Varying leptonic chemical potentials and spatial variation of primordial deuterium at high z
arXiv:astro-ph/9711202 · doi:10.1016/S1384-1076(99)00007-X
Abstract
We try to explain the spatial variation of primordial deuterium suggested by some observations by varying leptonic chemical potentials. The variation of the latter may take place in some scenarios of leptogenesis. The model predicts a large mass fraction of (35-60%) and (up to ) in deuterium-rich regions. Because of lepton family symmetry, the angular variations of cosmic microwave background radiation can be sufficiently small although still observable in future measurements.
16 pages, latex
References in corpus (2)
Cited by in corpus (11)
- The cosmological baryon density from the deuterium to hydrogen ratio towards QSO absorption systems: D/H towards Q1243+3047
- Update on neutrino mixing in the early Universe
- Active-Sterile neutrino oscillations and BBN+CMBR constraints
- Amplification of Isocurvature Perturbations induced by Active-Sterile Neutrino Oscillations
- On the primordial helium content: CMB and stellar constraints
- Cosmological Deuterium Production in Non-Standard Scenarios
- Inhomogeneous Neutrino Degeneracy and Big Bang Nucleosynthesis
- Big Bang Nucleosynthesis
- Big Bang Nucleosynthesis with Gaussian Inhomogeneous Neutrino Degeneracy
- Alternative Solutions to Big Bang Nucleosynthesis
- Does inhomogeneous big bang nucleosynthesis produce an inhomogeneous element distribution today?