Big-bang nucleosynthesis constraints on dark-matter sectors revisited
arXiv:1704.07803
Abstract
We extend previous studies of big bang nucleosynthesis, with the assumption that ordinary matter and dark matter sectors are entangled through the number of degrees of freedom entering the Friedmann equations. This conjecture allows us to find a relation between the temperatures of the weakly interacting matter and dark-matter sectors. The constraints imposed by observations are studied by comparison with calculations of big bang nucleosynthesis for the abundance of light elements. It is found that these constraints are compatible with cold dark matter and a wide range number of dark sectors.
7 pages, 2 figures
References in corpus (7)
- Strongly baryon-dominated disk galaxies at the peak of galaxy formation ten billion years ago
- Hylogenesis: A Unified Origin for Baryonic Visible Matter and Antibaryonic Dark Matter
- Frontiers in Nuclear Astrophysics
- A loophole to the universal photon spectrum in electromagnetic cascades: application to the "cosmological lithium problem"
- Revisiting Big-Bang Nucleosynthesis Constraints on Dark-Matter Annihilation
- The Past and Future of Light Dark Matter Direct Detection
- Solution to Big-Bang Nucleosynthesis in Hybrid Axion Dark Matter Model