Results 81 to 90 of about 1,475 (186)
Theory of neutrino masses and mixing [PDF]
23 pages, lecture presented at IV International Pontecorvo Neutrino Physics School, September 26 - October 6, 2010, Alushta, Crimea ...
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Flavor instabilities in dense neutrino media trigger exponential growth of flavor waves, yet their nonlinear saturation remains poorly understood. We examine a simple proxy for this effect in the form of a single-wave solution of an axially symmetric ...
Damiano F. G. Fiorillo, Georg G. Raffelt
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Neutrino loops from neutrino mixing
4 pages, 2 ...
Latosinski, A. +2 more
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Theory of neutrino masses and mixing [PDF]
In this talk I will review our present knowledge on neutrino masses and mixing trying to emphasize what has been definitively proved and what is in the process of being probed. I will also discuss the most important theoretical implications of these results: the existence of new physics, the estimate of the scale of this new physics as well as some ...
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Current and future neutrino oscillation constraints on leptonic unitarity
The unitarity of the lepton mixing matrix is a critical assumption underlying the standard neutrino-mixing paradigm. However, many models seeking to explain the as-yet-unknown origin of neutrino masses predict deviations from unitarity in the mixing of ...
Sebastian A. R. Ellis +2 more
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Dispersion relation of the neutrino plasma: unifying fast, slow, and collisional instabilities
In neutrino-dense astrophysical environments, these particles exchange flavor through a coherent weak field, forming a collisionless neutrino plasma with collective flavor dynamics.
Damiano F. G. Fiorillo, Georg G. Raffelt
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FLAVOR SYMMETRIES, NEUTRINO MASSES AND NEUTRINO MIXING
We discuss the neutrino mixing, using the texture 0 mass matrices, which work very well for the quarks. The solar mixing angle is directly linked to the mass ratio of the first two neutrinos. The neutrino masses are hierarchical, but the mass ratios turn out to be much smaller than for quarks. The atmospheric mixing angle is 38°.
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Status of neutrino mass and mixing [PDF]
In the last two decades experiments have established the existence of neutrino oscillations and most of the related parameters have by now been measured with reasonable accuracy. These results have accomplished a major progress for particle physics and cosmology.
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Vertex reconstruction in the TAO experiment
The Taishan Antineutrino Observatory (TAO) is a tonne-scale gadolinium-doped liquid scintillator satellite experiment of the Jiangmen Underground Neutrino Observatory (JUNO).
Hangyu Shi +4 more
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Flavour-symmetric type-II Dirac neutrino seesaw mechanism
We propose a Standard Model extension with underlying A4 flavour symmetry where small Dirac neutrino masses arise from a Type-II seesaw mechanism. The model predicts the “golden” flavour-dependent bottom-tau mass relation, requires an inverted neutrino ...
Cesar Bonilla +3 more
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