A Systematic NLTE Study of Very Metal-Poor Stars with Metallicity Down to $-4.3$ dex. II. Lithium Abundance and New Insight to the Lithium Plateau
Hong-Liang Yan, Jinxiao Qin, Shuai Liu, Zeming Zhou, Gang Zhao, Jianrong Shi, Sofya Alexeeva, Huawei Zhang, Haining Li, Huiling Chen, Junbo Zhang, Yufu Shen, Wako Aoki, Tadafumi Matsuno, Jingkun Zhao

TL;DR
This study analyzes lithium abundances in 103 very/extremely metal-poor stars, revealing complex behaviors and challenging previous notions of the lithium plateau, with implications for early Galactic chemical evolution.
Contribution
It provides a homogeneous NLTE analysis of lithium in VMP/EMP stars, extending the lithium plateau to lower metallicities and identifying multiple lithium production mechanisms.
Findings
The lithium abundance shows a positive slope with metallicity, extending the plateau.
Lithium abundance drops rapidly in evolved stars beyond the lower red giant branch.
Four Li-rich stars indicate complex lithium production mechanisms.
Abstract
Metal-poor stars are crucially important for understanding the early Galaxy, first stars, and the Universe. In this series of papers, we present a homogeneous non-local thermodynamic equilibrium (NLTE) abundances analysis of 12 elements for 103 very/extremely metal-poor (VMP/EMP) stars with metallicity down to dex. The sample was selected from the LAMOST survey and observed by the high-resolution spectroscopy of Subaru. In this paper, we present the NLTE abundances and evolution of lithium in these stars. We report different lithium behaviors corresponding to different evolutionary stages and their signatures: 1) The Spite Plateau shows a slightly positive slope, indicating increasing lithium abundance with increasing metallicity. Most significantly, it appears to extend to lower metallicities as previously suggested, calling into question the reality of the so-called 'meltdown'…
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