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MICE

n. An International M uon I onization C ooling E xperiment. p. m. MICE. preliminary logo. TOWARDS A PROPOSAL. on 25 March, the MICE collaboration was invited to present a proposal to RAL, with the help of RAL since then RAL nominated a project engineer (Iouri Ivanichenkov).

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MICE

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  1. n An International Muon Ionization Cooling Experiment p m MICE preliminary logo TOWARDS A PROPOSAL

  2. on 25 March, the MICE collaboration was invited to present a proposal to RAL, with the help of RAL since then RAL nominated a project engineer (Iouri Ivanichenkov) MICE found a home! questions: What will MICE be? Who will do what? Who will pay what? When can/should this be done? what will be the logo?

  3. MICE Video Conferences and collaboration meetings MUCOOL/MICE Collaboration meeting 22-26 October @Berkeley Finalize who does what and cost estimates Schedule remaining open questions (decision tree) at that time the input to the proposal should be defined and proposal drafting underway. Date of submission: 15 December 2002 Deadline for contributions 15 November 2002 dates for SG meeting collaboration board meeting dates for video conference MICE Software workshop? will be decided and proposed by next steering group phone meeting (Friday 19 July 4 pm CEST)   comments => alain.blondel@cern.ch

  4. Time lines and cost estimates will be collected by Mike Zisman and Rob Edgecock (cc: A.B. -> steering group) Technical specifications and service needs will be collected by Iouri Ivaniouchenkov and Ed Black (cc: AB and Rob Edgecock)

  5. from MICE LOI : 2002 The schedule of activities can be envisaged as follows, assuming all milestones are passed successfully. 2002: Preparation of proposal and fund raising Integrated simulation of experiment including beam, detectors and cooling cells Evaluation of possible sources of systematic errors Investigation of low equilibrium emittance lattice and of the compatibility with ring coolers Continuous comparison of the 200 MHz and 88 MHz scenarios Test of detectors in X ray environment (already underway) and choice of tracking devices Operation of 88 MHz cavity at CERN and of the test facilities at Fermilab Continued development of liquid hydrogen absorbers Development of alternative schemes for absorbers Competitive design and cost estimates for the solenoids Constitution of a collaboration structure and more detailed distribution of tasks and financial responsibilities Evaluation with the host laboratory of the requirements on space, facilities, safety and radiation issues, and infrastructure Submission of proposal in the course of 2002.

  6. PRIORITIES • Find a home for the experiment • Understand the X ray issue and quantify it in terms of • particle detector performance • 2.’ Develop reconstruction with noise and efficiencies • 3. Choose detectors • 3’. Finalize parameters • 4. Establish technical specs and cost estimates • 4’ Distribute contributions and begin fund hunt mission • 5. Write proposal DONE getting there, BRAVO! Crisis… see Hanke’s talk no, but define set of criteria, actions and decision points Some pending questions..>

  7. pending questions • what is the beam size in the cavities (to minimize Be foils dimensions) • thickness of liq. H2 absorbers • distance between spectrometer solenoid and cooling cell. • … … …

  8. After 1m in = 0 in = 1.330 in = 0.670 B=3.5T B=5T B=6.5T x[m]

  9. muons defocused by fringe field

  10. . Observed dark currents in 800MHz cavity in lab G. The cavity could not be run at a gradient higher than 5 MV/m without emitting one electron or more within a time window of 20 ns. (i.e. 10-8 mA) new curves indicate 10 MV/m Q. Is this the right figure of merit? with 200 MHz? Better probably: observed noise rate in actual detector near the cavity.

  11. => 6.70 MV/m => 4.65 MV/m .43 X 4 cells = 1.7 m  11.5 MV for 1X 4 = 6.70 MV/m 16 MV for 2X4 = 4.65 MV/m 16 MV for 1X4 = 9.3 MV/m

  12. First go at very incomplete tables of who does what

  13. First go at very incomplete tables of who does what to be shared as common fund global supervision of coils necessary (Green) among Oxford/ MUCOOL/ RAL/ LBL/ Saclay/ Italy 1.6 Suggestion: Mike Green will organize a get-together of those who could bid for the magnets and share (at least the cost, maybe construction) and come up with a proposal.

