Oscillation Induced Neutrino Asymmetry Growth in the Early Universe
arXiv:hep-ph/0112158 · doi:10.1088/1126-6708/2002/02/020
Abstract
We study the dynamics of active-sterile neutrino oscillations in the early universe using full momentum-dependent quantum-kinetic equations. These equations are too complicated to allow for an analytical treatment, and numerical solution is greatly complicated due to very pronounced and narrow structures in the momentum variable introduced by resonances. Here we introduce a novel dynamical discretization of the momentum variable which overcomes this problem. As a result we can follow the evolution of neutrino ensemble accurately well into the stable growing phase. Our results confirm the existence of a "chaotic region" of mixing parameters, for which the final sign of the asymmetry, and hence the SBBN prediction of He(4)-abundance cannot be accurately determined.
23 pages, 9 eps-figs, Latex, uses JHEP class
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- Thermalisation of light sterile neutrinos in the early universe
- Cosmology with self-interacting sterile neutrinos and dark matter - A pseudoscalar model
- Probing secret interactions of eV-scale sterile neutrinos with the diffuse supernova neutrino background
- Active-sterile neutrino oscillations in the early Universe with full collision terms
- Can active-sterile neutrino oscillations lead to chaotic behavior of the cosmological lepton asymmetry?
- Momentum distributions of cosmic relics: Improved analysis
- Chaos, Determinacy and Fractals in Active-Sterile Neutrino Oscillations in the Early Universe