Big Bang Nucleosynthesis: an accurate determination of light element yields
arXiv:astro-ph/9906232 · doi:10.1016/S0550-3213(99)00725-7
Abstract
We report the results of a new accurate evaluation of light nuclei yields in primordial nucleosynthesis. All radiative effects, finite nucleon mass, thermal and plasma corrections are included in the proton to neutron conversion rates. The relic densities of He4, D and Li7 have been numerically obtained via a new updated version of the standard BBN code. In particular the theoretical uncertainty on He4 is reduced to the order of 0.1%.
arXiv commentplain LaTeX, 35 pages, 10 figure.ps and 4 figure.eps
References in corpus (14)
- The Cosmological Baryon Density from the Deuterium Abundance at a redshift z = 3.57
- The primordial lithium abundance
- Nonequilibrium Corrections to the Spectra of Massless Neutrinos in the Early Universe
- Neutrino decoupling in the early Universe
- A High Deuterium Abundance at z=0.7
- Precision Prediction for the Big-Bang Abundance of Primordial Helium
- Refined Big Bang Nucleosynthesis Constraints on and
- Quantifying uncertainties in primordial nucleosynthesis without Monte Carlo simulations
- The Cosmological Density and Ionization of Hot Gas: Oxygen VI Absorption in Quasar Spectra
- Effect of Neutrino Heating on Primordial Nucleosynthesis
- Precision Rates for Nucleon Weak Interactions in Primordial Nucleosynthesis and He-4 Abundance
- Effect of Finite Mass on Primordial Nucleosynthesis
- Wave Function Renormalization at Finite Temperature
- Finite Temperature Wave-Function Renormalization, A Comparative Analysis
Cited by in corpus (29)
- Big-Bang Nucleosynthesis Predictions for Precision Cosmology
- Primordial Nucleosynthesis: from precision cosmology to fundamental physics
- Precision big bang nucleosynthesis with improved Helium-4 predictions
- The Deuterium to Hydrogen Abundance Ratio Towards a Fourth QSO: HS0105+1619
- Primordial Nucleosynthesis in Light of WMAP
- PArthENoPE: Public Algorithm Evaluating the Nucleosynthesis of Primordial Elements
- Nuclear Reaction Network for Primordial Nucleosynthesis: a detailed analysis of rates, uncertainties and light nuclei yields
- A Realistic Determination of the Error on the Primordial Helium Abundance: Steps Toward Non-Parametric Nebular Helium Abundances
- Probing oscillations into sterile neutrinos with cosmology, astrophysics and experiments
- Early-universe constraints on a time-varying fine structure constant
- Present status of primordial nucleosynthesis after WMAP: results from a new BBN code
- Constraining neutrino physics with BBN and CMBR
- Solar Neutrino Constraints on the BBN Production of Li
- Constraining the helium abundance with CMB
- Does Solar Physics Provide Constraints to Weakly Interacting Massive Particles?
- Updated constraint on a primordial magnetic field during big bang nucleosynthesis and a formulation of field effects
- Testing Standard and Degenerate Big Bang Nucleosynthesis with BOOMERanG and MAXIMA-1
- Revisiting the Constraint on the Helium Abundance from CMB
- Cosmological nucleosynthesis and active-sterile neutrino oscillations with small mass differences: The resonant case
- Effects of power law primordial magnetic field on big bang nucleosynthesis
- Kinetic theory of fermions in curved spacetime
- The Increase in the Primordial He-4 Yield in the Two-Doublet Four-Neutrino Mixing Scheme
- Overproduction of primordial helium-4 in the presence of neutrino oscillations
- Supersymmetric Dark Matter
- Nucleosynthesis constraint on Lorentz invariance violation in the neutrino sector
- Candidates for non-baryonic dark matter
- Neutrino Oscillations and the Early Universe
- Primordial Nucleosynthesis, Cosmic Microwave Background and Neutrinos
- Neutrinos and Primordial Nucleosynthesis