On semi-degenerate equilibrium configurations of a collisionless self-gravitating Fermi gas

Details On semi-degenerate equilibrium configurations of a collisionless self-gravitating Fermi gas On semi-degenerate equilibrium configurations of a collisionless self-gravitating Fermi gas

Mar 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983a%26a...119...35r&link_type=abstract

Astronomy and Astrophysics, vol. 119, no. 1, Mar. 1983, p. 35-41.

Astronomy and Astrophysics

Astrophysics

28

Cosmology, Galactic Clusters, Galactic Evolution, Galactic Radiation, Gravitation Theory, Neutrinos, Particle Mass, Astronomical Models, Collisionless Plasmas, Gravitational Collapse, Halos, Leptons, Mass Distribution

Scientific paper

The authors derive a self consistent solution to the problem of the gravitational equilibrium of a collisionless semi-degenerate Fermi gas. The treatment is applied to model massive halos observed on scales ranging from galaxies to clusters of galaxies, by means of nonzero mass neutrinos. A self consistent lower limit to the neutrino mass is derived for neutrinos to provide the dark mass on various scales in a lepton symmetric universe.

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