Abstract
Estimates of the deuterium abundance in quasar absorbers are reviewed, including a brief account of incorrect claims published by the author and a brief review of the problem of hydrogen contamination. It is concluded that the primordial abundance may be universal with a value (D/H)p ≈ 10−4, within about a factor of two, corresponding to ΩB h 20.7 ≈0.02 or η10 ≈ 2.7 in the Standard Big Bang. This agrees with current limits on primordial helium, Yp ≤ 0.243, which are shown to be surprisingly insensitive to models of stellar enrichment. It also agrees with a tabulated sum of the total density of baryons in observed components. Much lower primordial deuterium (≈ 2 × 10−5) is also possible but disagrees with currently estimated helium abundances; the larger baryon density in this case fits better with current models of the Lyman-α forest but requires the bulk of the baryons to be in some currently uncounted form.
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Hogan, C.J. (1998). Extragalactic Abundances of Hydrogen, Deuterium and Helium. In: Prantzos, N., Tosi, M., Von Steiger, R. (eds) Primordial Nuclei and Their Galactic Evolution. Space Sciences Series of ISSI, vol 4. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-5116-0_12
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