T2K is a long baseline neutrino oscillation experiment. A high intensity proton beam at J-PARC produces a narrow-band muon-neutrino beam with a peak energy of 0.6 GeV at the far detector, Super-Kamiokande, 295km from the production point.
Hadley David
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The gallium anomaly, i.e. the missing electron-neutrino flux from 37Ar and 51Cr electron-capture decays as measured by the GALLEX and SAGE solar-neutrino detectors, has been among us already for about two decades.
J. Kostensalo +3 more
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Mapping the neutrino floor for direct detection experiments based on dark matter-electron scattering [PDF]
Jason Wyenberg, Ian M. Shoemaker
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Sterile Neutrino Searches with MicroBooNE: Electron Neutrino Disappearance
A sterile neutrino is a well motivated minimal new physics model that leaves an imprint in neutrino oscillations. Over the last two decades, a number of hints pointing to a sterile neutrino have emerged, many of which are pointing near $m_4\sim1$ eV. Here we show how MicroBooNE data can be used to search for electron neutrino disappearance using each ...
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Mini-LANNDD T40: A detector to measure the neutrino-argon cross section and the electron-neutrino contamination in the off-axis NuMI beam [PDF]
D. Cline, Young-Ho Seo, F. Sergiampietri
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On the neutrino and electron masses in the theory of scale relativity [PDF]
Laurent Nottale
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New evaluation of the axial nucleon form factor from electron- and neutrino-scattering data and impact on neutrino-nucleus cross sections [PDF]
G. D. Megias +3 more
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On the Electron-Neutrino Angular Correlation [PDF]
The electron· neutrino angular correlation functions are calculated for the allowed 'and first forbidden tramitions in the Fermi theory of beta decay taking into account the effect of the nuclear charge. The interferences which arise due to squaring of terms . in the interaction are worked out perfectly.
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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
Implication of the Steady State Equilibrium Condition for Electron-Positron Gas in the Neutrino-driven Wind from Proto-Neutron Star [PDF]
Liu Men-Quan, Ye‐Fei Yuan
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