Physics
Scientific paper
Nov 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000phdt.........5f&link_type=abstract
Thesis (PhD). THE UNIVERSITY OF WISCONSIN - MADISON, Source DAI-B 61/05, p. 2602, Nov 2000, 136 pages.
Physics
2
Scientific paper
The neutrino-driven wind of a Type II supernova, is a likely site for the rapid neutron capture process (r-process) of heavy-element nucleosynthesis. Detailed models of the wind, however, have difficulty reproducing the solar system abundance pattern. In particular, models tend to find a ratio of neutrons to seed nuclei which is too low to account for the abundances of the heaviest elements, around A = 195. One way to increase the neutron-to-seed ratio is to increase the abundance of neutrons, or equivalently, to decrease the electron fraction in the wind. We study matter-enhanced neutrino transformation in the wind, using the channels ne
No associations
LandOfFree
Resonant active-sterile neutrino conversion and r-process nucleosynthesis in neutrino-heated supernova ejecta does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Resonant active-sterile neutrino conversion and r-process nucleosynthesis in neutrino-heated supernova ejecta, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Resonant active-sterile neutrino conversion and r-process nucleosynthesis in neutrino-heated supernova ejecta will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1115622