Fujihara SeminarNEUTRINO MASS AND SEESAW MECHANISMSeminar Hall, Building No.3
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| 8:00 | |||||
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| 8:30 |  | Y. Totsuka | (KEK ) | Opening address | |
| Y. Kurosawa | (Fujihara Foundation of Science ) | Welcome address | ||
| 8:40 | | K. Nishijima | (Nishina Memorial Foundation ) | Pauli and the Pauli group | |
| 9:10 | | T. Yanagida | (Tokyo ) | Large lepton mixing in a string brane world | |
| 9:55 | |||||
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| 10:25 | | B. Kayser | (Fermilab ) | The open neutrino questions | |
| 11:10 | | Y. Suzuki | (ICRR, Tokyo ) | Super-Kamiokande: Present and future | |
| 11:55 | | D. Sinclair | (Carleton ) | Results from SNO | |
| 12:40 | |||||
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| 14:10 | | K. Nishikawa | (Kyoto ) | K2K and a next-generation neutrino oscillation experiment from J-PARC to Kamioka | |
| 14:55 | | G. Altarelli | (CERN ) | Models of neutrino masses and mixings | |
| 15:40 | |||||
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| 16:10 | | S. Raby | (Ohio State ) | A natural framework for bi-large neutrino mixing | |
| 16:55 | | J. Pati | (Maryland ) | Neutrino masses, unification and our origin | |
| 17:40 | | T. Moroi | (Tohoku ) |
Curvaton mechanism and its implications to (s)neutrino cosmology | |
| 18:30 - 20:00 | |||||
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| 8:30 | | A. Masiero | (Padova ) | SUSY seesaw and FCNC | |
| 9:15 | | J. Hisano | (ICRR, Tokyo ) | Neutrino-inspired flavor physics | |
| 9:45 | | W. Buchmuller | (DESY ) | Leptons and quarks between branes and bulk | |
| 10:30 | |||||
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| 11:00 | | L.J. Hall | (Berkeley ) | Why are neutrinos light ? | |
| 11:45 | | J. Sato | (Saitama ) | Lepton flavor violation in long-baseline experiments | |
| 12:15 12:30 |
LUNCH | ||||
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| 14:00 | | M. Koshiba | (Tokyo ) | Special Lecture: Neutrino mass and seesaw mechanism | |
| 14:30 | | A. Suzuki | (Tohoku ) | Results from KamLAND | |
| 15:15 | | M.H. Shaevitz | (Columbia ) | MiniBooNE and sterile neutrinos | |
| 16:00 | |||||
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| 16:30 | | H. Minakata | (Tokyo Metropolitan ) | Toward exploring (1-3) sector of the MNS matrix | |
| 17:00 | | K. Hagiwara | (KEK ) | Physics prospects of future neutrino oscillation experiments | |
| 19:00 | |||||
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| 8:30 | | R. Peccei | (UCLA ) | The universality of seesaws | |
| 9:15 | | M. Kawasaki | (RESCEU, Tokyo ) | Big Bang nucleosynthesis, CMB, and neutrino | |
| 10:00 | |||||
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| 10:30 | | J. Ellis | (CERN ) | Sneutrino inflation | |
| 11:15 | | H. Murayama | (Berkeley ) | Alternatives to seesaw | |
| 12:00 | | M. Bando | (Aichi ) | Seesaw mechanism and neutrino mass matrix in GUT | |
| 12:30 | |||||
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| 14:00 | | M. Tanimoto | (Niigata ) | Seesaw realization of bi-large neutrino mixing and leptogenesis | |
| 14:30 | | S. Pakvasa | (Hawaii ) | Neutrino properties from high energy astrophysical neutrinos | |
| 15:15 | | H. Sugawara | (Hawaii ) | M-theory phenomenology and the seesaw mechanism | |
| 16:00 | |||||
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| 16:30 | | P. Ramond | (Florida ) | Neutrinos: key to new physics | |
| 17:15 | |||||
