Neutrinos, Weak Interactions, and r-process Nucleosynthesis
Nuclear Theory
2015-06-26 v1
Abstract
Two of the key issues in understanding the neutron-to-proton ratio in a core-collapse supernova are discussed. One of these is the behavior of the neutrino-nucleon cross sections as supernova energies. The other issue is the many-body properties of the neutrino gas near the core when both one- and two-body interaction terms are included.
Cite
@article{arxiv.nucl-th/0608047,
title = {Neutrinos, Weak Interactions, and r-process Nucleosynthesis},
author = {A. B. Balantekin},
journal= {arXiv preprint arXiv:nucl-th/0608047},
year = {2015}
}
Comments
To be published in the Proceedings of "International Symposium on Structure of Exotic Nuclei and Nuclear Forces (SENUF 06)", March 2006, Tokyo, Japan