Assessing Big-Bang Nucleosynthesis
Astrophysics
2009-10-28 v1
Abstract
Systematic uncertainties in the light-element abundances and their evolution make a rigorous statistical assessment difficult. However, using Bayesian methods we show that the following statement is robust: the predicted and measured abundances are consistent with 95\% credibility only if the baryon-to-photon ratio is between and and the number of light neutrino species is less than 3.9. Our analysis suggests that the He abundance may have been systematically underestimated.
Cite
@article{arxiv.astro-ph/9508029,
title = {Assessing Big-Bang Nucleosynthesis},
author = {Craig J. Copi and David N. Schramm and Michael S. Turner},
journal= {arXiv preprint arXiv:astro-ph/9508029},
year = {2009}
}
Comments
7 pages, LaTeX(2.09), 6 postscript figures (attached). A postscript version with figures can be found at ftp://astro.uchicago.edu/pub/astro/copi/assessing_BBN . (See the README file for details)