and Astroparticle Physics.

K. Nakamura NNN05, Aussois, April Overview of Hyper-Kamiokande R&D Kenzo NAKAMURA KEK April 7-9, 2005 NNN05 Aussois, Savoie, France.

The HERMES Dual-Radiator Ring Imaging Cerenkov Detector N.Akopov et al., Nucl. Instrum. Meth. A479 (2002) 511 Shibata Lab 11R50047 Jennifer Newsham YSEP.

LBNE Reconfiguration Workshop – April 2012 FD Assumptions and Cost Estimate 1 Bruce Baller.

General meeting LAGUNA LAGUNA – Fréjus site

New particle ID detector for Crystal Ball at MAMI-C Daniel Watts, University of Edinburgh John Annand 1, B. Briscoe 3, A. Clarkson 2, Evie Downie 1, D.

Niels Bohr hypothesized the existence of quantum mechanical restrictions on the principle of energy conservation, but Pauli couldn’t buy that: Wolfgang.

Simulation study of RENO-50 Jungsic Park Seoul National University RENO-50 International Workshop June 13-14, 2013 Hoam Faculty House, Korea.

Eun-Ju Jeon Sejong Univ. Sept. 09, 2010 Status of RENO Experiment Neutrino Oscillation Workshop (NOW 2010) September 4-11, 2010, Otranto, Lecce, Italy.

Preparing Foundations for Cylinders & ASME Tanks

SINP MSU, July 7, 2012 I.Belolaptikov behalf BAIKAL collaboration.

1 Discussion for basic options — engineering video conference July 12, 2006 Outline Water pool — advantages — issues, problems, engineering options Aquarium.

Homestake Massive Detector & Long Range Neutrino Oscillation Program 1) Introduction – Ken Lande 2) Long Base Line Neutrino Oscillations – Milind Diwan.

11-2 Volume of Prisms & Cylinders Mrs. Ballard & KL Schofield.

Detectors and Cross Talk Presented below are cross talk measurements carried out on 2 Burle and 1 Hamamatsu MCP PMTs and 1 Hamamatsu MultiAnode PMT (MAPMT).

Pre-Excavation Rock Evaluation 1)Goal- Excavate the largest possible safe and stable detector chamber 2) Procedure a) measure characteristics of the rock.

Wednesday, Feb. 14, 2007PHYS 5326, Spring 2007 Jae Yu 1 PHYS 5326 – Lecture #6 Wednesday, Feb. 14, 2007 Dr. Jae Yu 1.Neutrino Oscillation Formalism 2.Neutrino.

Cherenkov Counters for SoLID Z.-E. Meziani on behalf of Simona Malace & Haiyan Gao (Duke University) Eric Fuchey (Temple University) SoLID Dry Run Review,

Water Tank as the Outer Muon Veto Mingjun Chen

DESIGN AND CONSTRUCTION OF A MODULAR MASSIVE DETECTOR AT THE HOMESTAKE LAB Modular Mass – 100 Kilotons Modular Shape –Cylinder –50m dia x 50m high Depth.

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

Deep Underground Large Water Cerenkov Detectors Two types have been proposed. 1) Horizontal cylinders ~60 m diameter by 180 m long – UNO & HyperKamiokande.

STATUS OF MUV3 CONSTRUCTION A joint IHEP Protvino – Mainz – Pisa project MUV3  Proposed by Italo Mannelli: Thick scintillator tiles with direct light.

MINERvA Main INjector ExpeRiment for -A is the symbol for the neutrino. The beam that is sent to MINERvA is made out of neutrinos. In chemistry, an A stands.

EUROn Safety 13/06/2012M. Dracos1. Safety workshop 13/06/2012M. Dracos2 A first two days safety workshop has been organized at CERN last May (

Gary Feldman MINOS in Cambridge 24 March NO A Update MINOS Collaboration Meeting Cambridge, England 24 March 2009 Gary Feldman.

P.Auger, a major step: Need high statistics large detection area : 2 x3000 km² Uniform sky coverage 2 sites located in each hemisphere Argentina and USA.

VVS Prototype Construction at Fermilab Erik Ramberg 26 February,2002 Design issues for VVS Details of VVS prototype design Schedule and Budget Testing.

