Atomic and molecular processes in the early Universe

By S. Lepp, P. Stancil, A. Dalgarno. 2002

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Star Formation at Very Low Metallicity. I. Chemistry and Cooling at Low Densities (2007, background): “…H2 in primordial gas has attracted considerable study (Dalgarno & Lepp 1987; Black 1991; Abel et al. 1997; Galli & Palla 1998; Stancil et al. 1998; Lepp et al. 2002), and it is now generally accepted that only a small chemical network, of maybe 20Y30 reactions, is required to model H2 chemistry…”
The big problems in star formation: The star formation rate, stellar clustering, and the initial mass function (2014, background): “See Lepp et al. (2002) and Abel et al. (1997) for thorough reviews of the gasphase chemistry of H2 formation, including discussions of several other, sub-dominant formation channels that I have omitted here.”