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

Slides:



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

J. Strait Fermilab October 21, 2005 The Neutrino Detector of the Future: A Massive Liquid Argon TPC.
Precision Neutrino Oscillation Measurements & the Neutrino Factory Scoping Study for a Future Accelerator Neutrino Complex – Discussion Meeting Steve Geer,
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.
European Strategy for Particle Physics 2013 Preparatory group->Strategy group Individual town meetings Town meeting in Krakow: september 2012 Drafting.
Accelerator based Neutrino program around the world 1. Europe: Neutrino platform at CERN ESS second maximum? 2. Japan: T2K and HyperK status 3. USA: LBNF.
ISS-2 25 jan KEK Alain Blondel Physics of Future Neutrino Detectors PoF-NuDet detectors and beam instrumentation time scales and cost estimates.
ECFA-EPS Joint Session Imperial College/RAL Dave Wark Neutrino Physics – Accomplishments and Future Challenges Dave Wark Imperial/RAL (but speaking only.
Michel Spiro Particle Physics at the Megawatt proton source. CERN 27 May 2004 Long-range programme in neutrino physics: superbeam, β beam, neutrino factory.
Alain Blondel CHIPP Neutrino meeting NEUCHATEL June 2004.
25/10/2007M. Dracos1 EURO The European Design Study for a high intensity neutrino oscillation facility (Rob Edgecock, Mats Lindroos, Marcos Dracos)
Neutrino physics: experiments and infrastructure Anselmo Cervera Villanueva Université de Genève Orsay, 31/01/06.
F Future of Neutrino Program at FNAL NuMI Off-Axis Meeting Hugh Montgomery January 12, 2004.
Reactor & Accelerator Thanks to Bob McKeown for many of the slides.
How Will We See Leptonic CP Violation? D. Casper University of California, Irvine.
Alain Blondel Detectors UNO (400kton Water Cherenkov) Liquid Ar TPC (~100kton)
Summary of Nufact-03 Alain Blondel NuFact 03 5th International Workshop on Neutrino Factories & Superbeams Columbia University, New York 5-11 June 2003.
Summary of Nufact-03 Alain Blondel NuFact 03 5th International Workshop on Neutrino Factories & Superbeams Columbia University, New York 5-11 June 2003.
Jacques Bouchez CEA/DAPNIA-Saclay & APC-Paris ISS meeting, detector WG KEK, Jan23 rd, 2006 MEMPHYS : A megaton WČ detector in Fréjus underground laboratory.
T2K experiment at J-PARC Epiphany 2010D. Kiełczewska1 For T2K Collaboration Danuta Kiełczewska Warsaw University & Sołtan Institute for Nuclear Studies.
NEUTRINO PROPERTIES J.Bouchez CEA-Saclay Eurisol town meeting Orsay, 13/5/2003.
Summary of WG1 – Phenomenological issues Osamu Yasuda (TMU)
1 V. Antonelli, G. Battistoni, P. Ferrario 1, S. Forte (Università degli Studi di Milano e I.N.F.N. Sezione di Milano and 1 University of Valencia) Standard.
Alain Blondel CHIPP Neutrino meeting NEUCHATEL June 2004 Aims of the meeting At least four universities in Switzerland do research in Neutrino Physics.
L. MoscaEPIPHANY Conf 6-8 Jan EPIPHANY Conference at Cracow “Physics in Underground Laboratories and its connection with LHC” - 6 to 8 January 2010.
A neutrino program based on the machine upgrades of the LHC Pasquale Migliozzi INFN – Napoli A. Donini, E. Fernandez Martinez, P.M., S. Rigolin, L. Scotto.
ESS based neutrino Super Beam for CP Violation discovery Marcos DRACOS IPHC-IN2P3/CNRS Strasbourg 1 20 August 2013M. Dracos.
Long Baseline Experiments at Fermilab Maury Goodman.
Chang Kee Jung August 2007, LP07 Planning the Future Neutrino Projects in Global Context: Ideas, Challenges, and Limitations Planning the Future Neutrino.
Fermilab Neutrino Program Jim Strait Neutrino Discussion at CERN 26 November 2013.
Road Map of Future Neutrino Physics A personal view Ken Peach Round Table discussion at the 6 th NuFACT Workshop Osaka, Japan 26 th July – 1 st August.
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.
If  13 is large, then what ? Hisakazu Minakata Tokyo Metropolitan University.
R.G. 7/09/20101 Options for neutrinos. R.G. 7/09/20102 Conventional beam from the SPS (1/3) Neutrinos using the SPS Nominal CNGS 732 km baseline from.
Neutrino Physics Opportunities for Fermilab Steering Group 6/12/07 Andy Lankford UC Irvine.
