Year: 2006
Type: conference-paper
Abstract: Two of the key issues in understanding the neutron-to-proton ratio in a corecollapse 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.
Author: A B Balantekin
Institution: University of Wisconsin–Madison
Language: English
Topic: Neutrino Physics Research
Subfield: Nuclear and High Energy Physics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: diamond
Funder: National Science Foundation
OpenAlex ID: W1989104293