Refined Big Bang Nucleosynthesis Constraints on and
arXiv:astro-ph/9402010 · doi:10.1103/PhysRevLett.72.3309
Abstract
We include correlations between elemental abundances in a Monte Carlo statistical analysis of BBN predictions, which, along with updated reaction rates and an improved BBN code, lead to tightened constraints on and . Observational upper limits on the primordial \he and fractions of (by weight) and respectively lead to the limits: , and . The former limit appears to be incompatible with purely baryonic galactic halo dark matter, while the latter puts qualitatively new constraints on neutrinos, and physics beyond the standard model.
13 pages, latex, 3 uuencoded figures (appended)
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