NEUTRINO FACTORY &
MUON STORAGE RINGS AT
CERN
Workshop on a
M
U
O
N
IONIZATION COOLING EXPERIMENT
25-27 October 2001, in CERN PS auditorium,
Bldg. 6-2-006
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Preliminary Agenda
Thursday 25 october
09:00 Welcome
09:15 Motivation 0: A bit of physics: neutrino factory vs alternatives (JJ. Gomez-Cadenas)
09:40 Motivation I: what does neutrino factory gain with cooling (A. Lombardi)
10:00 Motivation II: why does neutrino factory need a cooling experiment
(D. Kaplan)
10:30
coffee break
11:00 report from working groups :
Group a : Simulations
Results of simulations of emmittance reduction
(Hanke, Migliorati...)
Results of simulations of emittance measurement, requirements on beam purity
(P. Janot)
14:00
Group a : Simulations(ctd)
200 MHz cooling experiment
(B. Palmer)
How to get better equilibrium emittance? Consistency with ring cooler?
Scenarios for experiments to be made with the facility, requests on beam and detectors (Hanke et al)
Group f : Beams
Design of a 200-300 MeV Muon Beam at PSI for the Muon Cooling Experiment( C. Petitjean)
Possible beam at RAL (R. Edgecock)
Questions to working groups and organization (A. Blondel)
17:00 end of plenary session
Friday 26 October 2001
morning : parallel group meetings
afternoon :
Group c : RF system
RF cavities design (200 MHz) (Bob Rimmer)
Economics of RF power vs number of cavities (Working group report)
88 MHz option (Roland Garoby)
results from lab G (Al Moretti)
Group g : X rays
X ray emission: how bad is it for the LH2 absorbers and for the detectors? (group report)
X ray emission: how to reduce it? (Jim Norem)
Experimental results (Yagmur Torun or Nick Solomey)
Group b: Hydrogen absorbers
Hydrogen absorber issues (Mary Anne Cummings)
R&D status of the convection type Liquid H2 absorber at KEK (Shigeru Ishimoto)
Design and cost of LH2 absorbers (Ed Black)
20:00
Workshop dinner
Saturday 27 October 2001
9:00
Group c : Magnets
Magnet issues (Mike Green)
Matching of the experimental solenoid with the cooling section
Size and design of the experimental solenoids?
Group e: Diagnostics
beam particle ID
Possible detectors for the cooling experiment
Running-in scenario for the cooling experiment
14:00
Organizational talks :
How can we finance this thing?
US
Europe
What is the overall programme of R&D needed before we can actually finalize the design of the experiment? Where is the bottleneck?
Status of write-up
Discussion and conclusions.
17:00 End
tk
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Last modified on
Fri, Oct 19, 2001