Issue |
EPJ Web of Conferences
Volume 93, 2015
CGS15 – Capture Gamma-Ray Spectroscopy and Related Topics
|
|
---|---|---|
Article Number | 03008 | |
Number of page(s) | 6 | |
Section | Nuclear Astrophysics | |
DOI | https://doi.org/10.1051/epjconf/20159303008 | |
Published online | 28 May 2015 |
https://doi.org/10.1051/epjconf/20159303008
Influence of nuclear reaction rates on the nucleosynthesis in neutrino-driven winds
1 Department of Physics, North Carolina State University, Raleigh, NC 27695-8202, USA
2 Department of Physics and Astronomy, Appalachian State University, Boone, NC 28608, USA
a e-mail: cfrohli@ncsu.edu
Published online: 28 May 2015
We study the sensitivity of the νp-process abundance pattern to (n,p), (p, γ), and (n, γ) rates for nuclei between Ni and Sn. We illustrate our findings for two different initial electron fractions and a representative trajectory. We discuss how these rates influence the abundance pattern and the nuclear flow.
© Owned by the authors, published by EDP Sciences, 2015
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.