2–6 Jul 2018
340 Mandume Ndemufayo Avenue
Africa/Windhoek timezone

Contribution List

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  1. Andrew Zulu (Namibia Univ. of Science and Tech.), Eli Kasai (University of Namibia), Kenneth Cecire (University of Notre Dame), Ketevi Adikle Assamagan (Brookhaven National Laboratory (US)), MWeneni Shahungu (NCRST)
    02/07/2018, 08:00
  2. Andrew Zulu (Namibia Univ. of Science and Tech.), Eli Kasai (University of Namibia)
    02/07/2018, 08:30
  3. Milan Diwan (BNL)
    02/07/2018, 14:00
  4. Heather Gray (LBNL)
    02/07/2018, 16:00
  5. Cathy Cutler (University of Missouri), David Bertsche (Deutsches Elektronen-Synchrotron (DE)), Diouma Kobor (University Assane Seck of Ziguinchor (UASZ)), Heather Gray (LBNL), Kate Shaw (INFN Gruppo Collegato di Udine and ICTP Trieste), Kenneth Cecire (University of Notre Dame), Mary Bishai (Brookhaven National Laboratory (US)), Miland Diwan (BNL)
    03/07/2018, 09:00

    Teachers rotate through 3 activities in 3 groups: Particle Cards, Rolling with Rutherford, and Cloud Chamber Observation.

  6. Albert De Roeck (CERN), Dave Charlton (University of Birmingham (GB)), Heather Gray (LBNL)
    03/07/2018, 10:30
  7. Miland Diwan (BNL)
    03/07/2018, 14:30
  8. Mario Campanelli (University College London (UK)), Milind Vaman Diwan (Brookhaven National Laboratory (US))
    03/07/2018, 16:30
  9. Andrew Zulu (Namibia Univ. of Science and Tech.), Eli Kasai (University of Namibia), Kenneth Cecire (University of Notre Dame), Ketevi Adikle Assamagan (Brookhaven National Laboratory (US)), MWeneni Shahungu (NCRST)
    04/07/2018, 08:30
  10. 04/07/2018, 14:00
  11. Cathy Cutler (University of Missouri), David Bertsche (Deutsches Elektronen-Synchrotron (DE)), Heather Gray (LBNL), Kate Shaw (INFN Gruppo Collegato di Udine and ICTP Trieste), Kenneth Cecire (University of Notre Dame), Mario Campanelli (University College London (UK)), Mary Bishai (Brookhaven National Laboratory (US)), Ulrich Goerlach (Centre National de la Recherche Scientifique (FR))
    05/07/2018, 09:00

    9:00-10:00
    - Intro to Indico schedule
    - Complete Accelerator and Detector presentations
    10:00-10:30
    - Introduction to Cosmic Rays and Cosmic Pi

  12. Cathy Cutler (University of Missouri), David Bertsche (Deutsches Elektronen-Synchrotron (DE)), Heather Gray (LBNL), Kate Shaw (INFN Gruppo Collegato di Udine and ICTP Trieste), Kenneth Cecire (University of Notre Dame), Mary Bishai (Brookhaven National Laboratory (US)), Ulrich Goerlach (Centre National de la Recherche Scientifique (FR))
    05/07/2018, 11:00

    11:00-11:30
    - Talk on Cosmic Rays
    - CR detector demo
    11:30-12:30
    - Zenith Angle experiment with CR detector
    - Examine results
    - Reflections/Q&A

  13. David Bertsche (Deutsches Elektronen-Synchrotron (DE)), Kate Shaw (INFN Gruppo Collegato di Udine and ICTP Trieste), Kenneth Cecire (University of Notre Dame), Mary Bishai (Brookhaven National Laboratory (US)), Ulrich Goerlach (Centre National de la Recherche Scientifique (FR))
    05/07/2018, 14:00
  14. David Bertsche (Deutsches Elektronen-Synchrotron (DE)), Kate Shaw (INFN Gruppo Collegato di Udine and ICTP Trieste), Kenneth Cecire (University of Notre Dame), Mary Bishai (Brookhaven National Laboratory (US)), Ulrich Goerlach (Centre National de la Recherche Scientifique (FR))
    05/07/2018, 14:30

    Teachers are given paper event displays with x- and y-axes of Z boson candidate dimuon events that are almost completely transverse to the beamline. They use protractors, vector analysis, momentum conservation, energy conservation, and the mass-energy-momentum relationship to calculate the Z mass.

  15. Nicole Galante (Stony Brook University)
    05/07/2018, 16:00
  16. Albert De Roeck (CERN), Dave Charlton (University of Birmingham (GB)), David Bertsche (Deutsches Elektronen-Synchrotron (DE)), Kate Shaw (INFN Gruppo Collegato di Udine and ICTP Trieste), Kenneth Cecire (University of Notre Dame)
    06/07/2018, 09:00

    Teachers are given a description of how the detector works and what to expect for results. Teachers examine the detector animation and make their own "cheat sheets" that show the types of events for which they will search. Finally, they will look at real events together.

  17. Dave Charlton (University of Birmingham (GB)), David Bertsche (Deutsches Elektronen-Synchrotron (DE)), Kate Shaw (INFN Gruppo Collegato di Udine and ICTP Trieste), Kenneth Cecire (University of Notre Dame)
    06/07/2018, 10:00
  18. Albert De Roeck (CERN), Dave Charlton (University of Birmingham (GB)), David Bertsche (Deutsches Elektronen-Synchrotron (DE)), Kate Shaw (INFN Gruppo Collegato di Udine and ICTP Trieste), Kenneth Cecire (University of Notre Dame)
    06/07/2018, 11:00

    Teachers will work in pairs. Each pair of teachers will be at a computer and be assigned a dataset of 100 CMS events to analyze visually to determine if each event is a candidate Z, W+, W-, or other particle. In the case of events that look like a Z signature (dilepton events), teachers will create a mass histogram in CIMA. Teachers will also count W+ vs W- events and electron vs muon final...

  19. Dave Charlton (University of Birmingham (GB)), David Bertsche (Deutsches Elektronen-Synchrotron (DE)), Kate Shaw (INFN Gruppo Collegato di Udine and ICTP Trieste), Kenneth Cecire (University of Notre Dame)
    06/07/2018, 14:00

    Teachers will look at masterclass results for the whole group and discuss with physicists. Teachers will also have an introduction to the World Wide Data Day (W2D2) measurement that high school learners will have in their workshops.

  20. Albert De Roeck (CERN), Dave Charlton (University of Birmingham (GB)), David Bertsche (Deutsches Elektronen-Synchrotron (DE)), Heather Gray (LBNL), Kate Shaw (INFN Gruppo Collegato di Udine and ICTP Trieste), Kenneth Cecire (University of Notre Dame), Milind Vaman Diwan (Brookhaven National Laboratory (US))
    06/07/2018, 16:00