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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Univ Roma La Sapienza, Dept Chem, I-00185 Rome, Italy
Univ Roma La Sapienza, CNISM, I-00185 Rome, ItalyUniv Roma La Sapienza, Dept Chem, I-00185 Rome, Italy
Bovino, S.
Stoecklin, T.
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Univ Bordeaux, Inst Mol Sci, F-33405 Talence, FranceUniv Roma La Sapienza, Dept Chem, I-00185 Rome, Italy
Stoecklin, T.
Gianturco, F. A.
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Univ Roma La Sapienza, Dept Chem, I-00185 Rome, Italy
Univ Roma La Sapienza, CNISM, I-00185 Rome, ItalyUniv Roma La Sapienza, Dept Chem, I-00185 Rome, Italy
机构:
Univ Roma La Sapienza, Dept Chem, I-00185 Rome, Italy
Univ Roma La Sapienza, CNISM, I-00185 Rome, ItalyUniv Roma La Sapienza, Dept Chem, I-00185 Rome, Italy
Bovino, S.
Stoecklin, T.
论文数: 0引用数: 0
h-index: 0
机构:
Univ Bordeaux, Inst Mol Sci, F-33405 Talence, FranceUniv Roma La Sapienza, Dept Chem, I-00185 Rome, Italy
Stoecklin, T.
Gianturco, F. A.
论文数: 0引用数: 0
h-index: 0
机构:
Univ Roma La Sapienza, Dept Chem, I-00185 Rome, Italy
Univ Roma La Sapienza, CNISM, I-00185 Rome, ItalyUniv Roma La Sapienza, Dept Chem, I-00185 Rome, Italy