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摘要:
Neutral isotopes and ions of H, He and Li define the chemistry of the early universe by collisional and radiative process, where under low temperature and radiation regime, only neutral species were essential in the cooling mass that gave origin to the first proto star structures. Nevertheless, up to now, in every kinetic model Li is permanently discarded from fundamental reactions due to its extremely low density. Contrarily to these previous models we have developed a novel kinetic model based on two consecutive reactions of Li and LiH with H, in order to generate a recursive process that fit well H2 production to temperatures as low as 200 K, according to the cosmological time at the end of the dark epoch. Our results show how Li and LiH merge as first catalyzers of the H to H2 chemical reaction and permit us to explain the expected abundance of H2 as the main coolant in the early universe as well as in cold regions of the cosmos.
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篇名 A Molecular Hydrogen Production Model from Li and LiH in the Early Universe
来源期刊 天文学与天体物理学国际期刊(英文) 学科 医学
关键词 H2 LI and LIH in the DARK EPOCH LI and LIH as PRIMITIVE Catalyzers H2 Production from LI Model
年,卷(期) 2013,(2) 所属期刊栏目
研究方向 页码范围 108-112
页数 5页 分类号 R73
字数 语种
DOI
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H2
LI
and
LIH
in
the
DARK
EPOCH
LI
and
LIH
as
PRIMITIVE
Catalyzers
H2
Production
from
LI
Model
研究起点
研究来源
研究分支
研究去脉
引文网络交叉学科
相关学者/机构
期刊影响力
天文学与天体物理学国际期刊(英文)
季刊
2161-4717
武汉市江夏区汤逊湖北路38号光谷总部空间
出版文献量(篇)
333
总下载数(次)
0
总被引数(次)
0
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