Neutrino masses, dark matter and the mysterious early quasars

The lightest right-handed or sterile neutrino, that is embedded in a renormalizable seesaw-like extension of the standard model, with a mass m ∼ 15 keV / c 2 and a tiny mixing θ ∼ 1 0 − 6.5 to one of the left-handed active neutrinos, is an attractive quasi-stable dark matter particle candidate. This sterile neutrino is produced in the early universe with the dark matter abundance required by WMAP. It is quasi-stable, decaying in about 1019 years into two neutrinos and an antineutrino, and it may be observed directly through its subdominant radiative decay into an active neutrino and a photon in about 1021 years. In contrast to the galaxies, that are known to form hierarchically, the supermassive black holes are formed anti-hierarchically, i.e. the most massive quasars first, and the least massive active galactic nuclei last. Here we argue that the anti-hierarchical formation of the supermassive black holes may be due to the possibility that both, the quasars and active galactic nuclei, may originate from supermassive degenerate neutrino balls that are swallowed up by stellar-mass black holes, produced by supernova explosions of massive stars at the centers of the neutrino balls.