Harkness-Brennan, LJ, Page, Robert and Judson, Daniel
(2018)
First Accurate Normalization of the β-delayed α Decay of 16N and Implications for the 12C(α,γ)16O Astrophysical Reaction Rate.
Physical Review Letters, 121 (14).
142701-.
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Abstract
The ^{12}C(α,γ)^{16}O reaction plays a central role in astrophysics, but its cross section at energies relevant for astrophysical applications is only poorly constrained by laboratory data. The reduced α width, γ_{11}, of the bound 1^{-} level in ^{16}O is particularly important to determine the cross section. The magnitude of γ_{11} is determined via sub-Coulomb α-transfer reactions or the β-delayed α decay of ^{16}N, but the latter approach is presently hampered by the lack of sufficiently precise data on the β-decay branching ratios. Here we report improved branching ratios for the bound 1^{-} level [b_{β,11}=(5.02±0.10)×10^{-2}] and for β-delayed α emission [b_{βα}=(1.59±0.06)×10^{-5}]. Our value for b_{βα} is 33% larger than previously held, leading to a substantial increase in γ_{11}. Our revised value for γ_{11} is in good agreement with the value obtained in α-transfer studies and the weighted average of the two gives a robust and precise determination of γ_{11}, which provides significantly improved constraints on the ^{12}C(α,γ) cross section in the energy range relevant to hydrostatic He burning.
Item Type: | Article |
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Additional Information: | 6 pages, 5 figures |
Uncontrolled Keywords: | beta decay, H & He burning, lifetimes and widths, nuclear structure and decays |
Depositing User: | Symplectic Admin |
Date Deposited: | 21 Jan 2019 10:09 |
Last Modified: | 19 Jan 2023 01:06 |
DOI: | 10.1103/PhysRevLett.121.142701 |
Open Access URL: | https://doi.org/10.1103/PhysRevLett.121.142701 |
Related URLs: | |
URI: | https://livrepository.liverpool.ac.uk/id/eprint/3031393 |
Available Versions of this Item
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First Accurate Normalization of the β-delayed α Decay of 16N and Implications for the 12C(α,γ)16O Astrophysical Reaction Rate. (deposited 25 Oct 2018 08:19)
- First Accurate Normalization of the β-delayed α Decay of 16N and Implications for the 12C(α,γ)16O Astrophysical Reaction Rate. (deposited 21 Jan 2019 10:09) [Currently Displayed]