Relatore
Marie Cornelius
(Niels Bohr Institute, University of Copenhagen)
Descrizione
Neutrinos play a fundamental role in core-collapse supernovae and compact binary mergers. In such dense environments, the coherent forward scattering of neutrinos on each other makes the flavor evolution a non-linear phenomenon. Using a quantum-kinetic approach, we model the neutrino flavor transformation in the presence of neutrino advection, neutrino-matter collisions, and neutrino self-interactions. In this talk, I will explore the impact of inhomogeneities arising in the matter background and temporal perturbations in the fast flavor evolution.
Autore principale
Marie Cornelius
(Niels Bohr Institute, University of Copenhagen)
Coautore
Irene Tamborra
(Niels Bohr Institute)
Shashank Shalgar
(Niels Bohr Institute)
