Stimulated Radiative Association of Li and H in the Early Universe

Details Stimulated Radiative Association of Li and H in the Early Universe Stimulated Radiative Association of Li and H in the Early Universe

Apr 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997apj...479..543s&link_type=abstract

Astrophysical Journal v.479, p.543

Astronomy and Astrophysics

Astronomy

31

Atomic Processes, Cosmology: Cosmic Microwave Background, Cosmology: Early Universe

Scientific paper

The enhancement of the rate coefficient for the radiative association of
Li and H to form LiH arising from stimulated emission by the cosmic
background radiation field is calculated. It is shown that the effect on
the fractional abundance of LiH in the early universe for redshifts z
between 1000 and 10 is small.

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