Cargando…
GeV-scale hot sterile neutrino oscillations: a numerical solution
The scenario of baryogenesis through GeV-scale sterile neutrino oscillations is governed by non-linear differential equations for the time evolution of a sterile neutrino density matrix and Standard Model lepton and baryon asymmetries. By employing up-to-date rate coefficients and a non-perturbative...
| Autores principales: | , |
|---|---|
| Lenguaje: | eng |
| Publicado: |
2017
|
| Materias: | |
| Acceso en línea: | https://dx.doi.org/10.1007/JHEP02(2018)078 http://cds.cern.ch/record/2301348 |