S. Q. Hou
New Thermonuclear Rate of <sup>7</sup>Li(d,n)2<sup>4</sup>He Relevant to the Cosmological Lithium Problem
Hou, S. Q.; Kajino, T.; Trueman, T. C.L.; Pignatari, M.; Luo, Y. D.; Bertulani, C. A.
Authors
T. Kajino
T. C.L. Trueman
M. Pignatari
Y. D. Luo
C. A. Bertulani
Abstract
Accurate 7Li(d,n)24He thermonuclear reaction rates are crucial for precise prediction of the primordial abundances of lithium and beryllium and to probe the mysteries beyond fundamental physics and the standard cosmological model. However, uncertainties still exist in current reaction rates of 7Li(d,n)24He widely used in big bang nucleosynthesis (BBN) simulations. In this work, we reevaluate the 7Li(d,n)24He reaction rate using the latest data on the three near-threshold 9Be excited states from experimental measurements. We present for the first time uncertainties that are directly constrained by experiments. Additionally, we take into account for the first time the contribution from the subthreshold resonance at 16.671 MeV of 9Be. We obtain a 7Li(d,n)24He rate that is overall smaller than the previous estimation by about a factor of 60 at the typical temperature of the onset of primordial nucleosynthesis. We implemented our new rate in BBN calculations, and we show that the new rates have a very limited impact on the final light element abundances in uniform density models. Typical abundance variations are in the order of 0.002%. For nonuniform density BBN models, the predicted 7Li production can be increased by 10% and the primordial production of light nuclides with mass number A > 7 can be increased by about 40%. Our results confirm that the cosmological lithium problem remains a long-standing unresolved puzzle from the standpoint of nuclear physics.
Citation
Hou, S. Q., Kajino, T., Trueman, T. C., Pignatari, M., Luo, Y. D., & Bertulani, C. A. (2021). New Thermonuclear Rate of 7Li(d,n)24He Relevant to the Cosmological Lithium Problem. The Astrophysical journal, 920(2), Article 145. https://doi.org/10.3847/1538-4357/ac1a11
Journal Article Type | Article |
---|---|
Acceptance Date | Aug 1, 2021 |
Online Publication Date | Oct 25, 2021 |
Publication Date | Oct 20, 2021 |
Deposit Date | Jan 22, 2022 |
Publicly Available Date | Oct 21, 2022 |
Journal | Astrophysical Journal |
Print ISSN | 0004-637X |
Electronic ISSN | 1538-4357 |
Publisher | American Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 920 |
Issue | 2 |
Article Number | 145 |
DOI | https://doi.org/10.3847/1538-4357/ac1a11 |
Keywords | Big Bang nucleosynthesis |
Public URL | https://hull-repository.worktribe.com/output/3886789 |
Files
Accepted manuscript
(380 Kb)
PDF
Copyright Statement
©2021 University of Hull
You might also like
Galactic Chemical Evolution of Radioactive Isotopes with an s-process Contribution
(2022)
Journal Article
The RADIOSTAR Project
(2022)
Journal Article
Progress on nuclear reaction rates affecting the stellar production of <sup>26</sup>Al
(2023)
Journal Article
The chemical evolution of the solar neighbourhood for planet-hosting stars
(2023)
Journal Article