Supernova neutrino flavor evolution at high densities
Solar and Stellar Astrophysics
2011-11-10 v1 High Energy Physics - Phenomenology
Nuclear Theory
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.
Cite
@article{arxiv.1111.2282,
title = {Supernova neutrino flavor evolution at high densities},
author = {A. B. Balantekin},
journal= {arXiv preprint arXiv:1111.2282},
year = {2011}
}
Comments
Proceedings of the "HAmburg neutrinos from Supernova Explosions (HANSE 2011)" workshop, DESY, Hamburg Site (Germany) from 19 to 23 July 2011