Gravitino dark matter and neutrino masses in partial split supersymmetry

In the previous sections we have shown how astronomical alignments and solar hierophanies – with a common interest in the solstices − were substantiated in the

Finally, experiments with solar [17–34], atmospheric [35–45], reactor [46–50], and long-baseline accelerator [51–59] neutrinos indicate that neutrino flavor change through

In this MSSM-seesaw context, the smallness of the light neutrino

In the context of galaxy formation, two fundamental properties are given by the underlying dark matter structure: the distribution of their masses at a certain redshift as the halo

A model of neutrino mass and dark matter with large neutrinoless double beta decay.. Julien Alcaide, Dipankar Das and

In the case of a keV-scale sterile neutrino search, the entire tritium β-decay spectrum is of interest and therefore the main spectrometer would operate at very small retarding

2 we can see that the direct population of the two ionic states from the ground state with the same photon energy cannot lead to any asymmetry because both the kinetic energies of

Each entry is a pair of values: the ratio of the line flux in the central 3 × 3 spaxels over the line flux in the central spaxel, and in parentheses the ratio of the average