Details

Subject(s)

• Neutrinos—Congresses [Browse]
• Neutrino interactions—Congresses [Browse]
• Solar neutrinos—Congresses [Browse]

Related name

• Nobel Symposium [Browse]
• Bergström, L. (Lars) [Browse]

Series

• Physica scripta (Stockholm, Sweden : 1982) ; v. T121. [More in this series]
• Physica scripta ; v. T121

Summary note

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 differen

Notes

"Recognised by the European Physical Society."

Bibliographic references

Includes bibliographical references.

Language note

English

Contents

• 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. 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
• 3. Recent developments regarding the solar surface composition

Show 3 more Contents items

ISBN

981-277-390-8

OCLC

181590708

International Article Number

• 9789812567376

Statement on language in description

Princeton University Library aims to describe library materials in a manner that is respectful to the individuals and communities who create, use, and are represented in the collections we manage. Read more...