Neutrino astrophysical potentialities of a large-mass modular detector based on large activated inorganic single crystals

Details Neutrino astrophysical potentialities of a large-mass modular detector based on large activated inorganic single crystals Neutrino astrophysical potentialities of a large-mass modular detector based on large activated inorganic single crystals

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990soph..128...67g&link_type=abstract

(IAU, The Inside the Sun Colloquium, 121st, Versailles, France, May 22-26, 1989) Solar Physics (ISSN 0038-0938), vol. 128, July

Astronomy and Astrophysics

Astrophysics

1

Nuclear Astrophysics, Scintillation Counters, Solar Neutrinos, Inorganic Materials, Particle Energy, Radiation Detectors, Single Crystals

Scientific paper

Nuclei with the highest rate of capture of low-energy neutrinos were investigated, and the following four were selected for consideration: Li-7, F-19, Na-23, and I-127. Several scintillators for the detection of solar neutrinos are proposed, including LiI(Tl), LiI(Sn), LiI(Eu), LiF(Eu), NaI(Tl), CsI(Tl), and CsI(Na), and the main parameters of the proposed neutrino detectors are discussed.

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