Introduction to the “Cavities and vessels” session ( by L. Mosca) 9h 10’ Presentation of the Laboratoire Souterrain de Modane (15’+ 5’) G. Gerbier (Saclay)

Slides:

Advertisements

Similar presentations

IDM2004 G. Gerbier LSM - Fréjus underground sites status and projects Gilles Gerbier CEA/Saclay - LSM.

Advertisements

Assay and Acquisition of Radiopure Materials Priscilla Cushman University of Minnesota July 14, 2010 NSF Review PRESENTATION(s) OUTLINE P. Cushman S4 Management.

NNN07 - Hamamatsu M. Russo - Switzerland Fréjus site pre-study and beyond NNN07 – HAMAMATSU Workshop on Next Generation Nucleon Decay and Neutrino.

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.

Heeger theta13, May A Neutrino Project at Diablo Canyon.

Underground Facilities Stub 2 Stub 2a,3 ‘H’ Area JIF Area The underground research facilities have evolved since dark matter studies began at Boulby. There.

KIGAM 1 Overview of geological situation for a possible T2KK detector site Chang-Ha Ryu Geotechnical Division Korea Intitute of Geoscience.

Henderson Mine Site. Henderson Mine Central Campus Shaft Collar Elev 10,400 ft Shaft Bottom Elev 7,500 ft LA Ramp Primary Access Ramp 3600 ft Central.

Large Excavations in the US Lee Petersen, CNA Consulting Engineers Presented by Chang Kee Jung, SUNY Stony Brook NNN05 Conference.

Michel Spiro Particle Physics at the Megawatt proton source. CERN 27 May 2004 Long-range programme in neutrino physics: superbeam, β beam, neutrino factory.

LAGUNA and Neutrino Physics NOW 2008 Lothar Oberauer TU München, Germany.

PD Connection with National Underground Lab R. Rameika Fermilab October 8, 2004.

B.Sadoulet CDMS DUSEL The Deep Underground Science and Engineering Laboratory Site Independent Study The process The science Infrastructure requirements.

NSF VISION in PARTICLE and NUCLEAR ASTROPHYSICS Richard N. Boyd  The Present  Dark Matter  Ultra high energy cosmic rays  Ultra high energy gamma rays.

October 12th, 2006L. Mosca LAGUNA Meeting in Zurich 1 IPP- ETH Zurich October 12th, 2006 LAGUNA Meeting WG 7: Safety and Environment Report by L. Mosca.

Status of activities of the WP4 on Radiopurity of Materials Pia Loaiza Laboratoire Souterrain de Modane JRA1 meeting Paris February 14 th, 2006.

Low radioactivity at the Modane Underground Laboratory

ILIAS Physics in deep underground laboratories JRA1 : Low background techniques WP4 : Radiopurity of materials Pía Loaiza Laboratoire Souterrain de Modane,

Eighth International SIGSOFT Symposium on Component-based Software Engineering (CBSE 2005) Software Components at Work.

LAGUNA at Fréjus LAGUNA/LAGUNA-LBNO General Meeting March 3 th -5 th, 2011, CERN Eng. Francesco Amberg.

Geosciences in an Underground Laboratory:

Nuclear Physics New Underground Laboratories in North America Steve Elliott Los Alamos National Laboratory.

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

Dark Matter Facts Baryonic Matter is only 20% of the Universe 80% is Dark Matter Dark Matter doesn’t interact with light or ordinary matter very frequently.

B.Sadoulet APS DUSEL The Deep Underground Science and Engineering Laboratory Site Independent Study The process The science Infrastructure requirements.

Deep Underground Science and Engineering Lab Hamish Robertson for the DUSEL S1 P/Is: E.W. Beier, C. Fairhurst, T.C. Onstott, R.G.H. Robertson, B. Sadoulet,

See UNO home page: UNO (Underground Nucleon decay and Neutrino Observatory) Jeffrey Wilkes University of Washington,

1 Lino Miramonti Milano University and INFN sez. Milano LRT Topical Workshop in Low Radioactivity Techniques (Sudbury, Canada) December 12-14, 2004.

UNO Cavity Liner System: Status Report and R&D Proposal D. Warner Colorado State University October 16, 2004.

L. MoscaNNN07 Conf - 2 to 5 Oct NNN07 Conference at Hamamatsu 2 to 5 October 2007 Report on LAGUNA Large Apparatus for Grand Unification and Neutrino.

September 4, 2003Jordan Goodman Ad Hoc Science Committee for the Proposed Laboratory for Science and Engineering at Homestake Who am I and what am I doing.

Deep Underground Laboratories and neutrino beams European facilities S. Katsanevas IN2P3 Thanks to Mezzetto, Bouchez, Mosca, Rubbia, Ronga, Cazes, Lindroos,Cadenas,

L. MoscaEPIPHANY Conf 6-8 Jan EPIPHANY Conference at Cracow “Physics in Underground Laboratories and its connection with LHC” - 6 to 8 January 2010.

18 January 2002CERN - Workshop on Large Detectors - L. R. Sulak1 Comparison of Detectors for Proton Decay L. R. Sulak Boston University overview and “long”

DUSEL Experiment Development and Coordination (DEDC) Internal Design Review July 16-18, 2008 Steve Elliott, Derek Elsworth, Daniela Leitner, Larry Murdoch,

Welcome to the 19 th Annual CMBG Conference Mike Hayes Exelon Generation.

Fraser Duncan Queen’s University Synergies in Low Background Techniques 26 July 2005 Underground Facilities at SNOLAB.

17 June 2004Neutrino L. Sulak1 the “Bright” Future for Neutrino Facilities around the world …a selected overview... L. R. Sulak CPPM Marseille and.

