Results 21 to 30 of about 588 (183)
Solar Models and Solar Neutrinos [PDF]
Invited talk at the XXIII Physics in Collisions Conference (PIC03), Zeuthen, Germany, June 2003, 18 pages, LaTeX, 6 eps and ps figures.
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Solar neutrino detection [PDF]
8 pages, 5 figures. III School on Cosmic Rays and Astrophysics August 25 to September 5, 2008 Arequipa (Peru) AIP conference ...
Lino Miramonti +4 more
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THE SOLAR CORE AND SOLAR NEUTRINOS [PDF]
9 pages; 4 .eps figures; contribution to Carolina Symposium on Neutrino Physics; includes World Scientific ws-p8-50x6-00.cls ...
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Potential for a precision measurement of solar pp neutrinos in the Serappis experiment
The Serappis (SEarch for RAre PP-neutrinos In Scintillator) project aims at a precision measurement of the flux of solar pp neutrinos on the few-percent level.
Lukas Bieger +58 more
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Detecting the upturn of the solar 8B neutrino spectrum with LENA
LENA (Low Energy Neutrino Astronomy) has been proposed as a next generation 50 kt liquid scintillator detector. The large target mass allows a high precision measurement of the solar 8B neutrino spectrum, with an unprecedented energy threshold of 2 MeV ...
R. Möllenberg +7 more
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Solar neutrinos and the decaying neutrino hypothesis
2 ...
Berryman, Jeffrey M. +2 more
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Highlight Talk from Super-Kamiokande
Super-Kamiokande (SK), a 50 kton water Cherenkov detector in Japan, is observing both atmospheric and solar neutrinos. It is also searching for supernova (relic) neutrinos, proton decays and dark matter-like particles. A three-flavor oscillation analysis
Yuuki Nakano +1 more
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11 pages, 6 figures, Proceedings of Physics in Collision Conference, Stanford, California, June ...
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Recent Borexino results and prospects for the near future
The Borexino experiment located in the Gran Sasso National Laboratory, is an organic liquid scintillator detector conceived for the real time spectroscopy of low energy solar neutrinos.
D’Angelo D. +95 more
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ecCNO solar neutrinos: A challenge for gigantic ultra-pure liquid scintillator detectors
Neutrinos produced in the Sun by electron capture reactions on 13N, 15O and 17F, to which we refer as ecCNO neutrinos, are not usually considered in solar neutrino analysis since the expected fluxes are extremely low.
F.L. Villante
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