速報-21;研究会「Future of Neutrino Physics」のプログラムのお知らせ 皆様 先日案内をお送りしました、研究会 "Future of neutrino physics" の(暫定)プログラムを以下にお送りします。(最終プログラムは当日 お配りします。) 興味をお持ちの方の、積極的参加を歓迎します。 (ただし、既に、旅費の補助と宿舎の手配は閉めきらせてしただきました。) 研究会世話人 梶田 kajita [at] suketto.icrr.u-tokyo.ac.jp 福田 fukuda [at] suketto.icrr.u-tokyo.ac.jp ------------------------------------ <<< (Preliminary) Program of the workshop "Future of Neutrino Physics" >>> Place: Auditorium, KEK @ Tanashi (Address: 3-2-1, Midori-cho, Tanashi-shi) * March 3 9:30-10:10 Review of neutrino mass and mixing models M.Tanimoto (Ehime) 10:10-10:50 Interpreting Super-Kamiokande Observations E.Lisi (Bari) 10:50-11:10 Break 11:10-11:40 Atmospheric neutrino measurement at Super-Kamiokande -present and future- T.Kajita (ICRR) 11:40-12:10 Cosmic ray flux measurements T.Sanuki (Tokyo) 12:10-12:30 Recent progress of the flux calculation of atmospheric neutrinos M.Honda (ICRR) 12:30-14:00 Lunch 14:00-14:30 Present status of K2K and the future T.Kobayashi (KEK) 14:30-15:00 Long-baseline neutrino oscillation experiment using emulsion chamber M.Nakamura (Nagoya) 15:00-15:20 Break 15:20-15:50 Lepton-flavor violation in Supersymmetric models J.Hisano (KEK) 15:50-16:20 Experiment to search for mu -> e + gamma T.Mori (Tokyo) 16:20-16:50 Possible detection of ultra-high energy neutrinos in Telescope Array M.Sasaki (ICRR) * March 4 9:30-10:00 Solar models based on helioseiseismology and the solar neutrino problem M.Takata (Tokyo) 10:00-10:20 Measurement of the 7Be(p, gamma)8B cross section at low energies with the coulomb dissociation of 8B T.Motobayashi (Rikkyo) 10:20-10:50 Solar fusion reactions: theoretical approach T.Kajino (NAO) 10:50-11:10 Break 11:10-11:40 Observation of solar neutrinos in Super-Kamiokande -present and future- Y.Takeuchi (ICRR) 11:40-12:05 The Kam-land experiment F.Suekane (Tohoku) 12:05-13:30 Lunch 13:30-14:10 Status of sone R&D projects for pp solar neutrinos -LENS, Hellaz, SuperMUNU - C.Tao (College de France) 14:10-14:35 A future pp solar neutrino experiment M.Nakahata (ICRR) 14:35-14:55 Gamow-Teller strengths for new solar neutrino detectors M.Fujiwara (Osaka) 14:55-15:15 Break 15:15-15:40 ***************** To be confirmed 15:40-16:05 Quark and lepton flavor mixing in the SU(5) GUT N.Okamura (KEK) 16:05-16:30 Vacuum solutions of neutrino anomalies through softly broken U(1) symmetry S.Rindani (Physical Research Lab.(India), and KEK) 16:30-16:55 Neutrino masses in E_6 unification M.Bando (Aichi)