Lithium-6 : evolution from big bang to present

@article{VangioniFlam1999Lithium6E,
  title={Lithium-6 : evolution from big bang to present},
  author={Elisabeth Vangioni-Flam and Michel Cass{\'e} and Roger. Cayrel and Jean Audouze and Monique Spite and F. Spite},
  journal={New Astronomy},
  year={1999},
  volume={4},
  pages={245-254}
}
The lithium content of the Galactic Halo stars
Thanks to the accurate determination of the baryon density of the universe by the recent cosmic microwave background experiments, updated predictions of the standard model of Big Bang nucleosynthesis
Galactic fly-bys: New source of lithium production
Observations of low-metallicity halo stars have revealed a puzzling result: the abundance of \li7 in these stars is at least three times lower than their predicted primordial abundance. It is unclear
Production of Lithium in the Galactic Disk
The abundance of Li in stars formed within the past 5 Gyr is log N(Li) = 3.2(± 0.2), while the corresponding value for the oldest stars in the Galaxy is log N(Li) = 2.2(± 0.2). The global evidence
Implications of a new temperature scale for halo dwarfs on LiBeB and chemical evolution
Big bang nucleosynthesis (BBN) and the cosmic baryon density from cosmic microwave background anisotropies together predict a primordial 7Li abundance a factor of 2-3 higher than that observed in
COSMOLOGICAL COSMIC RAYS AND THE OBSERVED ^6Li PLATEAU IN METAL-POOR HALO STARS
Very recent observations of the 6Li isotope in halo stars reveal a 6Li plateau about 1000 times above the predicted big bang nucleosynthesis abundance. We calculate the evolution of 6Li versus
The Revival of Galactic Cosmic-Ray Nucleosynthesis?
Because of the roughly linear correlation between Be/H and Fe/H in low-metallicity halo stars, it has been argued that a primary component in the nucleosynthesis of Be must be present in addition to
From First Stars to the Spite Plateau: A Possible Reconciliation of Halo Stars Observations with Predictions from Big Bang Nucleosynthesis
Since the pioneering observations of Spite & Spite in 1982, the constant lithium abundance of metal-poor ([Fe/H] < -1.3) halo stars near the turnoff has been attributed to a cosmological origin.
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The Revival of Galactic Cosmic-Ray Nucleosynthesis?
Because of the roughly linear correlation between Be/H and Fe/H in low-metallicity halo stars, it has been argued that a primary component in the nucleosynthesis of Be must be present in addition to
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