Neutrinos and matter-antimatter asymmetry of the universe

Details Neutrinos and matter-antimatter asymmetry of the universe Neutrinos and matter-antimatter asymmetry of the universe

2003-06-05

arxiv.org/abs/hep-ph/0306047v1

Physics

High Energy Physics

High Energy Physics - Phenomenology

14 pages, 6 figures; Talk at `Neutrino Telescopes', Venice, March 2003

Scientific paper

Interactions of heavy Majorana neutrinos in the thermal phase of the early universe may be the origin of the cosmological matter-antimatter asymmetry. Successful baryogenesis, independent of initial conditions, is possible for neutrino masses in the range $10^{-3} {eV} \leq m_i \lesssim 0.1$ eV. Remarkably, this mass window is consistent with the evidence for neutrino masses from oscillations.

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