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U.Gasparini10/04/031 Toward Physics TDR Barrel Muon week, Bologna, 9-12 April 2003 - CCS (Computing&Core Software) schedule 2003-2005 - Computing TDR (due.

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Presentation on theme: "U.Gasparini10/04/031 Toward Physics TDR Barrel Muon week, Bologna, 9-12 April 2003 - CCS (Computing&Core Software) schedule 2003-2005 - Computing TDR (due."— Presentation transcript:

1 U.Gasparini10/04/031 Toward Physics TDR Barrel Muon week, Bologna, 9-12 April 2003 - CCS (Computing&Core Software) schedule 2003-2005 - Computing TDR (due 2004) - Physics TDR (2005) - Post-DAQ TDR activity -‘Data challenges’ - Analysis groups and Physics TDR

2 U.Gasparini10/04/032 2003 –JuneSwitch from CMSIM to OSCAR –JulyStart full-scale 5 month production of GEANT4 events –SeptBaseline software for DC04 / C-TDR / Physics TDR 2004 –AprilDC04 complete –AprilFirst Draft C-TDR –OctComputing-TDR Submission 2005 –AprilDC05 complete (LCG-3 validation) –DecPhysics-TDR Submission 2006 –AprilDC06 complete (ready for real data) CCS schedule “data challenges”

3 U.Gasparini10/04/033 CCS schedule (detailed 2003-2004) CMSIM OSCAR development of first “full off-line” analyses (i.e. beyond HLT) on predefined benchmark channels

4 U.Gasparini10/04/034 Post DAQ TDR activity After completion of DAQ TDR (Dec.2002), main emphasis this year will be on: - switch to GEANT4 simulation, reproducing/improving in OSCAR+ORCA (full C++) chain the known HLT results from CMSIM + ORCA - by- products: - new Detector Description Database (DDD) system - refine sub-detectors geometries (when needed) [ e.g. for BMU: - insert proper staging between  SL - insert chimneys - include “+ve” “-ve” chamber readout ] - have consistent ORCA code between MC and TestBeam data analysis environment MB2.2.4 (courtesy of M.Benettoni)

5 U.Gasparini10/04/035 Post DAQ TDR activity -develop first full off-line analyses down to O(10 -5 -10 -7 ) Hz rate on few relevant benchmark signals - significant training/test of the software + computing system HLT outpupt, di-mu stream (  3 Hz) Low lumi (DAQ TDR, ch.15) H  WW  2  2 (see M.Zanetti’s talk)

6 6 Post DAQ TDR activity Current choises for full analyses within PRS/mu: - H  ZZ*  4   2-mu topologies:  - H  WW  2  (=> - challenging for background rejection;  - hot channel in the early days of LHC )  - Z ’  2  in the 1-2 TeV region (=> - challenging for p T resolution;  - impact of alignment;  - showering muons....)  These will likely to go in the “Volume 1” of the Physics TDR  (=> devoted to detector response, reconstruction of physics objects,  calibrations, detector parameterization), under responsability of PRS groups  => benchmark for any “fast/parametrized” simulation/reconstruction  “Volume 2”: High-level analyses, like Higgs, Supersymmetry, Exotic physics, etc.  => “physics reach”of CMS, scan of models’ parameters space....  (responsability of new analyses groups) next slide...

7 U.Gasparini10/04/037 SM Higgs searches Compare Tevatron: H  WW  2l  H  ZZ*  4l Run II A Luminosity They are here 140 GeV

8 U.Gasparini10/04/038 “Data challenge” preparation In Febr.’04, CMS will perform its first significant “Data Challenge” (DC04) i.e. large scale test of computing and analysis model: Inject into the system a “sustained data-taking rate of 25 Hz at luminosity 2 10 33 for 1 month” ( =>50 10 7 events), filter and analize them down to “physics plots” (+ calibration/alignment activity...)  prepare 50 M ev datasample (=> pre-data challange phase, MC production 10 times larger than for DAQ TDR; huge effort, GEANT4 training on big MC simulation (timing, crashes,...), Grid training, ect...): it will last 6 months, 2nd half of 2003  finalize HLT code for “Tier0” operations (50 M ev will be at HLT output)  use the 50 M ev for preliminary Physics TDR analysis (this will last presumably all 2004, after the DC04 itself) see Silvia’s talk for PRS/mu details

9 U.Gasparini10/04/039 Analisys groups New “analysis groups”: 1. Heavy Ions Bolek Wyslouch (MIT) 2. Higgs Sasha Nikitenko (IC) 3. Standard Model Joachim Mnich (Aachen) 4. SUSY/other Beyond the SM Luc Pape (CERN) Convenor First meetings during next CPT week (5-9 May) New CPT week layout to allocate time for the new groups

10 U.Gasparini10/04/0310 New CPT layout: Start Time Monday Tuesday Wednesday Thursday Friday 8.30 Tracker Muons b/tau CPT Plenary CPT Plenary Break Break Session 1 Session 3 10.30 Higgs SUSY and Beyond SM 14:00 ECAL HCAL PRS Steering e/gamma JetMET Committee CPT Plenary CPT Plenary Break Break Break Session 2 Session 4 16:30 Standard Heavy Ions CPT JTB Model (Joint Technical Board) This time (5-8 May): Physics Workshop on Thursday 8 th May (whole day) (see: http: //cmsdoc.cern.ch/cms/PRS/www/CPTweek_PRS_schedule.html )

11 11 Higgs Physics/Symmetry breaking Overview of CMS results and current work (15') Sasha Nikitenko 10:15 Higgs to sparticles and Higgs in cascade decays (25') Filip Moortgat 10:45 Higgs in SM and MSSM (I) (30') Michael Spira 11:15 Higgs in SM and MSSM (II) (30') Abdelhak Djouadi 11:45 WW scattering (30') Ezio Maina SUSY and other beyond SM Overview of CMS results and current work on SUSY (25') Alessia Tricomi 14:25 SUSY benchmarks (25') John Ellis 14:50 Comparison of SUSY generators (25') Sabine Kraml 15:15 Extra Dimensions and black holes (25') Gian Giudice 15:40 Radions (20') Daniele Dominici Standard Model Overview of CMS results and current work (25') Michael Dittmar 16:55 Top quark, electroweak physics etc (TBC) (30') Michelangelo Mangano 17:25 QCD (TBC) (30') James Stirling Heavy Ions High-Pt probes in Heavy-Ion Collisions (30') Urs Wiedemann CMS Physics workshop CERN, 8 th May 2003


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