Date: Thu, 4 Oct 2001 17:27:36 -0500 From: Jorge_G_Morfin <morfin@fnal.gov> To: Yoshitaka Itow <itow@suketto.icrr.u-tokyo.ac.jp> cc: <opc.nuint01@neutrino.kek.jp> Subject: Re: [itow@suketto.icrr.u-tokyo.ac.jp: [itow@suketto.icrr.u-tokyo.ac.jp: program]] Message-ID: <Pine.SGI.4.31.0110041617170.10604155-100000@fsgi01.fnal.gov> Dear Itow, It's both rewarding and daunting to see everything put together as we think it will actually occur. Only now, with this in front of us, can we get an impression of the flow of the Workshop. I agree with you that the schedule is VERY tight. In fact, I fear that we have so many talks/summaries/comments scheduled (Day 1 - 15, Day 2 - 13, Day 3 - 19!, 1/2Day 4 - 7) that we will have very little time for the all-important discussions which make this a Workshop and not a Symposium. Do others feel the same? If so is there still opportunity to thin the schedule by combining/cutting talks not already committed? For example, I could probably cut 2-3 talks from Session 3 by combining topics. My specific comments can be found in the appended schedule. Best regards, Jorge On Thu, 4 Oct 2001, Yoshitaka Itow wrote: > > HI, > > I made a time table of talks. > Assignment of length of talk is of cource tentative. > You can imagine the schdule is already very tight. > If you have a comment or correction, please tell. > > Regards, > > Y.Itow > > > > < Tentative Program for NUINT01 ver 0.1 Oct-4 > > > > *** 1st day <Dec 13> > > 8:50 Welcome address S.Yamada (KEK) (10') > > Session 1 Objectives and Motivations (Conveners: Sakuda*,Suzuki,Lipari) > > 9:00 For K2K/JHF Y.Itow (ICRR) (20'+5') > 9:25 For MINOS TBA (20'+5') > 9:50 For CNGS TBA (20'+5') > > 10:15-10:30 Coffee Break (15') > > 10:30 For Tau appearance Komatsu (Nagoya U) (20'+5') > 10:55 For CP in nu factory TBA (20'+5') > 11:20 Determination of neutrino oscillation parameters > with atmospheric neutrinos.Atomospheric nu > TBA (ICRR) (20'+5') > 11:45 Prospect of the proton decay experiment and > background for Proton decay > M.Shiozawa (ICRR) (10'+5') > > 12:00-13:30 Lunch > > 13:30 Supernova K.Langanke* () (20'+5') > 13:55 Leptogenesis E. Paschos () (20'+5') > 14:20 QCD and strong interactions TBA (for Mangano) () (20'+5') > > 14:45-15:00 Coffee Break > > Session 3. Theoretical Issues of Neutrino-Nucleus Interactions > and Nuclear Effects > (NUCLEAR EFFECTS IN ELECTRON-NUCLEUS INTERACTIONS THEORY > (Conveners: Morfin*, Seki, Lipari, Para) > > 15:00 Multi-body theory of e-Nucleus interactions > V. Pandharipande* (20'+5') > 15:25 nonP/PQCD look at e-Nucleus int. > T. Thomas (20'+5') > 15:50 Resonance region to DIS, q-hadron duality ** W. Melnitchouk/F. Close (20'+5') ** 16:15 elastic to resonance to DIS nucleon & nucleus TBA ** 16:50 HIgher Twist, Nuclear Effects and Fermi Motion in lepton-nucleus interactions A.Bodek (Rochester) (20'+5') > > > 18:00- Reception > > > > ** 2nd Day (Dec 14) > > Session 3. Theoretical Issues of Neutrino-Nucleus Interactions > and Nuclear Effects (Neutrino-Nucleus interactions) > (Conveners: Morfin*, Seki, Lipari, Para) > > 9:00 Neutrino nucleus interactions and Leptognesises > E. Paschos (20'+5') > 9:25 Final State Interactions in Neutrino Nucleus Scattering > O. Benhar (20'+5') > 9:50 Nuclear re-interactions > J. Marteau (20'+5') > 10:15 How vector current is made to be conserved in nuclei > Kubodera (20'+5') > > 10:40-10:55 Coffee Break > > > 4. Overview of the existing and new data on > neutrino-nucleus interactions and their uncertainties > (Conveners: Itow*/Suzuki/Sakuda) > > 10:55 Review of existing data I (Sub-GeV region) > M.Sakuda (35'+5') > 11:40 Review of existing data II (Multi-GeV region) > J.Morfin (35'+5') > > 12:15-13:30 Lunch > > > 13:30 New data on total cross secion and structure function > Anatoli Vovenko (IHEP) (20'+5') > 13:55 New data from NOMAD > M.Veltri (20'+5') > 14:20 New CC data from K2K Fine Grain Detector > TBA (20'+5') > 14:45 Inclusive measurement Fe in K2K Muon range detector > TBA (20'+5') > 15:10-15:25 Coffee Break > > 15:25 New CC data from K2K 1kt water Chrenkov Detector > TBA (20'+5') > 15:50 New NC data from K2K 1kt water Chrenkov Detector > C.Mauger (20'+5') > 16:15 Proton decay Background study > S.Mine (20'+5') > > > ***3rd day (Dec 15) > > Session 5-1. Comparison of the benchmark MC > Conveners: Casper*/Seki/Hayato/H.R.Gallagher > > > 8:45 NEUT Y.Hayato (KEK) (20'+5') > 9:10 NUANCE D.Casper (UCI) (20'+5') ** 9:35 MINOS/Soudan II H.Gallagher (20'+5') > 10:00 OPERA/NOMAD/DONUT P.Zucchelli (20'+5') > > 10:25-10:40 Coffee Break > > 10:40 Nomad/Icarus A.Rubbia (20'+5') > 11:05 MiniBooNE Mills (20'+5') > 11:30 Icarus F.Cavanna (20'+5') > > 11:55-13:00 Lunch > > Sesion 5-2. Benchmarck calculations and Theoretical calculations(Seki*) > > 13:00 J. Marteau (15'+5') > 13:20 E. Paschos (15'+5') > 13:40 H. Nakamura (15'+5') > 14:00 P. Lipari (15'+5') > 14:20 Gabriel Martinez-Pinedo'* (15'+5') > 14:40 Shri Krishna Singh* (15'+5') > 15:00 Giampaolo Co* (15'+5') > > 15:20-15:35 Coffee Break > > Session 6. Panel Discussion > > Conveners: Seki*/Hayato/Casper/H.R.Gallagher > Chair, Seki; Associate Chair, D. Casper > Panel discussions are carried out by: > V. R. Pandharipande, Y.Hayato, K. Kaneyuki, P. Vogel, > K. Kubodera, K. Langanke > G. Garvey > R. Milner > A. Thomas > H. Toki > M. J. Vincente-Vacas* > C. Ciofi degli Atti* > G. Co > S. K. Singh* > > 15:35 Summary of comparison of benchmark calculations > Toki/Kajita (15') > 15:50 How should Fermi gas model be applied and made realistic? > Vogel/comments; Langanke and Toki (40') > 16:30 How important nuclear correlations are and how should be incorporated, > and how the final-state interactions are best treated? > Pandharipande/comments, Co and Ciofi degli Atti* (40') > 17:10 How should the pion production be treated? > Vincente-Vacas* /comments by Hayato, A.Bodek?, and Singh* (40') > 17:50 The universal neutrino-nucleus MC code. > D.Casper (15') > > 19:00- Possible Dinner ? > > > ** 4th day (Dec16) > > 7. Future experiments and facilities (Conveners: Para*,Itow,Walter) > > 9:00 merits/disadvantages of the existing neutrino beams > (K2K, CERN, FNAL-Booster, FNAL-NuMI,....) > Andre Rubbia (20'+5') > > 9:25 New near detector of K2K, its physics goals and potential > A.Ichikawa (20'+5') > > 9:50 Experimentation at JLAB: what are the existing fecilities/experiments, > potential for modifications and upgrades, potential for new initiatives > TBA (20'+5') > > 10:15-10:30 Coffee Break > > 10:30 Near detector station at NuMI: overview, potential for dedicated > experiments, constraints.. > Rob Plunkett (20'+5') > > 10:55 'small ICARUS' detector as potential technique for studies of low energy > neutrino interactions > Flavio Cavanna (20'+5') > 11:20 Cross section measurements at CERN AD, Fermilab Debuncher > TBA (20'+5') > > 11:45 Summary and Goals for the next NuInt02 > TBA (20') > > > ********* End of Program **************************** > ---------------------------------------------------------------------- > /\/\ Yoshitaka Itow Kamioka Observatory, ICRR, Univ.of Tokyo > /\ \ TEL (0578)5-9610,9627 FAX (0578)5-2121 > / / \ E-mail itow@suketto.icrr.u-tokyo.ac.jp > / |~~/~| \ > / | + | \ 岐阜県吉城郡東茂住 神岡宇宙素粒子研究施設 > / |____| \ 東京大学宇宙線研究所 伊藤 好孝 > -------------------------------------------------------- > > >
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