Big Bang Nucleosynthesis: 2015

@inproceedings{Cyburt2015BigBN,
  title={Big Bang Nucleosynthesis: 2015},
  author={Richard H. Cyburt and Brian D. Fields and Keith A. Olive and Tsung Han Yeh},
  year={2015}
}
Big-bang nucleosynthesis (BBN) describes the production of the lightest nuclides via a dynamic interplay among the four fundamental forces during the first seconds of cosmic time. We briefly overview the essentials of this physics, and present new calculations of light element abundances through 6Li and 7Li, with updated nuclear reactions and uncertainties including those in the neutron lifetime. We provide fits to these results as a function of baryon density and of the number of neutrino… 

Big-Bang Nucleosynthesis after Planck

We assess the status of big-bang nucleosynthesis (BBN) in light of the final Planck data release and other recent developments, and in anticipation of future measurements. Planck data from the

Big-Bang Nucleosynthesis and Primordial Lithium Abundance Problem

Prediction of the primordial abundances of elements in the big-bang nucleosynthesis (BBN) is one of the three strong evidences for the big bang model. Precise knowledge of the baryon-to-photon ratio

An extended analysis of Heavy Neutral Leptons during Big Bang Nucleosynthesis

Heavy Neutral Leptons (HNLs) are strongly motivated by theory due to their capability of simultaneously explaining the observed phenomena of dark matter, neutrino oscillations and the baryon

New AlterBBN: A Code for Big Bang Nucleosynthesis with Light Dark Matter

The universe is full of stuff we cannot see, neither directly or indirectly. We do not understand the nature of the mysterious dark matter and how it interacts with normal matter. Big Bang

Consequences of neutrino self-interactions for weak decoupling and big bang nucleosynthesis

We calculate and discuss the implications of neutrino self-interactions for the physics of weak decoupling and big bang nucleosynthesis (BBN) in the early universe. In such neutrino-sector extensions

Breaking Be: a sterile neutrino solution to the cosmological lithium problem

The possibility that the so-called ``lithium problem'', i.e., the disagreement between the theoretical abundance predicted for primordial 7Li assuming standard nucleosynthesis and the value inferred

Primordial Deuterium after LUNA: concordances and error budget

The accurate evaluation of the nuclear reaction rates and corresponding uncertainties is an essential requisite for a precise determination of light nuclide primordial abundances. The recent

Baryon Acoustic Oscillations and the Hubble constant: past, present and future

We investigate constraints on the Hubble constant (H0) using Baryon Acoustic Oscillations (BAO) and baryon density measurements from Big Bang Nucleosynthesis (BBN). We start by investigating the

Direct and Indirect Measurements for a Better Understanding of the Primordial Nucleosynthesis

The Big Bang Nucleosynthesis (BBN) model is a great success of nuclear astrophysics due to the outstanding agreement between observational and predicted light elements abundances. One exception,

Big Bang nucleosynthesis constraint on baryonic isocurvature perturbations

We study the effect of large baryonic isocurvature perturbations on the abundance of deuterium (D) produced in big bang nucleosynthesis (BBN). Large baryonic isocurvature perturbations existing at
...

References

SHOWING 1-10 OF 95 REFERENCES

JCAP 0811

  • 012
  • 2008

Nucl

  • Phys. A 918, 61
  • 2013

Astrophys

  • J. 698, 1803
  • 2009

Astron

  • Astrophys. 115, 357
  • 1982

and P

    Phys

    • Rev. D 5, 1628
    • 1972

    Astron

    • Astrophys. 360, 15
    • 2000

    WMAP Science Team Collaboration

    • PTEP 2014, no. 6,
    • 2014

    WMAP Collaboration], Astrophys

    • J. Suppl
    • 2013

    JCAP 1005

    • 003 (2010) [arXiv:1001.5218 [astroph.CO]]; E. Aver, K. A. Olive and E. D. Skillman, JCAP 1103, 043
    • 2011
    ...