Abstract
Halons are the hypothetical massive elementary components of the galactic halo. They accrete steadily on to stars; a significant internal stellar energy sink results from their presence in a low-mass star. It is shown that halons could solve the solar neutrino problem and the problem of the galactic age.
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Finzi, A. Halons: Massive dark-matter candidates. Astrophys Space Sci 167, 55–59 (1990). https://doi.org/10.1007/BF00642062
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DOI: https://doi.org/10.1007/BF00642062