05331nam 22007214a 450 991045127890332120200520144314.0981-277-390-800318949028118479789812567376(CKB)1000000000410163(EBL)1679797(OCoLC)181590708(SSID)ssj0000209884(PQKBManifestationID)11198216(PQKBTitleCode)TC0000209884(PQKBWorkID)10265657(PQKB)10527368(MiAaPQ)EBC1679797(WSP)00006075(Au-PeEL)EBL1679797(CaPaEBR)ebr10201349(CaONFJC)MIL505378(EXLCZ)99100000000041016320061003d2005 uy 0engur|n|---|||||txtccrNeutrino physics[electronic resource] proceedings of Nobel Symposium 129 : Haga Slott, Enköping, Sweden, August 19-24, 2004 /editors, L. Bergström ... [et al.]New Jersey World Scientificc20051 online resource (192 p.)Physica scripta ;v. T121"Recognised by the European Physical Society."981-256-737-2 Includes bibliographical references.Contents ; John N. Bahcall (1934-2005) ; Preface ; List of Participants ; Committees ; Nobel Symposium on Neutrino Physics-Program ; The History of Neutrino Oscillations ; 1. Introduction ; 2. B. Pontecorvo ; 3. Z. Maki M . Nakagawa and S. Sakata4. B. Pontecorvo and collaborators 5. Conclusion ; References ; Super-Kamiokande Results on Neutrino Oscillations ; 1. Super-Kamiokande ; 2. Atmospheric neutrinos ; 3. Solar neutrinos ; 4. Super-Kamiokande II and III ; 5. Future of Super-Kamiokande ; ReferencesSudbury Neutrino Observatory Results 1. Introduction ; 2. Resolving the solar neutrino ""Problem"" ; 3. The Sudbury Neutrino Observatory ; 4. SNO measurements to date ; 5. Future SNO and SNOLAB measurements ; References ; Results from KamLAND Reactor Neutrino Detection1. Introduction 2. KamLAND detector ; 3. Detector performance ; 4. Reactor anti-neutrino detection ; 5. Data analysis ; 6. Neutrino oscillation analysis ; 7. Conclusions ; References ; New Opportunities for Surprise ; 1. Five clues and ideas ; 2. Why accelerator beams?3. One example surprise: what if LSND is correct? 4. An example explanation: sterile neutrinos ; 5. Pursuing these questions: MiniBooNE and beyond ; 6. Conclusions ; References ; Solar Models and Solar Neutrinos ; 1. Introduction ; 2. Solar model fluxes3. Recent developments regarding the solar surface composition Nobel Symposium 129 on Neutrino Physics was held at Haga Slott in Enköping, Sweden during August 19-24, 2004. Invited to the symposium were around 40 globally leading researchers in the field of neutrino physics, both experimental and theoretical. The dominant theme of the lectures was neutrino oscillations, which after several years were recently verified by results from the Super-Kamiokande detector in Kamioka, Japan and the SNO detector in Sudbury, Canada. Discussion focused especially on effects of neutrino oscillations derived from the presence of matter and the fact that three differenPhysica scripta (Stockholm, Sweden : 1982) ;v. T121.NeutrinosCongressesNeutrino interactionsCongressesSolar neutrinosCongressesElectronic books.NeutrinosNeutrino interactionsSolar neutrinos539.7/215Bergström L(Lars)862060Nobel SymposiumMiAaPQMiAaPQMiAaPQBOOK9910451278903321Neutrino physics1924310UNINA