6Li/7Li estimates for metal-poor stars
A.E. Garcia Perez, W. Aoki, S. Inoue, S.G. Ryan, T.K. Suzuki, and M., Chiba

TL;DR
This study measured lithium isotope ratios in five metal-poor stars to investigate the presence of lithium-6, but results were inconclusive due to sensitivity to analysis assumptions and spectral noise.
Contribution
First measurements of 6Li/7Li ratios in a new sample of metal-poor stars using high-resolution spectroscopy, aiming to confirm previous detections.
Findings
6Li/7Li ratios are very low or indistinguishable from zero within errors
Results are highly sensitive to spectral analysis assumptions
No definitive detection of lithium-6 in the sample
Abstract
The presence of the lithium-6 isotope in some metal-poor stars is a matter of surprise because of the high values observed. Non-standard models of Big Bang nucleosynthesis and pre-Galactic cosmic ray fusion and spallation have been proposed to explain these values. However, the observations of this light isotope are challenging which may make some detections disputable. The goal was to determine 6Li/7Li for a sample of metal-poor stars; three of them have been previously studied and the remaining two are new for this type of study. The purpose was to increase, if possible, the number of lithium-6 detections and to confirm previously published results. Spectra of the resonance doublet line of neutral lithium Li I 670.78nm were taken with the High Dispersion Spectrograph at the Subaru 8.2m-telescope for a sample of five metal-poor stars (-3.12 < [Fe/H] < -2.19). The contribution of…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
