Testing the weakly interacting, massive particle explanation of the solar neutrino puzzle with conventional silicon detectors

Details Testing the weakly interacting, massive particle explanation of the solar neutrino puzzle with conventional silicon detectors Testing the weakly interacting, massive particle explanation of the solar neutrino puzzle with conventional silicon detectors

Jan 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...324l..75s&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X), vol. 324, Jan. 15, 1988, p. L75-L79.

Statistics

Computation

24

Cosmology, Dark Matter, Nuclear Reactions, Particle Interactions, Solar Interior, Solar Neutrinos, Computational Astrophysics, Electromagnetic Radiation, Weak Interactions (Field Theory)

Scientific paper

The authors point out that ionization silicon detectors are sensitive enough to allow the search for weakly interacting dark matter particles with proton or neutron number coherent interactions for masses between 4 and 10 GeV/c2. These are the properties necessary to explain the deficit of solar neutrinos by the cooling of the Sun core by trapped dark matter particles.

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