The 2nd International Workshop on Low Energy Solar Neutrino Detection, Tokyo, Japan 4-5 December 2000
Author(s)
Bibliographic Information
The 2nd International Workshop on Low Energy Solar Neutrino Detection, Tokyo, Japan 4-5 December 2000
World Scientific, c2001
Available at 6 libraries
Note
Includes bibliographical references and index
Description and Table of Contents
Description
This proceedings volume presents discussions on the technical aspect of the detection of low energy solar neutrinos. Most of the problems related to the experiments aiming to measure low energy solar neutrinos are dealt with.
Table of Contents
- Low Energy Solar Neutrinos: An Introductory Overview (M Fukugita)
- Exotic Solutions to the Solar Neutrino Problem and Some Implications for Low Energy Solar Neutrino Experiments (H Nunokawa)
- Dark Matter (M Minowa)
- Status and Future Perspectives of GNO (N Ferrari)
- Status and Outlook of LENS (R S Raghavan)
- Calibration of the LENS Neutrino Response with Megacurie Source (M Cribier)
- MOON (Mo Observatory of Neutrinos) for Low Energy Neutrinos (H Ejiri)
- Uncertainties in Nuclear Matrix Elements (K Muto)
- Borexino (M G Giammarchi)
- Present Status of KamLAND (K Inoue)
- The HERON Project (R Lanou)
- Low Energy Solar Neutrino Detection by Liquid Xenon (Y Suzuki)
- XMASS (Xenon) II (S Suzuki)
- Detection of Very Small Neutrino Masses in Double-Beta Decay Using Laser Tagging (G Gratta)
- Isotope Separation (A N Choubine)
- CLEAN: A Self-Shielding Detector for Characterizing the Low Energy Solar Neutrino Spectrum (D Mckinsey)
- New Underground Neutrino Observatory - GENIUS - In the New Millennium: For Solar Neutrinos, Dark Matter and Double Beta Decay (H V Klapdor-Kleingrothaus)
- NUMU as a Solar Neutrino Detector (C Broggini)
- Neutron Background (J Abdurashitov)
- Radon Background Reduction and Material Selection (M Laubenstein)
- Muon Induced Background in Solar Neutrino Experiments (T Hagner)
- Determination of Primordial Radioactive Trace Elements in Neutrino Detector Components (R von Hentig)
- 37Ar Artificial Neutrino Source (A Gavrin)
- Why Do Solar Neutrino Experiments Below 1 MeV? (J N Bahcall).
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