  14. First go at very incomplete tables of who does what common funds ?

  15. First go at very incomplete tables of who does what to be shared point was made that slow control and online reconstruction should be addressed

  16. SIMULATIONS Simulation of performance of cooling cell fairly well understood. Now needed : … simulation of detector response, for design of e.g. downstream PID or to understand performance of Sci-Fi or TPG and first go at some systematics----- … groundwork by Janot needs to be extended … Yagmur has started with a GEANT4 version of MICE. ðothers (Steve Kahn, Vladimir Grichine, more needed) begin or volunteered to implement detector responses and reconstruction conceptual thinking of systematic uncertainties in the measurement needed

  17. Proposed grand time line: 2001 Expose detectors to RF radiation (potential show stopper) write first description of experiment with two options US design (200 MHz) or CERN design (88 MHz) US simulate CERN scheme [and vice versa if possible] Evaluate availability and cost of main cost drivers: RF cavities / amplifiers/ power supplies/solenoids for each scheme evaluate beams + host labs 1st workshop 25-27 October 2001, CERN ! 16 Nov. 2001 ! Chose technology + host lab, write + submit LETTER OF INTENT 25 March 2002 CLRC review June 2002 CLRC + PPARC invite submission of proposal end 2002 Proposal submission end 2004 1st beam (debugging of spectrometers)

  18. MICE : WHEN? GOAL: The long-term goal is to have a Conceptual Design Report for a Neutrino Factory Complex by the time of JHF and LHC start-up, so that, by that date, this would be a valid option for the future of HEP (European Muon Coordination and Oversight Group, April 2002) =2007 MICE must have measured cooling end 2006

  19. draft Proposal for MICE proposal Layout overall edition: Blondel & Kaplan • Executive Summary 1 page • table of contents 1 page • full author list -------!!!!!! 2 pages • responsibility structure 1 page • General motivation (S.Geer & K. Long) • 1.1 Neutrinos and our lives (PR motivation) • 1.2 Neutrino oscillations and the role of NuFact (Particle physics motivation) • 1.3 other physics at NuFact complex and Muon collider • 1.4 Neutrino Factory description (the accelerator) • 1.5 Role of cooling in Neutrino Factory and muon collider, • the need for MICE (Acc. physics motivation) 6 pages • 2. Cooling (Kaplan) • 2.1 principle of Ionization cooling • 2.2 cooling channel design • 2.3 possible extensions (gas cooling and ring coolers) 5 pages • 3. The International Muon Ionization Cooling Experiment (Blondel, Hanke, Palmer) • 3.1 Layout and principle • 3.2 Experiments to be performed • 3.3 Expected performance and statistical precision • 3.4 Systematic errors and resulting requirements • 3.5 possible development of the experiment in time 8 pages

  20. draft Proposal for MICE proposal Layout (ctd) 4. The magnetic channel (Green/Rey) 4.1 layout and optics (Palmer / Fernow) 4.2 design of coils (Green/Rey) 4.3 services (->move to infrastructure chapter 10) 4.4 magnetic measurements (Rey) 4.5 return flux and constraints 8 pages 4.6 responsibilities cost and time line 5. The RF system (Li, Haseroth) 5.1 Cavities 5.2 Windows 5.3 Power supplies 5.4 achievable performance 8 pages 5.6 services and safety (->move to infrastructure chapter 10) 5.5 responsibilities, cost and time-line 6. The absorbers (Cummings/Ishimoto) 6.1 general design 6.2 windows 6.3 thermodynamics (heat exchanger, etc..) 6.4 safety issues(->move to infrastructure chapter 10) 6.5 responsibilities, cost and time-line 8 pages

  21. draft Proposal for MICE proposal Layout (ctd) 7.Beam and beam line (Drumm) 7.1 layout and location 7.2 expected performance and time structure 7.3 time line 6 pages 8. Detectors (Bross/Palladino) 8.1 overall description, functionality and redundancy 8.2 TOF and trigger 8.3.1 tracking device (option I) Scintillating fiber tracker 8.3.2 tracking devices (option II) TPG 8.4 Particle ID 8.5 DAQ, on-line monitoring and reconstruction in each section : responsibilities, costs and time line 15 pages 9. RF radiation on detectors (Norem/McKigney) 9.1 general understanding and characteristics 9.2 measurement results and effect on detectors 9.3 projected effect on performance of MICE (with help of simulation team) 9.4 further measurements to come 6 pages

  22. draft Proposal for MICE proposal Layout (ctd) 10. implementation of MICE at RAL (Ivaniouchenkov, Black) 10.1 Hall layout 10.2 services, cryogenics etc… 10.3 safety issues 10.4 interference with ISIS 10.5 installation plan, time-line, costs and requirements 6 pages 11. Summary of responsibilities, costs, funding and grand time line (Zisman, Edgecock) 6 pages 12. Summary and requirements from RAL 3 pages references appendices (if needed) 92 pages…..

