Results 91 to 100 of about 579,711 (182)
13. Neutrino mixing 1 13. NEUTRINO MASS, MIXING, AND OSCILLATIONS
The experiments with solar, atmospheric, reactor and accelerator neutrinos have provided compelling evidences for oscillations of neutrinos caused by nonzero neutrino masses and neutrino mixing. The data imply the existence of 3-neutrino mixing in vacuum.
S. T. Petcov (sissa/infn Trieste +3 more
core
Neutrino mixing effects on the tau-neutrino mass limit
We point out that the usual experimental upper bounds on the ''tau-neutrino mass'' do not apply if neutrino mixing is considered. The suppression of the population of the tau decay spectrum near the end point, caused by mixing, may be compensated by an ...
Peres, O. L. G. [UNESP] +9 more
core +1 more source
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
Quantum estimation theory limits in neutrino oscillation experiments
Measurements of the Pontecorvo-Maki-Nakagawa-Sakata (PMNS) neutrino mixing parameters have entered a precision era, enabling increasingly stringent tests of neutrino oscillations.
Claudia Frugiuele +3 more
doaj +1 more source
Standard and Non-Standard Aspects of Neutrino Physics
This review provides a succinct overview of the basic aspects of neutrino physics. The topics covered include neutrinos in the standard model and the three-neutrino mixing scheme; the current status of neutrino oscillation measurements and what remains ...
Alessandro Granelli
doaj +1 more source
Supernova ν flavour conversions in DUNE: the slow, the fast and the standard
The flavour composition of a future supernova neutrino signal is expected to carry measurable imprints of flavour conversion processes in the dense stellar medium.
A. Giarnetti, J. T. Penedo
doaj +1 more source
We examine the octant sensitivity of the long-baseline neutrino oscillation experiments in view of light sterile neutrino flavors with masses in the 1 eV range. Considering the active-sterile mixing, we explore the possible preferred running modes either
Daljeet Kaur
doaj +1 more source
The question of neutrino mixing is considered within the grand unified field theory ...
Tanaka, K., Milton, K.
core
Theory of neutrino slow flavor evolution. Part I. Homogeneous medium
Dense neutrino gases can exhibit collective flavor instabilities, triggering large flavor conversions that are driven primarily by neutrino-neutrino refraction.
Damiano F. G. Fiorillo, Georg G. Raffelt
doaj +1 more source
Rephasing invariance and neutrino mixing
A rephasing invariant parametrization is introduced for three flavor neutrino mixing. For neutrino propagation in matter, these parameters are shown to obey evolution equations as functions of the induced neutrino mass.
Chiu, S. H., Kuo, T. K.
core

