no figs. Venice, Neut. Tel (AC's printer)
نویسنده
چکیده
We describe the current situation concerning methods to search for relic neutrinos from the Big Bang and from all past supernovae (SNs). The most promising method for Big Bang neutrinos is by the interaction of ultra-high-energy (UHE) neutrinos. For supernova neutrinos, both Super Kamiokandeand ICARUS-type detectors will be important to study both *e and e fluxes. We also discuss a dedicated supernova burst observatory (OMNIS) being planned for three sites in the world. We also describe the possible analysis of the supernova type-II (SNII) neutrinos, including flavor mixing, that might be carried out in the future.
منابع مشابه
Monitoring Land Subsidence in the Venice Lagoon with Terrasar-x
(1) GAMMA Remote Sensing, Worbstrasse 225, 3073 Gümligen, Switzerland tel: +41 31 951 7005, fax: +41 31 951 7008, e-mail:{strozzi,wegmuller}@gamma-rs.ch (2) Institute of Marine Sciences, National Research Council, National Research Council, San Polo 1364, 30125 Venice, Italy, Email: [email protected] (3) Dept. of Mathematical Methods and Models for Scientific Applications, University of P...
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