Neutrino oscillations in the early universe. Resonant case
A. D. Dolgov
Abstract
Lepton asymmetry generated in the early universe by neutrino oscillations into sterile partners is calculated. Kinetic equations are analytically reduced to a simple form that permits an easy numerical treatment. Asymptotic values of the asymmetry are at the level of 0.2-0.3 and are reasonably close to those obtained by other groups, though the approach to asymptotics in some cases is noticeably slower. No chaoticity is observed.
Create a lesson
Related papers
Theoretical calculations for t tH production
Nikolaos Kidonakis, Nodoka Yamanaka
BSMScanner: a lightweight framework for beyond-the-Standard-Model global fits
Mohamed Belfkir
Chiral mass corrections to decuplet hidden-charm pentaquark states
Yu-Quan Guo, Hao-Song Li
Probing eV-scale sterile neutrinos with neutrinoless double-beta decay and beta decay
Ruisha Yang, Jiajun Liao
χc0 production in Λn scattering process
Quan-Yun Guo, Zhuo Yu, Dian-Yong Chen
Mixed leptogenesis sources and low-energy neutrino portals
Yingnan Xu