Neutrino Oscillations
arXiv:1303.2272 · doi:10.1016/j.ppnp.2013.03.007
Abstract
This review summarizes recent experimental and theoretical progress in determining neutrino mixing angles and masses through neutrino oscillations. We describe the basic physics of oscillation phenomena in vacuum and matter, as well as the status of solar, reactor, atmospheric, and accelerator neutrino experiments that probe these phenomena. The results from current global analyses of neutrino parameters are given. Future efforts that may improve the precision with which these parameters are known or probe new aspects of the neutrino mixing matrix are described.
17 Pages, 3 figures
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Cited by in corpus (13)
- Status of neutrino oscillations 2018: first hint for normal mass ordering and improved CP sensitivity
- QCD and strongly coupled gauge theories: challenges and perspectives
- Probing CP violation with non-unitary mixing in long-baseline neutrino oscillation experiments: DUNE as a case study
- Constraints on non-flat cosmologies with massive neutrinos after Planck 2015
- Neutrino oscillations and the seesaw origin of neutrino mass
- Low Energy Probes of Physics Beyond the Standard Model
- Galaxy clustering, CMB and supernova data constraints on CDM model with massive neutrinos
- Cosmological Implications of Light Sterile Neutrinos produced after the QCD Phase Transition
- Effective theory tower for conversion
- Production of heavy sterile neutrinos from vector boson decay at electroweak temperatures
- The case for mixed dark matter from sterile neutrinos
- Asymmetric emissions of neutrinos in the cooling of rotating proto-neutron stars
- Neutrinos, Rare Isotopes of Exotic Nuclei and Nuclear Astrophysics