Comment on the neutrino fraction in our galactic halo

Details Comment on the neutrino fraction in our galactic halo Comment on the neutrino fraction in our galactic halo

Feb 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994phlb..321..390e&link_type=abstract

Physics Letters B, Volume 321, Issue 4, p. 390-393.

Physics

10

Scientific paper

Following Tremaine and Gunn, we discuss what fraction of the density of our galactic halo can be composed of neutrinos. We find that in many cosmological models with mixed hot and cold dark matter, which have been motivated by the recent COBE data and other measurements of large-scale structure, the neutrino mass density fraction in our galactic halo is likely to be much less than the neutrino fraction of the cosmological energy density.

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