Formation of Massive Galactic Halos with Neutrinos

Details Formation of Massive Galactic Halos with Neutrinos Formation of Massive Galactic Halos with Neutrinos

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983pthph..70..603f&link_type=abstract

Progress of Theoretical Physics, Vol. 70, No. 2, pp. 603-605

Physics

3

Scientific paper

Collapse of relic neutrinos is investigated numerically under the
condition of spherical symmetry. Infall of neutrinos produces an
envelope with ρ(r) ∝ r-2.2, in good agreement with a
density profile expected of a galactic halo. Comparison of the results
with a mass model of our Galaxy leads to mν ≅ 30 eV.

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