Faestermann, T. and Mohr, Péter and Hertenberger, R. and Wirth, H.-F. (2015) Broad levels in O 17 and their relevance for the astrophysical s process. PHYSICAL REVIEW C, 92 (5). ISSN 2469-9985
|
Text
1511.02642.pdf Available under License Creative Commons Attribution. Download (195kB) | Preview |
Abstract
Levels in 17O affect the astrophysical s-process in two opposite ways. The neutron production is enhanced by resonances in the 13C(α,n) 16O reaction at excitation energies around 7 MeV in 17O, and the number of available neutrons is reduced by low-lying resonances in the 16O(n,γ) 17O reaction corresponding to levels in 17O with excitation energies of 4−5MeV. The present work uses the 19F(d,α) 17O reaction to determine absolute widths of the relevant levels in 17O. The results improve the uncertainties of the previously adopted values and resolve a discrepancy between recent studies for the 1/2 + level close to the threshold of the 13C(α,n) 16O reaction. In addition, improved excitation energies and widths are provided for several states in 17O up to excitation energies close to 8 MeV.
Item Type: | Article |
---|---|
Subjects: | Q Science / természettudomány > QC Physics / fizika |
SWORD Depositor: | MTMT SWORD |
Depositing User: | MTMT SWORD |
Date Deposited: | 04 Dec 2023 12:37 |
Last Modified: | 04 Dec 2023 12:37 |
URI: | http://real.mtak.hu/id/eprint/181724 |
Actions (login required)
![]() |
Edit Item |