1 / 20

Etienne Augé Directeur Adjoint Scientifique

Etienne Augé Directeur Adjoint Scientifique. Recent projects at CNRS/IN2P3. www.in2p3.fr. IN2P3/CNRS. 10 Institutes. IN2P3/CNRS. CNRS Budget: 3,1 billions Euros Salaries: 2,2 billions Euros (70%) 25 630 permanent staff 11 450 researchers 14 180 Engineers, Technicians

xiu
Download Presentation

Etienne Augé Directeur Adjoint Scientifique

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. Etienne AugéDirecteur Adjoint Scientifique Recentprojectsat CNRS/IN2P3 www.in2p3.fr

  2. IN2P3/CNRS 10 Institutes

  3. IN2P3/CNRS • CNRS • Budget: 3,1 billions Euros • Salaries: 2,2 billions Euros • (70%) • 25 630 permanent staff • 11 450 researchers • 14 180 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 budget reduced by 15 % in 2012 … both project and labs support

  4. IN2P3 activities - Nuclear structure, far fromstability - Radioactive beams SPIRAL-2@GANIL Construction isprogressing - AGATA gamma detector Particle physics Astroparticle Nuclear physics • - Accelerator Driven System • High current, very stable proton linac • - NuclearWaste Management • (including radio-chemistry) • - New scenarios (Thorium-Lead) Accelerator Nuclear energy Health Computing/grid

  5. Accelerators • XFEL cavities/couplers : benchmark for a LC ? • Linac4 • Nanobeams / B factories • SPIRAL-2 at GANIL • High intensity proton accelerators (SPL, ESS…) • Laser-plasma acceleration TYL Workshop - Clermont-Ferrand, June 29th 2012

  6. 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….

  7. Puy de Dômeseen by atmospheric muons TYL Workshop - Clermont-Ferrand, June 29th 2012

  8. What is Universe made of ? The PLANCKsatellite,launched in 2009 eagerlywaitingthe mostprecisemap of the fluctuations of the CMB, to measure inflation. SNLS, SDSS-III,through the measurement of distant supernova,determinethe parameters of the equation of state for the darkenergywith the highestprecision in the world EDELWEIS-II statisticalsignificanceequal to the twootherleadingexperiments (CDMS/XENON)

  9. Universeat High Energy FERMI (since 2008) and HESS (since 2004) have multipliedby 10 the numberof detectedviolent sources atGeV and atTeVscales. They have demonstratedthe existence of cosmicaccelerators, approaching the résolution de l’enigma of the origin of cosmic rays AUGER (in 2008) has demonstrated the existence of a cut in the energyspectrum of CR at HE, and theiranisotropy Virgosince 2008 at the best sensitivitylevel in the world ANTARESthe largestsensitivity for observing the southernhemisphere (since 2008). The largest infrastructure in the world in the verydeepsea

  10. A sustained spatial program FERMI, 2008 JDEM/EUCLIDaround2020 LISAPATHFINDER2012 PLANCK, 2009 JEM-EUSO 2015 AMS 2010 LISA around 2020

  11. The next génération (2010-2020) CTA : HE photons KM3NET Neutrinos HE LSST, dark energy AUGER extension EURECA : dark matter advVIRGO Gravitational Waves SUPERNEMO v-less double beta decay

  12. 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 (I)

  13. 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 SuperNemo@LSM : neutrinoless double beta decay first prototype next year ? new cavern ? Particle physics (II)

  14. 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) Particle physics (III) Computing : CC-IN2P3 @Lyon Grid: T1 + 8 T2 for LHC Important effort to develop an academic cloud infrastructure More general effort on “Big Data”

  15. 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 16th at Paris (ECFA/LC input to European Strategy Group) ongoing prospective (I)

  16. 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 ongoing prospective (II)

  17. EuropeanStrategy • EuropeanStrategy 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 europeanlaboratories • The CERN DG + 4 members of the strategysecretariat • 5 invited (EU, FALC, ESFRI, ApPEC, NuPECC) • Preparatory Group: 16 • 4 members of the strategysecretariat • 4 SPC members • 4 ECFA members • 3 representatives (CERN, America, Asia) • 1 scientific assistant TYL Workshop - Clermont-Ferrand, June 29th 2012

  18. EuropeanStrategy (continued) • Town meeting in Kracow • September 10-12 • Submissions open untiljuly 31st • Drafting meeting in Erice • January 21-26 • Submissions open untiloctober 15th • Presentationat the CERN council: march 2013 • Specialcouncil session in Brussels: may/june 2013 TYL Workshop - Clermont-Ferrand, June 29th 2012

  19. 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 + smallprojects • Initiatives of excellence • 9 big clusters (researchuniversities) • 500 – 1000 M€ each (mostly capital money) TYL Workshop - Clermont-Ferrand, June 29th 2012

  20. Conclusion Manyappealingscientificprojects somevery large, some of smaller size Future must bepreparednow 2012 is a year for prospective at the French level at the Europeanlevel Some important instability in the institution specificfinancial effort (driven by international jury) large scientific infrastructures decrease in the budget distributed by IN2P3 International partnerships are an important asset for IN2P3

More Related