Galactic neutrino models

Details Galactic neutrino models Galactic neutrino models

Oct 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...114..405r&link_type=abstract

Astronomy and Astrophysics, vol. 114, no. 2, Oct. 1982, p. 405, 406.

Astronomy and Astrophysics

Astrophysics

Astronomical Models, Cosmology, Galactic Clusters, Galactic Radiation, Neutrinos, Degenerate Matter, Globular Clusters, Particle Mass

Scientific paper

Fully degenerate neutrino models appear to be in conflict with observations and therefore cannot account for most of the mass missing in galaxies and clusters. Attention is given to the possibility that galactic halos are dominated by freely streaming neutrinos in elongated orbits. The central concentration of the neutrino mass density may affect the distribution of globular clusters within 2 kpc of the center of the galaxy.

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