Abstract
The anomaly in lithium abundance is a well-known unresolved problem in nuclear astrophysics. A recent revisit to the problem tried the avenue of resonance enhancement to account for the primordial abundance in standard big-bang nucleosynthesis. Prior measurements of the reaction could not account for the individual contributions of the different excited states involved, particularly at higher energies close to the value of the reaction. We carried out an experiment at HIE-ISOLDE, CERN to study this reaction at , populating excitations up to 22 MeV in for the first time. The angular distributions of the several excited states have been measured and the contributions of the higher excited states in the total cross section at the relevant big-bang energies were obtained by extrapolation to the Gamow window using the talys code. The results show that by including the contribution of the 16.63 MeV state, the maximum value of the total factor inside the Gamow window comes out to be 167 MeV b as compared to earlier estimate of 100 MeV b. However, this still does not account for the lithium discrepancy.
- Received 10 February 2022
- Revised 26 April 2022
- Accepted 19 May 2022
- Corrected 15 December 2022
DOI:https://doi.org/10.1103/PhysRevLett.128.252701
Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI.
Published by the American Physical Society
Physics Subject Headings (PhySH)
Corrections
15 December 2022
Correction: The copyright license statement was presented incorrectly and has been fixed.