KOPIO Catcher System RSVP Baseline Review Brookhaven National Laboratory April 20, 2005 Noboru Sasao / Tadashi Nomura (Kyoto U.)

Mechanical Designs of The Central Detector Jinyu Fu

Catania 11 ICATPP october, 2009 Como 1/12 Catania Comparative measurements of the performances of four super bialkali large.

Asian facilities YangYang Underground Laboratory (Korea) India-based Neutrino Observatory(India) JinPing Deep Underground Laboratory (China) Kamioka Observatory.

EUROnu WP5 Detector Costing EuroNu Annual General Meeting, Strasbourg 3 June 2010 Paul Soler.

Introduction bin/Dev_DocDB/DisplayMeeting?conferenceid=54http://juno.ihep.ac.cn/cgi- bin/Dev_DocDB/DisplayMeeting?conferenceid=54.

Magnetized hadronic calorimeter and muon veto for the K +   +  experiment L. DiLella, May 25, 2004 Purpose:  Provide pion – muon separation (muon veto)

LAr1 Plans at FNAL Bruce Baller - Fermilab. Outline LAGUNA Meeting - Mar  LBNE LAr detector overview  Prototyping plan  1 kton prototype.

Medium baseline neutrino oscillation searches Andrew Bazarko, Princeton University Les Houches, 20 June 2001 LSND: MeVdecay at rest MeVdecay in flight.

E. W. Grashorn and A. Habig, UMD, for the MINOS Collaboration The Detectors of The Main Injector Neutrino Oscillation Search (MINOS) Experiment The MINOS.

Current status of XMASS experiment 11 th International Workshop on Low Temperature Detectors (LTD-11) Takeda Hall, University of Tokyo, JAPAN 8/1, 2005.

FCC-hh MDI 5 th Meeting Friday 13 th March 2015 Civil Engineering Layouts for Experimental Caverns – First Draft Charlie Cook (GS), John Osborne (GS)

M EGATON M ODULAR M ULTI -P URPOSE N EUTRINO D ETECTOR Ventilation Cooling Mark A. LaurentiMarch 2002 Modular Configuration.

Simulation of heat load at JHF decay pipe and beam dump KEK Yoshinari Hayato.

Hiroyuki Sekiya ICHEP2012 Jul 5 The Hyper-Kamiokande Experiment -Neutrino Physics Potentials- ICHEP2012 July Hiroyuki Sekiya ICRR,

LSc experiment set-up and research results LAGUNA 2014 Hanasaari, August 25, 2014 Wladyslaw H. Trzaska.

Neutron Shield/Muon Veto (WBS 1.3) and Underground Installation Issues (WBS 1.6) May 11, 2009 Erik Ramberg.

14/07/2008 Massimo Benettoni PMTs need replacement. SOB volume reduction is desirable. detectors: PMT Hamamatsu H8500 detectors resolution allows smaller.

“Megaton” Cerenkov Detector - Excavation Kenneth Lande, Univ. of Pennsylvania 4200 mwe Depth.

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.

Mark Vagins Kavli IPMU, University of Tokyo 4 th Open Meeting for the Hyper-Kamiokande Project Kashiwa January 28, 2014 Gd Status.

Jim Brennan for the WATCHMAN Collaboration Detector Engineering Design Simulation courtesy G. Jocher/J Learned, U Hawaii This work was performed under.

EURONu Collaboration Board,

$150K Chicago/ANL seed funding for Braidwood site investigation

Detector hall in mountain regions

Summary of fiducial volume test at KEK

Evaluate the integral using the indicated trigonometric substitution {image} {image}

Detector hall in mountain regions

Development of hybrid photomultiplier for Hyper-Kamiokande

Presentation transcript:

Deep Underground Large Water Cerenkov Detectors Two types have been proposed. 1) Horizontal cylinders ~60 m diameter by 180 m long – UNO & HyperKamiokande 2) Vertical cylinders – diameters 40 – 57 m, height constrained by PMT pressure limit – SuperKamiokande, Homestake and Frejus

2. Hyper-Kamiokande and T2K-II 4MW J-PARC beam 1Mton (0.54Mton fiducial mass) 2years of run + 6 years of anti- run  O(0.5 ・ 10 6 ) events for both runs