  23. Conclusions & discussion MICE has already shown to be a beneficial approach: RF emissions cost reductions safety windows .. etc.. There will be undoubtedly many other annoying discoveries, ….. followed by clever inventions MICE is essential to convince ourselves – and others – that we know how to build realistic cooling channels Getting a first measurement of cooling before LHC start-up should be feasible but requires good organization and priorities. Funding needs to be found also from outside MC. RAL is inviting us… we must take our chance.

  24. Steering committee: Europe: A. Blondel*1 , H. Haseroth, R. Edgecock, I. Ivaniouchenkov Japan : Y. Kuno US: S. Geer, D. Kaplan2, M. Zisman *convener for coming year, 1 EU spokesperson, 2 US spokesperson Yagmur Torun will be invited as Webmaster/ secretary. Web site: http://hep04.phys.iit.edu/cooldemo/ thanks to Yagmur Torun - torun@iit.edu

  25. a) concept development and simulations: Alessandra Lombardi (CERN)(Alessandra.Lombardi@cern.ch) (K. Hanke deputises) Robert B Palmer (BNL) (palmer@bnl.gov) Yagmur Torun <torun@iit.edu> b) Hydrogen absorbers: Shigeru Ishimoto (KEK) (shigeru.ishimoto@kek.jp) Mary-Anne Cummings (Northern Illinois)( macc@fnal.gov ) c) RF cavities and power supplies Derun Li ( dli@lbl.gov) Roland Garoby (CERN) (Roland.garoby@cern.ch) ->(Helmut Haseroth + RAL person to be identified) d) magnets Mike Green (LBNL) magreen@lbl.gov Jean-Michel Rey (CEA Saclay) e) particle detectors Vittorio Palladino (INFN Napoli) vittorio.palladino@na.infn.it Alan Bross (FNAL) bross@fnal.gov f) beam lines Paul Drumm (RAL) paul.drumm@rl.ac.uk g) RF radiation Jim Norem (Argonne)norem@anl.gov Ed McKigney (IC London) e.mckigney@ic.ac.uk

  26. Participating institutes (In parentheses: contact person in each institute) Louvain La Neuve (G. Grégoire) CERN** (H. Haseroth) NESTOR Institute (L. Resvanis) University of Athens (L. Resvanis) Hellenic Open University (S. Tzamarias) INFN Bari (G. Catanesi) INFN LNF Frascati (M. Castellano, L. Palumbo) INFN Legnaro (U. Gastaldi) INFN Milano (M. Bonesini) INFN Padova (M. Mezzetto) INFN Napoli (G. Osteria) INFN Roma I (L. Ludovici) INFN Roma II (L. Catani) INFN Roma III (L. Tortora) INFN Trieste (M. Apollonio) ** pending the review of CERN activities in accelerator R&D which will take place in the framework of the LHC cost-to-completion analysis. KEK (S. Ishimoto) Osaka University (Y. Kuno) ETH Zurich (A. Rubbia) Paut Scherrer Institute (C. Petitjean) University of Geneva (A. Blondel) University of Zurich (A. Van der Schaaf) Imperial College London (K. Long) Rutherford Appleton Laboratory (R. Edgecock) University of Birmingham (J. Wilson) University of Oxford (G. Barr)

  27. Participating institutes (ctd) (In parentheses: contact person in each institute) Argonne National Laboratory (J. Norem) Brookhaven National Laboratory (R. Palmer) Columbia University (A. Caldwell) Fairfield University (D.Winn) Fermi National Accelerator Laboratory (S. Geer) Illinois Institute of Technology (D. Kaplan) Lawrence Berkeley National Laboratory (M. Zisman) Michigan State University (M. Berz) Northern Illinois University (M. A. Cummings) Princeton University (K. McDonald) University of California Los Angeles (D. Cline) University of California, Riverside/Indiana University (G. Hanson) University of Chicago – Enrico Fermi Institute (K.-J. Kim) University of Illinois at Urbana-Champaign (D. Errede) University of Iowa (Y.Onel) University of Mississippi (D. Summers)

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