J. Bouchez CEA/DAPNIA CHIPP Neuchâtel June 21, 2004 A NEW UNDERGROUND LABORATORY AT FREJUS Motivations and prospects.
John Womersley Welcome Director of Particle Physics, CCLRC International Scoping Study Meeting, RAL April 2006.
Pre-  Factory Possibilities Leslie Camilleri CERN, PH Scoping Study Meeting Imperial College May 6, 2005.
NEUTRINO DETECTORS Cutting-Edge Accelerator Research for a Neutrino Factory and Other Applications Ajit Kurup for the FETS and UKNF Collaborations Cutting-Edge.
Super Beams, Beta Beams and Neutrino Factories (a dangerous trip to Terra Incognita) J.J. Gómez-Cadenas IFIC/U. Valencia Original results presented in.
Summary of Nufact-03 Alain Blondel NuFact 03 5th International Workshop on Neutrino Factories & Superbeams Columbia University, New York 5-11 June 2003.
ESS based neutrino Super Beam for CP Violation discovery Marcos DRACOS IPHC-IN2P3/CNRS Strasbourg 1 10 September 2013M. Dracos.
Alain Blondel -- After the ISS -- What did ISS achieve? 1. Established a « baseline » for the accelerator study 2. Rejuvenated simulation and study of.
NUFACT’06 Summary of working group 1 Neutrino Oscillations Experiments Mark Messier Indiana University August 30, 2006.
CERN, 15/03/05EURISOL - Beta Beam Task1 EURISOL and the Beta-Beam Task Status and Planning Michael Benedikt Mats Lindroos AB-Department, CERN.
SPL, Beta beams and the Neutrino Factory. Leslie Camilleri NuSAG 20th May 2006.
Status and Plans for EUROnu FP7 Design Study Status and Plans for EUROnu FP7 Design Study EUROnu = A High Intensity Neutrino Oscillation Facility in Europe.
John Womersley 1/13 Fermilab’s Future John Womersley Fermilab May 2004.
Accelerator-based Long-Baseline Neutrino Oscillation Experiments Kam-Biu Luk University of California, Berkeley and Lawrence Berkeley National Laboratory.
1 Neutrino detector test beam requirements 0. Disclaimer 1. News from the neutrino scene 2. Beam requirements for AIDA and others.
2 July 2002 S. Kahn BNL Homestake Long Baseline1 A Super-Neutrino Beam from BNL to Homestake Steve Kahn For the BNL-Homestake Collaboration Presented at.
Future neutrino oscillation experiments J.J. Gómez-Cadenas U. Valencia/KEK Original results presented in this talk based on work done in collaboration.
Jose Bernabeu U. Valencia and IFIC XIII International Workshop on Neutrino Telescopes March 2009 CP Violation in Neutrino Oscillations without Antineutrinos:
Energy Dependence and Physics Reach in regard to Beta/EC Beams J. Bernabeu U. Valencia and IFIC B. Pontecorvo School September 2007.
A monochromatic neutrino beam for  13 and  J. Bernabeu U. de Valencia and IFIC NO-VE III International Workshop on: "NEUTRINO OSCILLATIONS IN VENICE"
EU accelerator contributions to the IDS … R. Garoby ISS meeting RAL 28/04/2006.
EURO EURO A High Intensity Neutrino Oscillation Facility in Europe Introduction Aims Structure Tasks Link to other activities Future dates.
Jacques Bouchez Radioactive Beams for Nuclear and Neutrino Physics Les Arcs Mars 2003.
A CCELERATOR S ESSIONS S UMMARY D AVE W ARK, I LIAS E FTHYMIOPOULOS Neutrino Strategy Workshop CERN, October 3, 2009 Outline  Show highlights from the.
PPAP Review 09 Imperial College/RAL Dave Wark Future Neutrino Oscillation Experiments Dave Wark Imperial/RAL PPAP Birmingham July 15 th, 2009.
Beta beams Jacques Bouchez CEA Salay/ APC Paris Basics of beta beams The baseline CERN scenario Higher energy beta beams Other ideas Conclusions POFPA.
CARESG, 11Apr2006V. Palladino Report on BENE Activities Beams for European Neutrino Experiments (BENE) subtitle: A Network aiming at a consensual road.
ICARUS-LBNE project A. Guglielmi 1.LBNE-ICARUS Padova meeting 2.SPS-C C. Rubbia presentation.
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.
Marcos DRACOS IPHC-IN2P3/CNRS Université de Strasbourg
LAGUNA and beyond GDR Neutrino at Orsay-PNO October 11th, 2010
IPHC-IN2P3/CNRS Strasbourg
Alain Blondel 11 October 2010 GDR NEU2012 summary
W. T. Weng Brookhaven National Laboratory
Fermilab Proton Beams: Program Perspectives Greg Bock Fermilab Science and Engineering at Henderson-DUSEL Capstone Workshop Stony Brook May 5,
Presentation transcript:

