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A new particle, the cosmion, has been proposed to be the dark matter of the Universe and to explain the solar {ν} deficit by cooling the solar core to reduce ⁸B {ν} production. Such cosmions in the galactic halo would scatter from nuclei in terrestrial detectors. Measurements were made in Si ionization detectors in a very-low-background environment down to energies of 1.1 keV. These results exclude nearly all of the mass range possible for cosmions with coherent nuclear interactions.
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Caldwell et al. (1990) studied this question.
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