中文

Assessing Big-Bang Nucleosynthesis

天体物理学 2009-10-28 v1

摘要

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 2×10102\times 10^{-10} and 6.5×10106.5\times 10^{-10} and the number of light neutrino species is less than 3.9. Our analysis suggests that the 4^4He abundance may have been systematically underestimated.

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引用

@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}
}

备注

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)