The deficit of neutrino fluxes from Sun detected in all the solar neutrino experiments is a very complex astrophysical but also an elementary particle problem that cannot fit with the Standard Model of the Electroweek Interactions. Many experiments to detect the solar neutrino have been proposed using In as target nucleus due to the low energy threshold of the reaction and and the very good signature for the neutrino event. The new possibilities coming from the development of new InP-based detectors are discussed.
Semi-insulating InP detectors for solar neutrino experiments / Pelfer, P. G.; Dubecky, F.; Fornari, R.; Pikna, M.; Gombia, E.; Zatko, B.; Darmo, J.; Krempasky, M.; Sekacova:, M.. - (2000), pp. 889459.99-889459.104. (Intervento presentato al convegno 3rd International EuroConference on Advanced Semiconductor Devices and Microsystems, ASDAM 2003 tenutosi a Smolenice Castle, Slovakia nel 2000) [10.1109/ASDAM.2000.889459].
Semi-insulating InP detectors for solar neutrino experiments
R. FornariMembro del Collaboration Group
;
2000-01-01
Abstract
The deficit of neutrino fluxes from Sun detected in all the solar neutrino experiments is a very complex astrophysical but also an elementary particle problem that cannot fit with the Standard Model of the Electroweek Interactions. Many experiments to detect the solar neutrino have been proposed using In as target nucleus due to the low energy threshold of the reaction and and the very good signature for the neutrino event. The new possibilities coming from the development of new InP-based detectors are discussed.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
