Speaker
Description
Summary
Our research is focused on the effects arising near neutrinospheres of core-collapse supernovae due to an interplay between collective effects in neutrino oscillations and the hypothesized non-standard neutrino interactions stemming from beyond-Standard-Model physics. We use numerical simulations (the so-called single-angle scheme) based on analytically derived effective Hamiltonians for collective oscillations, and then carry out a linear stability analysis revealing the spectrum and amplitudes of instabilities. It turns out that certain types of NSIs (notably the transition magnetic moment of Majorana neutrinos) does not trigger 'first-order' instabilities forbidden by certain 'selection rules', while perturbations introduced by other types of NSIs undergo an avalanche-like growth to quite observable values.