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.
