Solar and supernova neutrino physics with Sudbury Neutrino Observatory

1992 ◽  
Vol 45 (4) ◽  
pp. 1059-1065 ◽  
Author(s):  
A. B. Balantekin ◽  
F. Loreti
Keyword(s):  
Neutrino Physics ◽  
Sudbury Neutrino Observatory ◽  
Supernova Neutrino

RECENT RESULTS FROM THE SUPER-KAMIOKANDE EXPERIMENT

2008 ◽  
Vol 23 (21) ◽  
pp. 3358-3365
Author(s):  
SHAOMIN CHEN
Keyword(s):  
Neutrino Physics ◽  
Current Status ◽  
Future Prospects ◽  
Transition Processes ◽  
The Future ◽  
Supernova Neutrino

This talk presents the current status of the Super-Kamiokande experiment, including the recent results on atmospheric, solar and supernova neutrino physics. Also presented are the searches on ΔB ≠ 0 transition processes and the future prospects.

Supernova Neutrino Physics with a Megaton Detector

2005 ◽  
Vol 143 ◽  
pp. 558
Author(s):  
G.L. Fogli ◽  
E. Lisi ◽  
A. Mirizzi ◽  
D. Montanino
Keyword(s):  
Neutrino Physics ◽  
Supernova Neutrino

scholarly journals Supernova neutrino physics in future water-Cherenkov detectors

2007 ◽  
Author(s):  
Eligio Lisi ◽  
Gianluigi Fogli ◽  
Alessandro Mirizzi ◽  
Daniele Montanino
Keyword(s):  
Neutrino Physics ◽  
Cherenkov Detectors ◽  
Supernova Neutrino ◽  
Water Cherenkov Detectors

scholarly journals LOW ENERGY NEUTRINO PHYSICS AFTER SNO AND KamLAND

2004 ◽  
Vol 19 (05) ◽  
pp. 337-348 ◽  
Author(s):  
L. OBERAUER
Keyword(s):  
Neutrino Physics ◽  
Solar Neutrino ◽  
Liquid Scintillator ◽  
Low Energy ◽  
Neutrino Masses ◽  
Neutrino Experiment ◽  
Neutrino Detection ◽  
Energy Neutrino ◽  
Supernova Neutrino ◽  
Solar Neutrino Experiment

In the recent years important discoveries in the field of low energy neutrino physics (Eν in the ≈ MeV range) have been achieved. Results of the solar neutrino experiment SNO show clearly flavor transitions from νe to νμ,τ. In addition, the long standing solar neutrino problem is basically solved. With KamLAND, an experiment measuring neutrinos emitted from nuclear reactors at large distances, evidence for neutrino oscillations has been found. The values for the oscillation parameters, amplitude and phase, have been restricted. In this paper the potential of future projects in low energy neutrino physics is discussed. This encompasses future solar and reactor experiments as well as the direct search for neutrino masses. Finally the potential of a large liquid scintillator detector in an underground laboratory for supernova neutrino detection, solar neutrino detection, and the search for proton decay p→K+ν is discussed.

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