EPJ Web of Conferences
Volume 109, 2016The 13th International Symposium on Origin of Matter and Evolution of Galaxies (OMEG2015)
|Number of page(s)||7|
|Section||Theoretical Nuclear Physics for Astrophysics|
|Published online||12 February 2016|
Statistical Model Analysis of (n, α) Cross Sections for 4.0-6.5 MeV Neutrons
1 School of Engineering and Applied Sciences, Nuclear Research Center, National University of Mongolia, Ulaanbaatar 210646, Mongolia
2 Frank Laboratory of Neutron Physics, JINR, Dubna, Russia
3 Institute of Heavy Ion Physics, Peking University, Beijing, P.R.China
a e-mail: email@example.com
Published online: 12 February 2016
The statistical model based on the Weisskopf-Ewing theory and constant nuclear temperature approximation is used for systematical analysis of the 4.0-6.5 MeV neutron induced (n, α) reaction cross sections. The α-clusterization effect was considered in the (n, α) cross sections. A certain dependence of the (n, α) cross sections on the relative neutron excess parameter of the target nuclei was observed. The systematic regularity of the (n, α) cross sections behaviour is useful to estimate the same reaction cross sections for unstable isotopes. The results of our analysis can be used for nuclear astrophysical calculations such as helium burning and possible branching in the s-process.
© Owned by the authors, published by EDP Sciences, 2016
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.