Single neutron transfer on <SUP>23</SUP>Ne and its relevance for the pathway of nucleosynthesis in astrophysical X-ray bursts



Lotay, G, Henderson, J, Catford, WN, Ali, FA, Berean, J, Bernier, N, Bhattacharjee, SS, Bowry, M, Caballero-Folch, R, Davids, B
et al (show 25 more authors) (2022) Single neutron transfer on <SUP>23</SUP>Ne and its relevance for the pathway of nucleosynthesis in astrophysical X-ray bursts. PHYSICS LETTERS B, 833. p. 137361.

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Abstract

We present new experimental measurements of resonance strengths in the astrophysical 23Al(p,γ)24Si reaction, constraining the pathway of nucleosynthesis beyond 22Mg in X-ray burster scenarios. Specifically, we have performed the first measurement of the (d,p) reaction using a radioactive beam of 23Ne to explore levels in 24Ne, the mirror analog of 24Si. Four strong single-particle states were observed and corresponding neutron spectroscopic factors were extracted with a precision of ∼20%. Using these spectroscopic factors, together with mirror state identifications, we have reduced uncertainties in the strength of the key ℓ = 0 resonance at Er = 157 keV, in the astrophysical 23Al(p,γ) reaction, by a factor of 4. Our results show that the 22Mg(p,γ)23Al(p,γ) pathway dominates over the competing 22Mg(α,p) reaction in all but the most energetic X-ray burster events (T>0.85 GK), significantly affecting energy production and the preservation of hydrogen fuel.

Item Type: Article
Uncontrolled Keywords: 7 Affordable and Clean Energy
Divisions: Faculty of Science and Engineering > School of Physical Sciences
Depositing User: Symplectic Admin
Date Deposited: 14 Mar 2023 15:57
Last Modified: 17 Mar 2024 15:03
DOI: 10.1016/j.physletb.2022.137361
Open Access URL: https://doi.org/10.1016/j.physletb.2022.137361
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URI: https://livrepository.liverpool.ac.uk/id/eprint/3169069