Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
9857797 | Nuclear Physics B - Proceedings Supplements | 2005 | 6 Pages |
Abstract
The understanding of core collapse supernovae (SN) is an important open problem. These objects are intense sources of neutrinos, that can be observed with several types of terrestrial detectors. These two simple considerations, already, motivate close attention toward neutrino interactions in the region from few to 200 MeV. In this work, we offer a selection of results and expectations, and discuss important goals still to be reached.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Nuclear and High Energy Physics
Authors
M.L. Costantini, A. Ianni, F. Vissani,