Neutrino flavor evolution in dense environments and the r-process
High Energy Physics - Phenomenology
2021-11-17 v1 Solar and Stellar Astrophysics
Nuclear Theory
Abstract
In dense environments, standard and non-standard neutrino interactions with the background particles trigger a variety of flavor mechanisms, which can impact r-process nucleosynthetic abundances. Future observations of a(n) (extra)galactic supernova will tell us about properties of neutrinos and of the astrophysical source that produce them. The upcoming measurement of the diffuse supernova neutrino background constitute a unique source of information. We highlight some recent developments.
Keywords
Cite
@article{arxiv.2111.08250,
title = {Neutrino flavor evolution in dense environments and the r-process},
author = {Maria Cristina Volpe},
journal= {arXiv preprint arXiv:2111.08250},
year = {2021}
}
Comments
5 pages, Proceedings for PANIC2021