Halons - Massive dark-matter candidates

Details Halons - Massive dark-matter candidates Halons - Massive dark-matter candidates

May 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.167...55f&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 167, no. 1, May 1990, p. 55-59.

Astronomy and Astrophysics

Astrophysics

Dark Matter, Elementary Particles, Galactic Structure, Stellar Evolution, Halos, Solar Neutrinos, Stellar Mass Accretion

Scientific paper

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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