Results 41 to 50 of about 1,191,896 (269)

Neutrino masses and solar neutrinos [PDF]

open access: yesPhysical Review D, 1992
It has been pointed out by Bahcall and Bethe and others that all solar-neutrino data can be explained by Mikheyev-Smirnov-Wolfenstein oscillations with $m({\ensuremath{\nu}}_{\ensuremath{\mu}})\ensuremath{\sim}{10}^{\ensuremath{-}3}$ eV consistent with ideas of grand unified theories (GUT's).
openaire   +2 more sources

Solar neutrinos: Solar physics and neutrino physics [PDF]

open access: yesNuclear Physics B - Proceedings Supplements, 1994
Abstract It is shown that the current solar neutrino situation, with results from the Homestake experiment, the Kamiokande experiment, GALLEX and SAGE is unfortunately still ambiguous. The differences between observations and the standard solar theory may still be due to either astrophysical inputs or new neutrino physics.
D.N. Schramm, X. Shi
openaire   +1 more source

Neutrino oscillation anomalies [PDF]

open access: yesEPJ Web of Conferences, 2023
I give an overview of some of the several anomalies appearing in neutrino oscillation experiments, setting particular focus to the reactor antineutrino anomaly and the Gallium anomaly. I will discuss these two anomalies in some detail and, in particular,
Ternes Christoph Andreas
doaj   +1 more source

Solar neutrino detection in a large volume double-phase liquid argon experiment [PDF]

open access: yes, 2015
Precision measurements of solar neutrinos emitted by specific nuclear reaction chains in the Sun are of great interest for developing an improved understanding of star formation and evolution.
D. Franco   +36 more
semanticscholar   +1 more source

NuFIT: Three-Flavour Global Analyses of Neutrino Oscillation Experiments [PDF]

open access: yesUniverse, 2021
In this contribution, we summarise the determination of neutrino masses and mixing arising from global analysis of data from atmospheric, solar, reactor, and accelerator neutrino experiments performed in the framework of three-neutrino mixing and ...
M. Gonzalez-Garcia   +2 more
semanticscholar   +1 more source

Recent results from Borexino on solar neutrinos [PDF]

open access: yesEPJ Web of Conferences, 2023
Borexino has been a neutrino detector based on ultrapure liquid scintillator, located at the Laboratori Nazionali del Gran Sasso, Italy. Its main scientific goal was the real-time measurement of solar neutrino fluxes, which play an irreplaceable role for
Basilico D.   +79 more
doaj   +1 more source

ecCNO solar neutrinos: A challenge for gigantic ultra-pure liquid scintillator detectors

open access: yesPhysics Letters B, 2015
Neutrinos produced in the Sun by electron capture reactions on 13N, 15O and 17F, to which we refer as ecCNO neutrinos, are not usually considered in solar neutrino analysis since the expected fluxes are extremely low.
F.L. Villante
doaj   +1 more source

Constraints on flavor-diagonal non-standard neutrino interactions from Borexino Phase-II

open access: yesJournal of High Energy Physics, 2020
The Borexino detector measures solar neutrino fluxes via neutrino-electron elastic scattering. Observed spectra are determined by the solar-ν e survival probability P ee (E), and the chiral couplings of the neutrino and electron. Some theories of physics
The Borexino collaboration   +106 more
doaj   +1 more source

DARWIN – a next-generation liquid xenon observatory for dark matter and neutrino physics [PDF]

open access: yesInternational Conference on Rebooting Computing, 2021
The nature of dark matter and properties of neutrinos are among the most pressing issues in contemporary particle physics. The dual-phase xenon time-projection chamber is the leading technology to cover the available parameter space for weakly ...
J. Aalbers   +499 more
semanticscholar   +1 more source

Solar Neutrinos Spectroscopy with Borexino Phase-II

open access: yesUniverse, 2018
Solar neutrinos have played a central role in the discovery of the neutrino oscillation mechanism. They still are proving to be a unique tool to help investigate the fusion reactions that power stars and further probe basic neutrino properties.
Lino Miramonti   +109 more
doaj   +1 more source

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