Supernova neutrino flavor evolution at high densities
A. B. Balantekin (Wisconsin U., Madison)
TL;DR
This paper discusses the complex behavior of neutrino flavor evolution in the dense environment near a supernova's core, emphasizing the role of neutrino-neutrino interactions and symmetries in this non-linear system.
Contribution
It provides an analysis of the symmetries and properties of the non-linear neutrino-neutrino interaction system in supernova conditions.
Findings
Neutrino-neutrino interactions significantly influence flavor evolution.
Symmetries in the non-linear system affect the dynamics.
Properties of the many-neutrino system are characterized.
Abstract
These conference proceedings cover various aspects of neutrino propagation through the high matter and neutrino densities near the proto-neutron star in a core-collapse supernova. A significant feature of this regime is the impact of neutrino-neutrino interactions. Properties of this non-linear many-neutrino system are discussed with a particular emphasis on its symmetries.
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Taxonomy
TopicsNeutrino Physics Research · Particle physics theoretical and experimental studies · Astrophysics and Cosmic Phenomena