Electronics Hut PMTs 50,000 t Water Tank  39.3 m  H41.4 m Control Units & Observation Room Mt. Ikenoyama Elevation 1368 m SK 1,000 m SL 350 m Access Tunnels SL 350 m SL 365 m SL m

DESIGN AND CONSTRUCTION OF A MODULAR MASSIVE DETECTOR AT THE HOMESTAKE LAB Modular Mass – 100 Kilotons - fiducial Modular Shape –Cylinder –53m dia x 53m high Depth – 4200 mwe (cosmic ray rate = 0.1Hz) Photocathode coverage – 25% Initial Detector – 3 modules (300 kilotons) Construction time - 5 years for 3 modules Cost - ~ $100 M / module Ultimate detector – 10 modules (1 Megaton)

SINGLE 100 KILOTON MODULE - HOMESTAKE March 2002Mark A. Laurenti

MEMPHYS at Fréjus Up to 5 shafts possible Each 57m diam., 57m high For most studies assumed 3 x 145 ktons. Water Cerenkov Per shaft: 81,000 12” PMT’s  80 M€ including electronics (65M$ KL 62M$ ) +80 M€ for civil engineering. (65M$ KL 29M$ ) Depth: 4800 m.w.e FOR 100 ktons)

Rock Mechanics and Excavation Rock characteristics will be measured & evaluated by Bill Pariseau (Utah) & NIOSH– Now an official NIOSH project (NIOSH is new name for U.S. Bureau of Mines) Chamber design by Mark Laurenti – former Homestake chief mine engineer and Underground Superintendent

Photomultipliers Plan to use 11 –12 inch diameter hemispherical PMT (Frejus plans to use 12 inch dia PMTs) Smaller diameter PMTs reduces the danger of chain implosion – (SuperK accident) Gives improved angular resolution ~PMTdia/Detector radius Multiple manufacturer option Must determine hydrostatic pressure tolerance of PMTs -

PMT Hydrostatic Tests Will use 32 Hamamatsu 10 1/2 inch dia.hemispherical PMTs for ultimate pressure tests and for long term (multi- year) static pressure tests – insure no long term fatigue effects Will also measure effect of pressure shocks

PMT Installation & Maintenance Side PMTs will be mounted on a 52 meter dia. cylinder – leaving a ½ m thick veto region – light divider part of PMT mount Fiducial region is 50 m diameter & 50 m high (may be increased if PMT hydrostatic tests indicate greater depth possible) PMTs installed or removed without draining water fill -

Water Fill Have estimates for a commercial, “turn key” system, fill one detector in < 2 months. Plan to purify inflowing underground water – thus avoid removing water from the surface water system -

One Module Three Modules Construction (including 30% contingency) $29.1M$66.1M Photomultipliers and Electronics $62.1M$186.3M Other$7.9M Contingency (Other + PM) $17.5M$48.6M TOTAL$116.6M$308.9M

Chamber Excavation One Chamber Three Chambers Labor & benefits$6.060M$12.030M Mining Equipment Operation1.430M4.279M Supplies4.961M14.685M Precast concrete liner3.575M10.725M Outside contractor0.132M0.396M Plastic liner0.250M0.750M Rock removal1.000M3.000M Mining Equipment-Purchase5.000M Contingency-30%6.722M15.260M TOTAL29.130M66.125M

Photomultipliers & Electronics Cost for one PM 28 cm dia PM tube$880 Installation/PM$165 Electronics/PM$120 Cable/PM$77 Total per photomultiplier tube$1242 One 100 kiloton Detector$62.1M Three 100 kiloton Detectors186.3M

Other items Development Labor$3.000M Water Purification System* (for 10 modules) 4.500M Calibration equipment0.400M TOTAL$7.900M

SUMMARY 1) Initial Detector – Three 100 kiloton modules 2) Total cost - $308M. 3) Construction time – 5 years

Questions for Hamamatsu 1) What is the quantum efficiency of your 10 ½ inch diameter PMTs? 2) What is the electron collection efficiency? 3) What is the PMT rise time and jitter? 4) Do you have any plans for a 12 inch dia. Hemispherical PMT? 5) Any other PMT developments of interest to us?