S. Ota
(Li 6, d) and (Li 6, t) reactions on Ne 22 and implications for s -process nucleosynthesis
Ota, S.; Christian, G.; Catford, W. N.; Lotay, G.; Pignatari, M.; Battino, U.; Bennett, E. A.; Dede, S.; Doherty, D. T.; Hallam, S.; Herwig, F.; Hooker, J.; Hunt, C.; Jayatissa, H.; Matta, A.; Moukaddam, M.; Rao, E.; Rogachev, G. V.; Saastamoinen, A.; Scriven, D.; Tostevin, J. A.; Upadhyayula, S.; Wilkinson, R.
Authors
G. Christian
W. N. Catford
G. Lotay
M. Pignatari
U. Battino
E. A. Bennett
S. Dede
D. T. Doherty
S. Hallam
F. Herwig
J. Hooker
C. Hunt
H. Jayatissa
A. Matta
M. Moukaddam
E. Rao
G. V. Rogachev
A. Saastamoinen
D. Scriven
J. A. Tostevin
S. Upadhyayula
R. Wilkinson
Abstract
We studied α cluster states in Mg26 via the Ne22(Li6,dγ)Mg26 reaction in inverse kinematics at an energy of 7 MeV/nucleon. States between Ex = 4-14 MeV in Mg26 were populated and relative α spectroscopic factors were determined. Some of these states correspond to resonances in the Gamow window of the Ne22(α,n)Mg25 reaction, which is one of the main neutron sources in the astrophysical s-process. Using our new Ne22(α,n)Mg25 and Ne22(α,γ)Mg26 reaction rates, we performed new s-process calculations for massive stars and asymptotic giant branch stars and compared the resulting abundances with the abundances obtained using other Ne22+α rates from the literature. We observe an impact on the s-process abundances up to a factor of three for intermediate-mass AGB stars and up to a factor of ten for massive stars. Additionally, states in Mg25 at Ex < 7.5 MeV are identified via the Ne22(Li6,t)Mg25 reaction for the first time. We present the (Li6, t) spectroscopic factors of these states and note similarities to the (d,p) reaction in terms of reaction selectivity.
Citation
Ota, S., Christian, G., Catford, W. N., Lotay, G., Pignatari, M., Battino, U., Bennett, E. A., Dede, S., Doherty, D. T., Hallam, S., Herwig, F., Hooker, J., Hunt, C., Jayatissa, H., Matta, A., Moukaddam, M., Rao, E., Rogachev, G. V., Saastamoinen, A., Scriven, D., …Wilkinson, R. (2021). (Li 6, d) and (Li 6, t) reactions on Ne 22 and implications for s -process nucleosynthesis. Physical Review C, 104(5), Article 055806. https://doi.org/10.1103/PhysRevC.104.055806
Journal Article Type | Article |
---|---|
Acceptance Date | Nov 3, 2021 |
Publication Date | Nov 24, 2021 |
Deposit Date | Jan 22, 2022 |
Journal | Physical Review C |
Print ISSN | 2469-9985 |
Electronic ISSN | 2469-9993 |
Publisher | American Physical Society |
Peer Reviewed | Not Peer Reviewed |
Volume | 104 |
Issue | 5 |
Article Number | 055806 |
DOI | https://doi.org/10.1103/PhysRevC.104.055806 |
Public URL | https://hull-repository.worktribe.com/output/3895083 |
Related Public URLs | https://openresearch.surrey.ac.uk/esploro/outputs/journalArticle/6Li-d-and-6Li-t-reactions/99618063302346?institution=44SUR_INST |
You might also like
Impact of Newly Measured Nuclear Reaction Rates on 26Al Ejected Yields from Massive Stars
(2024)
Journal Article
The NuGrid AGB Evolution and Nucleosynthesis Data Set
(2022)
Journal Article
Slow White Dwarf Mergers as a New Galactic Source of Trans-Iron Elements
(2021)
Presentation / Conference Contribution
Type Ia Supernova Nucleosynthesis: Metallicity-dependent Yields
(2023)
Journal Article
Downloadable Citations
About Repository@Hull
Administrator e-mail: repository@hull.ac.uk
This application uses the following open-source libraries:
SheetJS Community Edition
Apache License Version 2.0 (http://www.apache.org/licenses/)
PDF.js
Apache License Version 2.0 (http://www.apache.org/licenses/)
Font Awesome
SIL OFL 1.1 (http://scripts.sil.org/OFL)
MIT License (http://opensource.org/licenses/mit-license.html)
CC BY 3.0 ( http://creativecommons.org/licenses/by/3.0/)
Powered by Worktribe © 2025
Advanced Search