In the next decade the construction of a kilometer-scale Astrophysical Neutrino Observatory in the Mediterranean Sea could become a reality. NEMO Collaboration has been funded both to study the characteristics of some deep sea Mediterranean sites, close to the Italian coast, where the kilometer-scale Cer enkov Detector could be located, and to develop technologies relevant for its design and optimization. Results obtained so far and the program of work for the near future will be described.
Site characterization for a km**3 scale deep underwater astrophysical neutrino observatory in the Mediterranean Sea / Capone, Antonio. - 2:(1999), pp. 444-447. (Intervento presentato al convegno 26th International Cosmic Ray Conference (ICRC 99) tenutosi a Salt Lake City, Utah nel 17-25 Aug 1999).
Site characterization for a km**3 scale deep underwater astrophysical neutrino observatory in the Mediterranean Sea.
CAPONE, Antonio
1999
Abstract
In the next decade the construction of a kilometer-scale Astrophysical Neutrino Observatory in the Mediterranean Sea could become a reality. NEMO Collaboration has been funded both to study the characteristics of some deep sea Mediterranean sites, close to the Italian coast, where the kilometer-scale Cer enkov Detector could be located, and to develop technologies relevant for its design and optimization. Results obtained so far and the program of work for the near future will be described.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
