Neutrino physics : proceedings of Nobel Symposium 129 : Haga Slott, Enköping, Sweden, August 19-24, 2004 /

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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 osc...

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Detalles Bibliográficos
Clasificación:Libro Electrónico
Autor Corporativo: Nobel Symposium
Otros Autores: Bergström, L. (Lars) (Editor )
Formato: Electrónico Congresos, conferencias eBook
Idioma:Inglés
Publicado: Hackensack, NJ : World Scientific, [2006]
Colección:Physica scripta (Stockholm, Sweden : 1982) ; v. T121.
Temas:
Neutrinos > Congresses.
Neutrino interactions > Congresses.
Solar neutrinos > Congresses.
Neutrinos > Congrès.
Neutrinos > Interactions > Congrès.
Neutrinos solaires > Congrès.
SCIENCE > Physics > Nuclear.
SCIENCE > Physics > Atomic & Molecular.
Neutrino interactions.
Neutrinos.
Solar neutrinos.
Conference papers and proceedings.
Acceso en línea:Texto completo
Tabla de Contenidos:
  • 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. Sakata.
  • 4. 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 ; References.
  • Sudbury 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 Detection.
  • 1. 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 fluxes.

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