Non-baryonic matter from the halo and the solar neutrino problem

Details Non-baryonic matter from the halo and the solar neutrino problem Non-baryonic matter from the halo and the solar neutrino problem

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...211..441f&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 211, no. 2, March 1989, p. 441-446.

Astronomy and Astrophysics

Astrophysics

5

Elementary Particles, Milky Way Galaxy, Solar Neutrinos, Stellar Evolution, Stellar Structure, Chlorine, Halos, Solar Neighborhood, Stellar Mass Accretion

Scientific paper

The hypothetical massive nonbaryonic components of the Galactic halo known as halons are discussed. The distribution of halons in the solar interior is examined. Evolutionary solar models with halons are considered, showing that the inclusion of halons into solar models causes the temperature of the present sun to have a shallow minimum at the center, with a maximum of about 13 million K. In addition, the rate of capture of solar neutrinos by Cl-37 is studied.

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