Running of Radiative Neutrino Masses: The Scotogenic Model

We study the renormalization group equations of Ma's scotogenic model, which generates an active neutrino mass at 1-loop level. In addition to other benefits, the main advantage of the mechanism exploited in this model is to lead to a natural loop-suppression of the neutrino mass, and therefore to an explanation for its smallness. However, since the structure of the neutrino mass matrix is altered compared to the ordinary type I seesaw case, the corresponding running is altered as well. We have derived the full set of renormalization group equations for the scotogenic model which, to our knowledge, had not been presented previously in the literature. This set of equations reflects some interesting structural properties of the model, and it is an illustrative example for how the running of neutrino parameters in radiative models is modified compared to models with tree-level mass generation. We also study a simplified numerical example to illustrate some general tendencies of the running. Interestingly, the structure of the RGEs can be exploited such that a bimaximal leptonic mixing pattern at the high-energy scale is translated into a valid mixing pattern at low energies, featuring a large value of \theta_{13}. This suggests very interesting connections to flavour symmetries.Comment: 35 pages, 10 figures, 2 table

Magnetic structure of the Nd5Ge3 compound

Neutron diffraction measurements of the Nd5Ge3 intermetallic compound with a hexagonal structure (space group P6(3)/mcm) have been performed at temperatures of similar to 10 and 293 K. The basis functions of irreducible representations of the space group D (6h) (3) (P6(3)/mcm), which are calculated as a result of the symmetry analysis of possible magnetic structures with the wave vector k = mu b (1), are used to facilitate the search for a real model of the magnetic structure of the compound

Additional file 4 of Mapping age- and sex-specific HIV prevalence in adults in sub-Saharan Africa, 2000–2018

Additional file 4: Supplemental results.1. README. 2. Prevalence range across districts. 3. Prevalence range between sexes. 4. Prevalence range between ages. 5. Age-specific district ranges

Additional file 4 of Mapping age- and sex-specific HIV prevalence in adults in sub-Saharan Africa, 2000–2018

Additional file 4: Supplemental results.1. README. 2. Prevalence range across districts. 3. Prevalence range between sexes. 4. Prevalence range between ages. 5. Age-specific district ranges