MOON...M olybdenum O bservatory O f N eutrinos . Ejiri et al. PRL 85 (2000) 2917 Low Energy Solar Neutrino Spectroscopy Search for 0in 100 Mo Supernova Neutrino er Doe, University of Washington S 2002, Washington DC, 19 - 21 September, 2002 Physics Goals:
MOON ... M olybdenum O bservatory O f N eutrinos. H. Ejiri et al. PRL 85 (2000) 2917. Physics Goals:. Low Energy Solar Neutrino Spectroscopy Search for 0 in 100 Mo Supernova Neutrino. Peter Doe, University of Washington NeSS 2002, Washington DC, 19 - 21 September, 2002. 100 Mo. - PowerPoint PPT Presentation
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MOON...Molybdenum Observatory Of NeutrinosH. Ejiri et al. PRL 85 (2000) 2917
•Low Energy Solar Neutrino Spectroscopy
• Search for 0 in 100Mo
• Supernova Neutrino
Peter Doe, University of WashingtonNeSS 2002, Washington DC, 19 - 21 September, 2002
Physics Goals:
100Mo
Why Low Energy Solar Neutrinos?
• Eth = 0.168 MeVpp + 7Be Solar Neutrino spectroscopy in real-time
• Large CC ratesRaw rates/ton100Mo/year = 40 7Be, 120 pp