1 / 37

LHC experiments starting with the p- pbar community in 1986

LHC experiments starting with the p- pbar community in 1986 . Observe the collisions. CMS. LHC Experiments. ATLAS, CMS: - Higgs boson(s) - SUSY particles - more dimensions? ALICE: Quark Gluon Plasma LHC-B: - CP violation in B. Example: Technologies’ watch . From CERN IT. RD20.

kirk
Download Presentation

LHC experiments starting with the p- pbar community in 1986

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. LHC experiments starting with the p-pbar community in 1986 Global collaboration Hans Hoffmann, CERN honorary

  2. Global collaboration Hans Hoffmann, CERN honorary

  3. Observe the collisions Global collaboration Hans Hoffmann, CERN honorary

  4. CMS Global collaboration Hans Hoffmann, CERN honorary

  5. LHC Experiments ATLAS, CMS: - Higgs boson(s) - SUSY particles - more dimensions? ALICE: Quark Gluon Plasma LHC-B: - CP violation in B Global collaboration Hans Hoffmann, CERN honorary

  6. Example: Technologies’ watch From CERN IT Global collaboration Hans Hoffmann, CERN honorary

  7. RD20 RDxx RD27 RD34 Design Phase Construction Phase Conception Phase RD3 RD6 Maximum use of everybody’s knowledge M&O MOU operation MOU 2003 MOU memorandum of understanding “construction” LOI letter of intent 1992 EAGLE ASCOT RDyy TP technical proposal 1994 RD13 TDRs technical design reports from 1996 Beam 2009 ATLAS only ExploitationPhase Global collaboration Hans Hoffmann, CERN honorary

  8. Collaboration Board (Chair: K. Jon-And Deputy: G. Herten) ATLAS Plenary Meeting Resources Review Board Spokesperson (F. Gianotti 2 Deputies) CB Chair Advisory Group ATLAS Organization January 2009 Technical Coordinator (M. Nessi) Resources Coordinator (M. Nordberg) Executive Board Inner Detector (L. Rossi) Tile Calorimeter (B. Stanek) Magnet System (H. ten Kate) Electronics Coordination (P. Farthouat) Trigger Coordination (N. Ellis) Data Prep. Coordination (C. Guyot) Additional Members (T. Kobayashi, M. Tuts, A. Zaitsev) LAr Calorimeter (I. Wingerter-Seez) Muon Instrumentation (L. Pontecorvo) Trigger/DAQ ( C. Bee, L. Mapelli) Commissioning/ Run Coordinator (T. Wengler) Computing Coordination (D. Barberis, D. Quarrie) Physics Coordination (D. Charlton) Global collaboration Hans Hoffmann, CERN honorary

  9. Last years’ ATLAS meetings CERN in everyday life H F Hoffmann CERN honorary

  10. “Virtual” international big science laboratory Funded, supervised by ~50 funding agencies • 37 Countries • 169 Institutions • 2800 Scientific Authors • (1850 with a PhD) • Technical persons • Thousands of industrial relations Global collaboration Hans Hoffmann, CERN honorary

  11. Number of scientists: 2100 Number of institutes: 167 Number of countries: 37 ATLAS (Spokesperson FabiolaGianotti) Global collaboration Hans Hoffmann, CERN honorary

  12. The ATLAS Cavern Global collaboration Hans Hoffmann, CERN honorary

  13. Global collaboration Hans Hoffmann, CERN honorary

  14. The ATLAS Cavern Global collaboration Hans Hoffmann, CERN honorary

  15. Assembly CMS Global collaboration Hans Hoffmann, CERN honorary

  16. ATLAS M.Nessi Global collaboration Hans Hoffmann, CERN honorary

  17. Global collaboration Hans Hoffmann, CERN honorary

  18. Tracker Trajectographe à silicium Des capteurs en silicium très finement segmentés (rubans et pixels) permettent de suivre la trajectoire des particules et de mesurer leur impulsion Comparable à un appareil photo à 70 millions de pixels prenant 40 millions de clichés par seconde! But: mesurer les trajectoires & l’ impulsion des particules chargées

