The neutrino flux and spectra formation in a supernova core is studied by using a Monte
Carlo code. The dominant opacity contribution for ν μ is elastic scattering on nucleons ν μ …

The current status of the physics of massive neutrinos is reviewed with a forward-looking
emphasis. The article begins with the general phenomenology of neutrino oscillations in …

We describe the effects of neutrino propagation in the matter of the Earth relevant to
experiments with atmospheric and accelerator neutrinos and aimed at the determination of …

When Kai Zuber's pioneering text on neutrinos was published in 2003, the author correctly
predicted that the field would see tremendous growth in the immediate future. In that book …

We show that by combining high precision measurements of the atmospheric δ m 2 in both
the electron and muon neutrino (or antineutrino) disappearance channels one can …

We explore the features of neutrino oscillation which are relevant for measurements of the
leptonic CP violating phase δ and the sign of∆ m 2 13 in experiments with low-energy …

Assuming Majorana neutrinos, we infer from oscillation data the expected values of the
parameters mνe and mee probed by β and 0ν2β-decay experiments. If neutrinos have a …

We start our analysis by deriving a master equation that describes the motion of a field with
arbitrary spin s on a 3-brane embedded in a non-rotating, uncharged (4+ n)-dimensional …

We propose a new parameterization of the antineutrino flux from core collapse supernovae,
that allows an interpretation of its astrophysical parameters within the Bethe and Wilson …

Core-collapse supernova explosions play a wide role in astrophysics by producing compact
remnants (neutron stars or black holes) and the synthesis and injection of many heavy …