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14 000 Researchers12 000 Engineers, Technicians,
Administrative in 1300 lab
IN2P3 INSU SPM STIC SPI SC SDV SHS
NuclearParticle
Universe PhysicsMaths
Computing EngineerChemistry
Bio.
Humanities
Personnel:
1931 2671 2833 1317 1409 3496 5748 3969
Budget: 2,2 G€
CNRS
MPPU ST2I
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CNRS Priorities • Life Sciences
• Computer sciences
• Nanotechnologies
• Environment
• Interdisciplinarity
CNRS
A new strategic plan in preparationBut also new environment for research in France (as in UK, Italy,…)
•New agencies: ANR, A2I
•New campus-like structures: RTRA, PRES
•New status for universities
•New network like structures: Carnot Institutes
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18 laboratories800 recherchers (CNRS + Universities)1600 ITA/IATOS 60 projects
Interdisciplinary applicationsNuclear EnergyBiomedicalCondensed matter...
Basic Rechearch Nuclear PhysicsParticle PhysicsAstroparticle Physics
InstrumentationDetectors, Accelerators,Computing
Theory
IN2P3 conducts pp and np for the entire french academic world (except CEA)
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Particle Physics Computing
Nuclear Physics Astroparticle Physics Nuclear Energy
Applications Accelerators
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IN2P3/CNRS: 20 labs
BUDGET170 MŪ
57%11%
26,5%
2% 3,5%
CNRS Staff + UniversityInvestment + running CNRS + UniversityOthers ressources
STAFF2500
13%
17,5%
4,5% 3,5%
61,5%
CNRS Researchers University ResearchersCNRS Technical Staff None permanentsUniversity Technical
CNRSCNRS
Uni.
Uni.
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International Collaborations
Bilateral agreements with: Spain, Tchec. Republic, Poland, Romania, GSI, DubnaNikhef, US, Japan, China, Corea
Regular meetings with: DOE, KEK, INFN, PPARC, EPSRC, BMBF, NIKHEF
Collaborations with many other countries… NuPECC, APPEC
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Particle Physics at IN2P3 200 Physicists/10 Laboratories
Ongoing ExperimentsBaBar (30/4)D0 (30/7)H1 (15/3)Near Future ExperimentsATLAS (60/6)CMS (30/4)LHCb (20/4)LCG Far Future ExperimentsILC (15/5)CLIC (4/2)
Date of completion≤ 2009≤ 2008≤ 2007Date of readiness 2008 2008 2008≤ 2009
2025?
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Research AimsOngoing ExperimentsBaBar SLAC USD0 FNAL USH1 DESY DNear Future Experiments
LHC CERNATLAS CERNCMS CERNLHCb CERNLCG ccin2p3Far Future ExperimentsILC, CLIC WHERE?
Preparation to LHC PhysicsHiggs and new PhysicsCP ViolationProton Structure Tier 1 and 2 for LHCR&D for ILC and CLIC
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Quarks and gluons17%
Hadronic physics9%
Nuclear Structure, dynamics
39%
Nuclear Energy19%
Theory16%
NUCLEAR PHYSICS290 permanent scientists
221 physicists (experimentalists), 46 theorists, 23 radiochemists, 10 laboratories
ALICE, RHIC
GANIL, Orsay (ALTO), GSI,LEGNARO, JYVASKYLA, ISOLDE, DUBNA
TJLAB (G0, DVCS)GSI (HADES)
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TPCTPC
PHOSPHOS
Muon armMuon arm
TOFTOFTRDTRDHMPIDHMPID
PMDPMD
ITSITS
ALICE (CERN)IN2P3 5 laboratories - Dimuon arm - Internal tracking system (ITS) Investment: 6.6 M€
Nature of the confinement of quarks and gluons
Hadronic physics
Understand the structure of nucleons and light nucleiConfinement of quarks et gluons in hadronsStrong interaction (QCD)Structure modifications of hadrons in nuclear matterTJNAF, GSI
HADES
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Some key facts:New limits of stability (37Ne) Discovery of 48Ni 2p radioactivityNew deformations, New magicityNuclear moleculesNew detectors (EXOGAM, VAMOS)
R&D for SPIRAL2: ALTO (agreementDUBNA-IPNO)R&D future detectors: AGATA
- Origin of nuclear binding- Limits of nuclear stability- Heavy and super-heavy elements
- Formation of elements in the universe (nucléosynthesis)
SPIRALCAEN
Structure and the dynamics of nuclei. Nature of the nucleonic matter
KEEP THE INTERNATIONAL COMPETITIVITY OF GANIL KEEP THE INTERNATIONAL COMPETITIVITY OF GANIL SPIRAL2 projectSPIRAL2 project- 2002-2008 experiments with SPIRAL I- 2002-2008 experiments with SPIRAL I SPIRAL II , a priority stated by NuPECC SPIRAL II , a priority stated by NuPECC 118M€ (full cost) - cofinanced by Region (33%) 118M€ (full cost) - cofinanced by Region (33%) Decision expected end-2004- into operation: 2009Decision expected end-2004- into operation: 2009-Complementarity with GSI - Future with EURISOL…Complementarity with GSI - Future with EURISOL…
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SPIRAL II project SPIRAL II project
Driver SC Linac: 40MeV, 5mA d Driver SC Linac: 40MeV, 5mA d et 14.5 AMeV, 1pmA heavy-ionset 14.5 AMeV, 1pmA heavy-ions
d->n d->n 1212C converter + C converter + 238238UCUCxx target target
Post-acceleration in CIMEPost-acceleration in CIMEEnergy < 6 AMeVEnergy < 6 AMeV
>1013 fissions/sec.
