Coherent Active-Sterile Neutrino Flavor Transformation in the Early Universe
arXiv:astro-ph/0607403 · doi:10.1103/PhysRevLett.97.141301
Abstract
We solve the problem of coherent Mikheyev-Smirnov-Wolfenstein (MSW) resonant active-to-sterile neutrino flavor conversion driven by an initial lepton number in the early universe. We find incomplete destruction of lepton number in this process and a sterile neutrino energy distribution with a distinctive cusp and high energy tail. These features imply alteration of the non-zero lepton number primordial nucleosynthesis paradigm when there exist sterile neutrinos with rest masses ~ 1 eV. This could result in better light element probes of (constraints on) these particles.
4 pages, 3 figures, matches version printed in PRL
Cited by in corpus (13)
- Sterile neutrinos, dark matter, and the pulsar velocities in models with a Higgs singlet
- Mixing of Active and Sterile Neutrinos
- Sterile neutrinos, lepton asymmetries, primordial elements: how much of each?
- Lepton Number-Driven Sterile Neutrino Production in the Early Universe
- Neutrino flavor transformation in the lepton-asymmetric universe
- Lepton asymmetry, neutrino spectral distortions, and big bang nucleosynthesis
- Production of a sterile species via active-sterile mixing: an exactly solvable model
- Testing Primordial Abundances With Sterile Neutrinos
- Cosmic Neutrino Decoupling and its Observable Imprints: Insights from Entropic-Dual Transport
- Effects of active-sterile neutrino mixing during primordial nucleosynthesis
- Sterile neutrino states
- The effect of primordial fluctuations on neutrino oscillations
- Production of a sterile species: quantum kinetics