On the relative abundance of LiH and LiH+ molecules in the early universe: new results from quantum reactions

Details On the relative abundance of LiH and LiH+ molecules in the early universe: new results from quantum reactions On the relative abundance of LiH and LiH+ molecules in the early universe: new results from quantum reactions

2011-02-18

arxiv.org/abs/1102.3812v1

Astronomy and Astrophysics

Astrophysics

Cosmology and Extragalactic Astrophysics

The Astrophysical Journal, in press

Scientific paper

The relative efficiencies of the chemical pathways that can lead to the destruction of LiH and LiH+ molecules, conjectured to be present in the primordial gas and to control molecular cooling processes in the gravitational collapse of the post-recombination era, are revisited by using accurate quantum calculations for the several reactions involved. The new rates are employed to survey the behavior of the relative abundance of these molecules at redshifts of interest for early universe conditions. We find significant differences with respect to previous calculations, the present ones yielding LIH abundances higher than LiH+ at all redshifts.

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