Results 131 to 140 of about 59,601 (214)
Schemes of Neutrino Mixings (Oscillations) and Their Mixing Matrices
Three schemes of neutrino mixings (oscillations) together with their mixing matrices (analogous to Kabibbo-Kobayashi-Maskawa matrices) are considered. In these schemes neutrino transitions are virtual if neutrino masses are different.
Beshtoev, Kh. M.
core
We determine the possible values of the effective Majorana neutrino mass $|< m > |= |\sum_j U_{ej}^2 m_j|$ in the different phenomenologically viable three and four-neutrino scenarios.
Achkar +17 more
core +4 more sources
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
doaj +1 more source
Neutrino masses and flavor mixing [PDF]
We discuss the neutrino oscillations, using texture zero mass matrices for the leptons. The reactor mixing angle θl is calculated. The ratio of the masses of two neutrinos is determined by the solar mixing angle. We can calculate the masses of the three neutrinos: m1 ≈ 0.003 eV , m2 ≈ 0.012 eV , m3 ≈ 0.048 eV .
openaire +2 more sources
Neutrino oscillation prospects with a dual-baseline beam from BNL to SNOLAB and SURF
The Electron-Ion Collider (EIC) is a next-generation accelerator primarily designed to study the internal structure of nucleons through high-precision electron-hadron collisions.
Nishat Fiza +3 more
doaj +1 more source
Parametrizing the neutrino mixing matrix [PDF]
We propose parametrizations of the neutrino mixing matrix. We discuss several Ansatzes: in some of them $V_{e3}=0$ but in others $V_{e3}$ typically ``comes out'' to be of order $\simeq 0.05.$
openaire +2 more sources
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
Neutrino oscillations and scattering theory
We derive the neutrino oscillation probability in vacuum using scattering theory methods developed earlier in the context of collider physics [1–3]. It is computed from Feynman diagrams that combine neutrino production and detection processes into a ...
Ilian Dobrev +2 more
doaj +1 more source
87th Annual Meeting of the Meteoritical Society 2025: Abstracts
Meteoritics &Planetary Science, Volume 60, Issue S1, Page 30-350, August 2025.
wiley +1 more source
Confronting solutions of the Gallium Anomaly with reactor rate data
Recently, several models have been suggested to reduce the tension between Gallium and reactor antineutrino spectral ratio data which is found in the framework of 3+1 active-sterile neutrino mixing.
Carlo Giunti, Christoph A. Ternes
doaj +1 more source