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

PROTON DRIVER FOR CERN NEUTRINO FACTORY

Frejus lab is 130 km away from CERN ! E  = 270 MeV => baseline 135 km

A SAFETY GALLERY TO BE BUILT ALONG THE EXISTING TUNNEL

PROPOSAL FOR A NEW UNDERGROUND LAB AT FREJUS Excavation of safety gallery completed around 2009 when machines meet at the center. Excellent opportunity to dig a new cavity at reduced cost in the middle of the tunnel, which could be ready by 2012 and house a detector for the neutrino superbeam Horizontal access, rock quality known and good (and no water!) Schedule of such a detector comes much after T2K phase 1 and NuMI off-axis (now NOVA). So, directly propose a detector able to see CP violation => Megaton Cerenkov detector (or liquid Ar) First studies based on a UNO-like detector show excellent sensitivity to θ 13 and δ CP, similar to T2K phase 2 (4 MW + HK) Project favourably considered by our scientific authorities, with a strong support from local authorities

MORE RECENT DEVELOPMENTS A new idea (P.Zucchelli): Beta beams, produced by radioactive ions stored in a decay ring, give a novel way to produce e and anti- e beams of very high purity, perfectly known spectrum and intensity. The required ion energy is achievable with the SPS ! (see M.Lindroos’talk tomorrow) The combination of beta beams and superbeams gives unique redundancy (CP,T,CPT in different ways), and a direct handle on how the detector sees the signal in each beam (as it is the bulk of events seen with the other beam) The superbeam has been further optimized (higher energy, higher intensity) see M.Mezzetto’s talk tomorrow on the remarkable performances of Beta beams + superbeams. Beta beams profit from a strong synergy with nuclear physicists using radioactive ions produced by the ISOL technique: Neutrino beta beams are now part of the design study funded by Europe on the EURISOL facility.

EXCLUDED BY CHOOZ Θ 13 degrees YEAR Minos, Icarus, Opera Double Chooz T2K1, NovA SB  B T2K 2

SCHEDULE Super and beta beams will hopefully be ready before 2020…. ….BUT We do not have to wait for them to build a detector, as non- accelerator physics is at least as rich as neutrino beam physics: proton decay, with some chance of discovery SN explosion ( for SN mechanism AND neutrino oscillations) So, our preferred strategy is: 1.Build a cavity and a detector, taking benefit of the safety gallery 2.Start non-accelerator physics right away 3.Begin neutrino oscillation study as soon as beams are available

A possibly optimistic schedule for a european lab. at Frejus Year Safety tunnel Excavation Lab cavity Excavation P.S Study detector PM R&DPMT production Det.preparation InstallationOutside lab. Non-acc.physics P-decay, SN Superbeam ConstructionSuperbeam betabeam ???????? Beta beam Several modules: physics can start when the 1 st is ready

.

Perlite insulation  ≈70 m h =20 m Electronic crates 100 kt liquid argon (see A. Rubbia’s talk)

FROM DREAM TO REALITY 1.A prestudy on the feasibility of the cavity has been launched: It will address maximal dimensions, preferred topology, cost… (both for Cerenkov and LAr): first results (very preliminary) will be presented by M.Levy on Saturday morning 2. Funding for a more detailed study will be requested to Europe in 2007 (next call) 3. R&D on photodetection is mandatory, a collaboration with Photonis has started. Other ideas on low cost large area photodetection (micromegas) are also considered. 4. We are looking forward to a closer inter-regional (north- America, Japan, Europe) cooperation, demonstrating a strong and converging interest on this very fundamental and promising field of physics

The end … of the prologue