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The primordial lithium abundance

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Bonifacio, P., Molaro, P.·1997·Monthly Notices of the Royal Astronomical Society

Abstract

Lithium abundances in a selected sample of halo stars have been revised by using the new accurate infrared flux method (IRFM) effective temperatures by Alonso, Arribas & Martíinez-Roger. From 41 plateau stars (Teff>5700 and [Fe/H] ≤ −1.5) we found no evidence for intrinsic dispersion, a tiny trend with Teff and no trend with [Fe/H]. The trend with the Teff is fully consistent with the standard Li isochrones of Deliyannis, Demarque & Kawaler, implying a primordial value for Li of A(Li) = 2.238 ± 0.0121σ ± 0.05sys. The present results argue against any kind of depletion predicted by diffusion, rotational mixing or stellar winds. Therefore the Li observed in Population II stars provides a direct and reliable estimate of the baryonic density which can rival other baryonic indicators such as the deuterium in high-redshift systems. The present upwards revision of primordial Li in the framework of standard big bang nucleosynthesis (SBBN) gives, at 1σ, two solutions for the baryonic density: ΩBh2=0.0062+0.0018−0.0011 or ΩBh2 = 0.0146+0.0029−0.0033.

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Metadata

Authors
Bonifacio, P., & Molaro, P.
Venue
Monthly Notices of the Royal Astronomical Society
Published
1997-03-11
Volume
285
Issue
4
Pages
847-861
ISSN
  • 0035-8711 (ISSN-L)
  • 1365-2966
OpenAlex
W2003678605
Cited by
263
References
0
FWCI
28.95
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: The primordial lithium abundance. https://app.cochat.ai/papers/10.1093/mnras/285.4.847
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Bonifacio, P., & Molaro, P. (1997). The primordial lithium abundance. Monthly Notices of the Royal Astronomical Society. https://doi.org/10.1093/mnras/285.4.847

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