Cosmological Implications of Neutrinos
arXiv:hep-ph/0208222 · doi:10.1080/0124421021000054202
Abstract
The lectures describe several cosmological effects produced by neutrinos. Upper and lower cosmological limits on neutrino mass are derived. The role that neutrinos may play in formation of large scale structure of the universe is described and neutrino mass limits are presented. Effects of neutrinos on cosmological background radiation and on big bang nucleosynthesis are discussed. Limits on the number of neutrino flavors and mass/mixing are given.
41 page, 7 figures; lectures presented at ITEP Winter School, February, 2002; to be published in the Proceedings
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- Searching for sterile neutrinos from and decays
- Sterile neutrinos produced near the EW scale I: mixing angles, MSW resonances and production rates
- Neutrino Oscillations in the Early Universe: A Real Time Formulation
- Production of heavy sterile neutrinos from vector boson decay at electroweak temperatures
- Production of a sterile species via active-sterile mixing: an exactly solvable model
- WIMP abundance and lepton (flavour) asymmetry
- Neutrino Oscillations, Entanglement and Coherence: A Quantum Field Theory Study In Real Time
- Space-time evolution of heavy sterile neutrinos in cascade decays
- Dynamics of disentanglement, density matrix and coherence in neutrino oscillations
- Space-time propagation of neutrino wave packets at high temperature and density
- Charged lepton mixing and oscillations from neutrino mixing in the early Universe
- Non equilibrium dynamics of mixing, oscillations and equilibration: a model study
- Oscillations and evolution of a hot and dense gas of flavor neutrinos: a quantum field theory study
- The case for mixed dark matter from sterile neutrinos
- Neutrino collective excitations in the Standard Model at high temperature
- Neutrino Oscillations and the Early Universe
- Detecting the neutrino mass and mass hierarchy from global data
- Dark Neutrinos
- Production of a sterile species: quantum kinetics