in2p3 33 years

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FJPPL, May 17 th, 2008


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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

IN2P301


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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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in2p3 33 years

Documents

gsi future

nuclear mattertjnaf

future experimentsatlas

new agencies

new environment

nuclear stability heavy

new limits of stability

nuclear binding limits