Results 121 to 130 of about 59,601 (214)
Type II See-Saw Mechanism, Deviations from Bimaximal Neutrino Mixing and Leptogenesis
A possible interplay of both terms in the type II see-saw formula is illustrated by presenting a novel way to generate deviations from exact bimaximal neutrino mixing. In type II see-saw mechanism with dominance of the non-canonical SU(2)_L triplet term,
A. Bandyopadhyay +23 more
core +1 more source
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°.
openaire +2 more sources
Theory of neutrino slow flavor evolution. Part II. Space-time evolution of linear instabilities
Slow flavor evolution (defined as driven by neutrino masses and not necessarily “slow”) is receiving fresh attention in the context of compact astrophysical environments.
Damiano F. G. Fiorillo, Georg G. Raffelt
doaj +1 more source
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
doaj +1 more source
Neutrino masses, mixing and oscillations [PDF]
39 pages, 1 ...
openaire +3 more sources
The JUNO Collaboration has recently released its first reactor antineutrino oscillation result, achieving unprecedented precision in the measurement of ∆ m 21 2 $$ \Delta {m}_{21}^2 $$ and sin2 θ 12.
Yu-Feng Li +3 more
doaj +1 more source
The effects of Majorana phases in three-generation neutrinos
Neutrino-oscillation solutions for the atmospheric neutrino anomaly and the solar neutrino deficit can determine the texture of the neutrino mass matrix according to three types of neutrino mass hierarchies as Type A: $m_1^{} \ll m_2^{} \ll m_3 ...
Haba, N., Matsui, Y., Okamura, N.
core +2 more sources
NEUTRINO MASS, MIXING, AND OSCILLATION [PDF]
Do neutrinos have nonzero masses? If they do, then these masses are very tiny, and can be sought only in very sensitive experiments. The most sensitive of these search for neutrino oscillation, a quantum interference effect which requires neutrino mass and leptonic mixing.
openaire +2 more sources
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
doaj +1 more source
Leptogenesis in an SU(5)×A5 golden ratio flavour model
In this paper we discuss a minor modification of a previous SU(5)×A5 flavour model which exhibits at leading order golden ratio mixing and sum rules for the heavy and the light neutrino masses.
Julia Gehrlein +3 more
doaj +1 more source

