Physics
Scientific paper
Jul 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998apj...501..486t&link_type=abstract
Astrophysical Journal v.501, p.486
Physics
8
Black Hole Physics, Cosmology: Dark Matter, Elementary Particles, Nuclear Reactions, Nucleosynthesis, Abundances
Scientific paper
We propose a novel scenario for the formation and time evolution of dark matter balls composed of degenerate, self-gravitating tau -neutrinos and antineutrinos. This model is based on the interplay of two competing processes: annihilation of the particle-antiparticle pairs via weak interaction and spherical (Bondi) accretion of these particles. Our model can account for the formation of dark matter balls, which could play a role similar to that of supermassive (~109 M&sun;) black holes in active galactic nuclei if the neutrino mass is in the range 10-25 keV/c2.
Tsiklauri David
Viollier Raoul D.
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