Results 41 to 50 of about 2,982,415 (265)

Final results of the search for ν μ → ν e oscillations with the OPERA detector in the CNGS beam

open access: yesJournal of High Energy Physics, 2018
The OPERA experiment has discovered the tau neutrino appearance in the CNGS muon neutrino beam, in agreement with the 3 neutrino flavour oscillation hypothesis.
The OPERA collaboration   +132 more
doaj   +1 more source

Electron-neutrino scattering off nuclei from two different theoretical perspectives [PDF]

open access: yes, 2016
We analyze charged-current electron-neutrino cross sections on Carbon. We consider two different theoretical approaches, on one hand the Continuum Random Phase Approximation (CRPA) which allows a description of giant resonances and quasielastic ...
M. Martini   +5 more
semanticscholar   +1 more source

Neutrino spin oscillations in polarized matter

open access: yesPhysics Letters B, 2019
We study the neutrino spin oscillations, i.e., neutrino spin precession caused by the neutrino interaction with matter polarized by external magnetic field (or, equivalently, by the interaction of the induced magnetic moment (IMM) of a neutrino with the ...
A. Grigoriev, E. Kupcheva, A. Ternov
doaj   +1 more source

Dynamic fast flavor oscillation waves in dense neutrino gases

open access: yesPhysics Letters B, 2020
The flavor transformation in a dense neutrino gas can have a significant impact on the physical and chemical evolution of its surroundings. In this work we demonstrate that a dynamic, fast flavor oscillation wave can develop spontaneously in a one ...
Joshua D. Martin   +2 more
doaj   +1 more source

Searching for BSM neutrino interactions in dark matter detectors

open access: yesJournal of High Energy Physics, 2019
Neutrino interactions beyond the Standard Model (BSM) are theoretically well motivated and have an important impact on the future precision measurement of neutrino oscillation. In this work, we study the sensitivity of a multi-ton-scale liquid Xenon dark
Jonathan M. Link, Xun-Jie Xu
doaj   +1 more source

Recent Results of Electron-Neutrino Appearance Measurement at NOvA [PDF]

open access: yes, 2016
NOvA is a long-baseline accelerator-based neutrino oscillation experiment that is optimized for $\nu_e$ measurements. It uses the upgraded NuMI beam from Fermilab and measures electron-neutrino appearance and muon-neutrino disappearance at its Far ...
J. Bian
semanticscholar   +1 more source

Latest Results from the T2K Neutrino Experiment

open access: yesUniverse, 2019
The T2K long baseline neutrino oscillation experiment measures muon neutrino disappearance and electron neutrino appearance in accelerator-produced neutrino and anti-neutrino beams.
Dean Karlen   +1 more
doaj   +1 more source

Electron–neutrino survival probability from solar-neutrino data

open access: yesPhysics Letters B, 2001
With SNO data on electron-neutrino flux from the sun, it is possible to derive the $ _e$ survival probability $P_{ee}(E)$ from existing experimental data of Super-Kamiokande, gallium experiments and Homestake. The combined data of SNO and Super-Kamiokande provide boron $ _e$ flux and the total flux of all active boron neutrinos, giving thus $P_{ee}(E)
Berezinsky, V, Lissia, M
openaire   +2 more sources

Lepton number violating electron recoils in a U(1)B−L model with non-standard interactions

open access: yesNuclear Physics B, 2023
We propose an SU(3)C×SU(2)L×U(1)Y×U(1)B−L model, in which the neutrino masses and mixings can be generated via Type-I seesaw mechanism after U(1)B−L breaking.
Yugen Lin, Yu Gao, Tianjun Li
doaj   +1 more source

Characterization of the ^{163}Ho Electron Capture Spectrum: A Step Towards the Electron Neutrino Mass Determination.

open access: yesPhysical Review Letters, 2017
The isotope ^{163}Ho is in many ways the best candidate to perform experiments to investigate the value of the electron neutrino mass. It undergoes an electron capture process to ^{163}Dy with an energy available to the decay, Q_{EC}, of about 2.8 keV ...
P. Ranitzsch   +9 more
semanticscholar   +1 more source

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