International Underground science: Status and Prospects Fabrice Piquemal Laboratoire Souterrain de Modane (CNRS/IN2P3 and CEA/IRFU) and CENBG (CNRS/IN2P3.

A large water shield for dark matter, double beta decay and low background screening. T. Shutt - Case R. Gaitskell - Brown.

VT-NRL Kimballton Kimballton Soudan Sudbury Homestake Henderson WIPP San Jacinto Icicle Creek.

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.

Monday, Feb. 19, 2007PHYS 5326, Spring 2007 Jae Yu 1 PHYS 5326 – Lecture #7 Monday, Feb. 19, 2007 Dr. Jae Yu 1.Neutrino Oscillation Experiments 2.Long.

Warszawa, July 3rd Measurements of natural radioactivity in European underground labs within the ILIAS project Jan Kisiel Institute of Physics, University.

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

A new underground laboratory at Frejus Jacques Bouchez CEA-SACLAY NNN05-Aussois April 7, 2005 Historical overview Latest developments Outlook.

Underground Laboratories and Low Background Experiments Pia Loaiza Laboratoire Souterrain de Modane Bordeaux, March 16 th, 2006.

Priscilla Cushman DUSEL S4 Workshop University of Minnesota Oct 1, 2009 Lead, SD Principle Investigators Priscilla Cushman (University of Minnesota) Dongming.

The EDELWEISS-II experiment Silvia SCORZA Université Claude Bernard- Institut de Physique nucléaire de Lyon CEA-Saclay DAPNIA/DRECAM (FRANCE), CNRS/CRTBT.

Deep Underground Science and Engineering Laboratory at Homestake1 Richard DiGennaro, LBNL DUSEL Project Manager 20 June 2008 Facility Planning for DUSEL.

Low Background Studies at the Soudan Underground Laboratory-9/20/ Low Background Studies at the Soudan Underground Laboratory The Soudan Underground.

1 LTR 2004 Sudbury, December 2004 Helenia Menghetti, Marco Selvi Bologna University and INFN Large Volume Detector The Large Volume Detector (LVD)

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

Muon-induced neutron background at Boulby mine Vitaly A. Kudryavtsev University of Sheffield UKDMC meeting, ICSTM, London, 27 June 2002.

Conventional Facilities for the Far Detector Options Assumptions and Cost Estimates T. Lundin April 25, 2012 LBNE Reconfiguration Workshop - 25, 26 - April-2012.

DRAFT US Department of Energy Underground Fire Protection Guide James Priest, PhD & James Niehoff DGS-SEE Seminar on Fire Protection for Physics Research.

China Deep Underground Laboratory and Dark Matter Search Hesheng Chen Institute of High Energy Physics.

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

W W P M Wireless Wearable Physiological Monitors.

NNN11 Conference at Zurich 7-9 November 2011 The LSM Laboratory at the Fréjus site : present and future by L. Mosca ( LSM/CEA/CNRS)

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.

LIGO-G Z Aspen Winter Conference 2005 Sessions:Mon ,16:30 – 19:30 Thu ,18:10 – 19:30 Fri ,09:40 – 10:50 Benefits.

LAGUNA and beyond GDR Neutrino at Orsay-PNO October 11th, 2010

Flavor Mixing of quarks.

TPC Conference, Paris 5 -7 December, 2016

Train-the-Trainer Sessions 240 sessions with 8,187 participants

Summary Some Issues of Future Consideration

WG 3 : Cavity Data Banks 9:00 ~ 10:30 Session-I 4 Talks

Assay and Acquisition of Radiopure Materials

Where in the World are We?

Presentation transcript:

Introduction to the “Cavities and vessels” session ( by L. Mosca) 9h 10’ Presentation of the Laboratoire Souterrain de Modane (15’+ 5’) G. Gerbier (Saclay) 9h 30’ Large excavations in the USA (25’+ 5’) L. Petersen (Minneapolis) talk presented by Chang Kee Jung (Stony Brook) 10h 00’ Study on the Excavation of the Hyper-KAMIOKANDE Cavern (35’+ 5’) T. Nakagawa (Tokyo) 10h 40’ Coffee break (20’) h 00’ Large excavations in Europe (25’+ 5’) M. Lévy (Paris) 11h 30’ Engineering of large and deep rock caverns for physics research (25’+ 5’) P. Duffaut (Paris) __________________________________________________________________________ 12h 00’ Concluding Remarks of the Conference (20’+ 5’) K. Nakamura (KEK)

Candidate sites for future projects of Very Large (“Megaton scale”) Laboratories Japan : YperKamioka site North America : Cascades-Icicle Creek, WA (USA) Henderson Mine, Empire, CO (USA) Homestake Mine, Lead, SD (USA) Kimballton Mine, Giles Co., VA (USA) San Jacinto, CA (USA) Soudan Mine, Soudan, MN (USA) SNOLAB, Sudbury, ONT (Canada) WIPP, Carlsbad, NM (USA) Europe : Fréjus tunnel (France/Italy) Poland site

(m 3 ) (mwe) Gran Sasso Super-K Sudbury II Fréjus-LSM Volume (m 3 ) vs Depth (mwe) for already existing laboratories Baksan Soudan II Canfranc II Pyhäsalmi I Homestake Boulby II

Volume (m 3 ) vs Depth (mwe) for 3 projects of future Labs ( the already existing Labs are also shown for comparison) Yper-KFréjus-Memphys UNO-Henderson (m 3 ) (mwe)

and HyperKamiokande

The CERN-Fréjus MEMPHYS Project

So, the challenge is now : to find out the best site(s) with : - relatively large depth - very large volume (megaton scale) - …….. - convenient position (long baseline) with respect to accelerator(s) and to be able to excavate and stabilize the cavities let us see with the talks of this session ….