Assessing Big-Bang Nucleosynthesis
- 27 November 1995
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review Letters
- Vol. 75 (22) , 3981-3984
- https://doi.org/10.1103/physrevlett.75.3981
Abstract
Systematic uncertainties in the light-element abundances and their evolution complicate a rigorous statistical assessment. 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 × and 6.5 × and the number of light neutrino species is less than 3.9. Our analysis suggests that the abundance may have been systematically underestimated.
Keywords
All Related Versions
This publication has 18 references indexed in Scilit:
- Big Bang Nucleosynthesis in Crisis?Physical Review Letters, 1995
- Spatially resolved optical and near-infrared spectroscopy of the low-metallicity galaxy UGC 4483The Astrophysical Journal, 1994
- Deuterium abundance and background radiation temperature in high-redshift primordial cloudsNature, 1994
- Probing the early universe: a review of primordial nucleosynthesis beyond the standard big bangPhysics Reports, 1993
- Goddard high-resolution spectrograph observations of the local interstellar medium and the deuterium/hydrogen ratio along the line of sight toward CapellaThe Astrophysical Journal, 1993
- Primordial nucleosynthesis reduxThe Astrophysical Journal, 1991
- Interstellar lines in spectra of extragalactic sources. III Markarian 509, Arakelian 120, and 3C 273The Astrophysical Journal, 1984
- The origin of deuteriumNature, 1976
- On the Origin of Light ElementsThe Astrophysical Journal, 1973
- The Mystery of the Cosmic Helium AbundanceNature, 1964