______________________________________________ Etienne Augé Directeur Adjoint Scientifique Recent projects at CNRS/IN2P3

______________________________________________ IN2P3/CNRS 10 Institutes

______________________________________________ CNRS Budget: 3,1 billions Euros –Salaries: 2,2 billions Euros (70%) permanent staff – researchers – Engineers, Technicians 8900 CDD, docts/post-docs 1053 research units 96 service units IN2P3 Since 1971 Budget : 164 millions Euros (5%) –Salaries: 118 millions Euros (70%) 1896 permanent staff – 525 researchers (5%) –1371 Engineers, Tech (10%) 396 professors and assistant-prof 217 Engineers, Tech (university staff) 700 CDD, docs, post-docs 20 Laboratories (2%) –Computer Center CC-IN2P3 (Lyon) –GANIL (Caen) –LSM (Modane ) IN2P3/CNRS IN2P3 budget reduced by 15 % in 2012 … both project and labs support

______________________________________________ IN2P3 activities Nuclear physics Particle physicsAstroparticle Computing/grid Health Nuclear energy Accelerator - Nuclear structure, far from stability - Radioactive beams  Construction is progressing - AGATA gamma detector - Accelerator Driven System  High current, very stable proton linac - Nuclear Waste Management (including radio-chemistry) - New scenarios (Thorium-Lead)

______________________________________________ Accelerators -XFEL cavities/couplers : benchmark for a LC ? -Linac 4 -Nanobeams / B factories -SPIRAL-2 at GANIL -High intensity proton accelerators (SPL, ESS…) -Laser-plasma acceleration TYL Workshop - Clermont-Ferrand, June 29th 2012

______________________________________________ From particle physics to applications Biological science : Particle detector (SiPM, pixel) and microelectronics Computing : G4 simulation (GATE), image reconstruction, grid Accelerator : hadrontherapy, ThomX… Environment science : CMOS camera for submarine life study Particle detector for vulcanology Detector applications also in photon science, grid for chemistry….

______________________________________________ Puy de Dôme seen by atmospheric muons TYL Workshop - Clermont-Ferrand, June 29th 2012

______________________________________________ 8 What is Universe made of ? The PLANCK satellite,launched in 2009 eagerly waiting the most precise map of the fluctuations of the CMB, to measure inflation. SNLS, SDSS-III,through the measurement of distant supernova, determine the parameters of the equation of state for the dark energy with the highest precision in the world EDELWEIS-II statistical significance equal to the two other leading experiments (CDMS/XENON)

______________________________________________ Universe at High Energy FERMI (since 2008) and HESS (since 2004) have multiplied by 10 the number of detected violent sources at GeV and at TeV scales. They have demonstrated the existence of cosmic accelerators, approaching the résolution de l’enigma of the origin of cosmic rays AUGER (in 2008) has demonstrated the existence of a cut in the energy spectrum of CR at HE, and their anisotropy Virgo since 2008 at the best sensitivity level in the world ANTARES the largest sensitivity for observing the southern hemisphere (since 2008). The largest infrastructure in the world in the very deep sea

______________________________________________ A sustained spatial program FERMI, 2008 PLANCK, 2009 LISA around 2020 JDEM/EUCLID around 2020 AMS 2010 LISAPATHFINDER 2012 JEM-EUSO 2015

______________________________________________ LSST, dark energy The next génération ( ) CTA : HE photons EURECA : dark matter SUPERNEMO v-less double beta decay AUGER extension advVIRGO Gravitational Waves KM3NET Neutrinos HE

______________________________________________ Particle physics (I) Most of the projects common to IN2P3 and IRFU within strong international collaborations. LHC (~350 permanent research staff) ATLAS, CMS and ALICE (IN2P3 + IRFU) LHCb (IN2P3)  Strong contribution to construction and data analysis (Higgs, top,…)  R&D for phase-I upgrade

______________________________________________ Particle physics (II) Finishing analysis in DZero (Higgs, top, W mass), BaBar and H1 Contribution to neutron electrical dipolar moment (nEDM at PSI, IN2P3) and antimatter gravitity at CERN (Aegis/IN2P3 and Gbar/IRFU) being discussed Neutrinos : Opera (IN2P3) : tau neutrino appearance… data taking in 2012 Double Chooz and T2K (IN2P3 + IRFU) : sin(  13 )… near detector : neutrinoless double beta decay first prototype next year ? new cavern ?

______________________________________________ Particle physics (III) Detectors developments for a future Linear collider (LC) -Calorimeters (IN2P3) -Pixel and CMOS detectors (IN2P3+IRFU) -Microelectronics (IN2P3+IRFU) -Micro-pattern gas detectors (IN2P3+IRFU) Computing : T1 + 8 T2 for LHC Important effort to develop an academic cloud infrastructure More general effort on “Big Data”

______________________________________________ ongoing prospective (I) First priority is the LHC : data taking + analysis + phase I upgrade (IN2P3 scientific council in June 2012 to define contributions). High lumi (>2022) or High energy for LHC was discussed and strongly depends on new physics observed or not in 13 TeV running Linear collider (LC): Quite some discussions about a “Fast-Track LC (in Japan)” starting at 230 GeV (if Higgs discovered at LHC at 125 GeV !) and upgradable at 500 GeV) or a higher energy (longer term) few-TeV project.  Consensus seems to appear to participate and push for such a Fast- Track LC project : use Higgs discovery opportunity to convince ministry  LC town Hall meeting of May 16 th at Paris (ECFA/LC input to European Strategy Group)

______________________________________________ ongoing prospective (II) Precision measurement experiments (nEDM, Aegis, Gbar, Super B) : - Neither clear nor strong conclusion - Small community…. Neutrinos : Interest to participate to a long baseline neutrino project in Europe A strategic vision has here to be set : - might need to choose between long baseline or neutrinoless project… -LSM host lab for new generation neutrino experiment (CP violation) or dark matter detector ?  LSM extension

______________________________________________ European Strategy European Strategy Group (ESG): 46 1 representative for each of the 20 member states 1 representative for each of the 5 observer states 1 representative for each of the 2 associate states The director of the 9 major european laboratories The CERN DG + 4 members of the strategy secretariat 5 invited (EU, FALC, ESFRI, ApPEC, NuPECC) Preparatory Group: 16 4 members of the strategy secretariat 4 SPC members 4 ECFA members 3 representatives (CERN, America, Asia) 1 scientific assistant TYL Workshop - Clermont-Ferrand, June 29th 2012

______________________________________________ European Strategy (continued) Town meeting in Kracow –September –Submissions open until july 31st Drafting meeting in Erice –January –Submissions open until october 15th Presentation at the CERN council: march 2013 Special council session in Brussels: may/june 2013 TYL Workshop - Clermont-Ferrand, June 29th 2012

______________________________________________ Investment for the Future Equipements of excellence (max 20 M€) –Thom-X, CILEX, S3, DESIR, Andromède, Arronax+ Laboratories of excellence –Forming consortiums of few laboratories –Budget for temporary positions + small projects Initiatives of excellence 9 big clusters (research universities) 500 – 1000 M€ each (mostly capital money) TYL Workshop - Clermont-Ferrand, June 29th 2012

______________________________________________ Conclusion Many appealing scientific projects some very large, some of smaller size Future must be prepared now 2012 is a year for prospective at the French level at the European level Some important instability in the institution specific financial effort (driven by international jury) large scientific infrastructures decrease in the budget distributed by IN2P3 International partnerships are an important asset for IN2P3