•Multi-beams (up to 5)•Into operation: 2009
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Pluridisciplinary Program PACE Back-end of electronuclear cycle
IN2P3 focused on transmutation of nuclear wastes and innovative systems for the future of nuclear Energy - Experimental validation of Accelerator Driven Systems (ADS)
R&D European programs (MEGAPIE, n-TOF, MUSE, PDS-XADS, EUROTRANS)- High intensity accelerator developments (IPHI)
Innovative systems for Nuclear Energy based on the Th cycle Scenarios, focused on the concept of a molten salt reactor
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SUPERNEMOR&D
NEMO3
Double betaNeutrino mass
T2K DOUBLE CHOOZ
OPERA
neutrinooscillation
Neutrino
PLANCKBRAIN
Cosmologicalparameters
SNAP 2015
SNIFSSNLS
DarkEnergy
EDELWEISS
DarkMatter
Cosmology
Current IN2P3 program
On Astroparticle, Cosmology and Neutrino
Astroparticle
High EnergyGamma Rays
NeutrinoTelescope
CosmicRays
Gravitationalwaves
HESSHESS II
GLAST ANTARES
KM3>2010
AUGERCODALEMA
AMSCREAM
VIRGOVIRGO+
advVIRGO
LISA2013-15
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ASTROPARTICLE PHYSICS & NEUTRINO200 researchers, 154 engineers, 70 non permanent staff
Engineers & techniciens
SUPERNOVA10%
EDELWEISS6%
NEMO - OPERA - DOUBLE CHOOZ
21%
PLANCK15%
VIRGO - LISA10%
AUGER-AMS15%
ANTARES11%
HESS - GLAST9%
AUTRES3%
Permanent researchers
NEMO - OPERA - DOUBLE CHOOZ
19%
EDELWEISS5% SUPERNOVA
11%
PLANCK7%
VIRGO - LISA9%
AUGER-AMS15%
ANTARES6%
HESS - GLAST13%
AUTRES15%
Space programs 25 %
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A « cosmic ray » program
HESS, Namibia, 2004 AUGER, Argentina, 2005
VIRGO, Pisa, 2006 ANTARES, Toulon, 2006
High energy gamma, ultra high energy cosmic rays, gravitational waves, neutrinos
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In the near futureCosmic rays and cosmology in space
GLAST, 2007 AMS 2009PLANCK, 2008
SNAP/JDEM 2015
SNIFS, SNLS
High energy gamma rays, antimatter, CMB, Dark Energy
LISA 2015
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LSM in Fréjus • NEMO3, double beta
decay (2003-)• EDELWEISS II, dark
matter (2006)• Low radioactivity studies
(ILIAS)• Search for SHE in nature
Laboratoire Souterrainde Modane, France
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Neutrino roadmap
• OPERA(2006)• In the next few years:
– DOUBLECHOOZ (2008-2009)– T2K (2009-2013)
• R&D for SuperNEMO, double beta decay (>2010)
• At the horizon of 2015-18– Megatonne detector in Fréjus in
relation to super and beta beam from CERN?
65m
80mMEMPHYS
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investissement et fonctionnement
0
500
1000
1500
2000
2500
3000
3500
4000
2005 2006 2007 2008 2009 2010
année
k€
LISA
DOUBLE-CHOOZ
T2K
EDELWEISS
OPERA
ANTARES
HESS
PLANCK
GLAST
Snae
SNAP
AUTRES
AMS
NEMO
AUGER
pourcentage des 3 secteurs
34%
52%
14%
neutrino
astrop
cosmo
Sources:
•AP
•TGE HESS
•Prgm Astrop
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Astroparticle missionsmissions
0
200
400
600
800
1000
1200
1400
1600
1800
2005 2006 2007 2008 2009 2010
année
k€
AUTRES
T2K
PLANCK
EDELWEISS
SNAP
LISA
AMS
DOUBLE-CHOOZ
ANTARES
NEMO
Snae
GLAST
AUGER
HESS
OPERA
34%
50%
16%
neutrino
astrop
cosmoSee talk by AM Ferrer and L. Mallet for Human Ressources
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Conclusions• The research environment in France is changing fast. • It abandons the model of « unique desk » agencies
providing autonomously all resources, hiring people, and managing their careers to « grant providing » agencies
• The IN2P3 concentrating on a project by project management structure hopes to keep its potential of large project funding, the concomitant pluri-annual character of engagements and the autonomy of its strategic thinking (in coordination with the other agencies in France, Europe and the world)
.
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