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- W3100685835 abstract "We have reviewed the chemistry and cooling behaviour of low-density (n H2 + H+, and H- + H -> H2 + e-, is likely to be converted into its para configuration on a faster time scale than the formation time scale. We have tested the model extensively and shown it to agree well with former studies. We further studied the chemical kinetics in great detail and devised a minimal model which is substantially simpler than the full reaction network but predicts correct abundances. This minimal model shows convincingly that 12 collisional processes are sufficient to model the H, He, H+, H-, He+, He++, and H2 abundances in low density primordial gas for applications with no radiation fields." @default.
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- W3100685835 date "1997-08-01" @default.
- W3100685835 modified "2023-10-02" @default.
- W3100685835 title "Modeling primordial gas in numerical cosmology" @default.
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- W3100685835 doi "https://doi.org/10.1016/s1384-1076(97)00010-9" @default.
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