arXiv:astro-ph/9902106·v1·Astrophysics
An Active-Sterile Neutrino Transformation Solution for r-Process Nucleosynthesis
G. C. McLaughlin🇺🇸 · J.M. Fetter🇺🇸 · A.B. Balantekin🇺🇸 · G.M. Fuller (Institute for Nuclear Theory, Univ. Washington, Seattle)🇺🇸
Abstract
We discuss how matter-enhanced active-sterile neutrino transformation in both neutrino and antineutrino channels could enable the production of the rapid neutron capture (r-process) nuclei in neutrino-heated supernova ejecta. In this scheme the lightest sterile neutrino would be heavier than the electron neutrino and split from it by a vacuum mass-squared difference roughly between 3 and 70 eV and vacuum mixing angle given by .
Comments: 27 pages plus twelve figures. Submitted to Phys. Rev. C