  19. EM calorimeter 80 000 xtals, lead tungsten oxide, 80% metal: transparent

  20. Trigger and Dataflow Time 40 MHz 16 Million channels 3 Gigacell buffers Charge s Level 1 Pattern 100 kHz Read Out Buffers 200 Gigabytes ms Level 2 1000 Gigabit/s 1 kHz sec 100 Gigabit/s Level 3 100 Hz Permanent Storage 1 Petabyte/y Global collaboration Hans Hoffmann, CERN honorary

  21. Software structure/layers Applications are built on top of frameworks and implementing the required algorithms Applications Event DetDesc. Calib. expt. specific Every experiment has a framework for basic services and various specialized frameworks: event model, detector description, visualization, persistency, interactivity, simulation, calibration, etc. Experiment Framework Simulation DataMngmt. Distrib. Analysis Specialized domains that are common among the experiments ( some in grid middleware) Core Libraries common for expts. Core libraries and services that are widely used and provide basic functionality non-HEP specific software packages Many non-HEP libraries widely used GRID Middleware grids/networks “Software and Grids” OS & Net services Grid 2008; H F Hoffmann, CERN

  22. What to do with the data? @ @CERN in the Grid event filter (selection & reconstruction) Event Summary Data (ESD) processed data detector batch physics analysis raw data Analysis Object Data (AOD) (extracted by physics topic) event reconstruction event generation, simulation individual physics analysis Detector calibration alignment Global collaboration Hans Hoffmann, CERN honorary 22

  23. Balloon (30 Km) CD stack with 1 year LHC data! (~ 20 Km) Concorde (15 Km) Mt. Blanc (4.8 Km) July 2008 “Digital camera”, 150 M pixels, observing: 109 frames/s, recording selected frames: 200/s, ~1 GB/s recorded volume Global collaboration Hans Hoffmann, CERN honorary

  24. Computing GRID the size of the planet!

  25. International cooperation: Russian workers converting shells to CMS detector parts Global collaboration Hans Hoffmann, CERN honorary

  26. Contribution from Pakistan Structure CMS est constitué de plus de 10 000 tonnes d’acier – en comparaison la Tour Eiffel ne pèse “que” 7 000 tonnes! Ce “socle” a été réalisé au Pakistan et est arrivé au CERN par bateau, train et camion!

  27. CMS Global collaboration Hans Hoffmann, CERN honorary

  28. ALICE: an ultra-sensitive eye on the Universe: Quark-gluon plasma?

  29. 31 countries, 109 institutes, 1000 scientific/technical participants

  30. LHCb: an asymmetrical perspective

  31. What is the Grid? The World Wide Web provides seamless access to information that is stored in many millions of different geographical locations In contrast, the Grid is an emerging infrastructure that provides seamless access to computing power, software and data; distributed over the globe enabling CERN users to work from home as if at CERN CERN in everyday life H F Hoffmann CERN honorary

  32. Marek Domaracky CERN in everyday life H F Hoffmann CERN honorary

  33. Provide equal access to the data, software, compute power. . to all participating scientists “e-Science is about more than networks, Grids, High Performance Computing...; e-science is about global collaboration in key areas of science and the next generation of infrastructure that will enable it.”John Taylor, Director Research Councils, UK, 2000 CERN in everyday life H F Hoffmann CERN honorary

  34. e-science infrastructure ingredients people & VOs skills & training computers (HPC; HTC); computer aided services e-libraries archive/curation centres Multidisciplinary Collaborations: Common objectives Open sharing Critical mass Trust and respect >Best efforts Quality Assurance Service-oriented interoperable open software large data repositories; data services communication means facilities, instruments, services networks, services, dark λ CERN in everyday life H F Hoffmann CERN honorary

  35. Global collaboration Hans Hoffmann, CERN honorary

  36. Black hole of 3.5 10 6 solar masses Distance to Centre Galaxy 28 000 light years

  37. Ismail Serageldin

More Related