Results 71 to 80 of about 1,298,977 (255)
Shedding light on LMA-dark solar neutrino solution by medium baseline reactor experiments: JUNO and RENO-50 [PDF]
A bstractIn the presence of Non-Standard neutral current Interactions (NSI) a new solution to solar neutrino anomaly with cos 2θ12 < 0 appears. We investigate how this solution can be tested by upcoming intermediate baseline reactor experiments, JUNO and
P. Bakhti, Y. Farzan
semanticscholar +1 more source
History of Solar Neutrino Observations [PDF]
The first solar neutrino experiment led by Raymond Davis Jr. showed a deficit of neutrinos relative to the solar model prediction, referred to as the "solar neutrino problem" since the 1970s. The Kamiokande experiment led by Masatoshi Koshiba successfully observed solar neutrinos, as first reported in 1989.
arxiv
Solar neutrinos: Solar physics and neutrino physics [PDF]
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, D.N. Schramm, X. Shi
openaire +2 more sources
A road map to solar neutrino fluxes, neutrino oscillation parameters, and tests for new physics [PDF]
We analyze all available solar and related reactor neutrino experiments, as well as simulated future 7Be, p-p, pep, and ^8B solar neutrino experiments.
Bahcall, John N., Pena-Garay, Carlos
core +5 more sources
NEUTRINO-DRIVEN EXPLOSION OF A 20 SOLAR-MASS STAR IN THREE DIMENSIONS ENABLED BY STRANGE-QUARK CONTRIBUTIONS TO NEUTRINO–NUCLEON SCATTERING [PDF]
Interactions with neutrons and protons play a crucial role for the neutrino opacity of matter in the supernova core. Their current implementation in many simulation codes, however, is rather schematic and ignores not only modifications for the correlated
T. Melson+5 more
semanticscholar +1 more source
Solar Neutrinos Spectroscopy with Borexino Phase-II
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
Constraints on flavor-diagonal non-standard neutrino interactions from Borexino Phase-II
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
Measurements of the atmospheric neutrino flux by Super-Kamiokande: energy spectra, geomagnetic effects, and solar modulation [PDF]
A comprehensive study on the atmospheric neutrino flux in the energy region from sub-GeV up to several TeV using the Super-Kamiokande water Cherenkov detector is presented. The energy and azimuthal spectra of the atmospheric νe and νµ fluxes are measured.
K. Okumura
semanticscholar +1 more source
The interaction of neutrino transition magnetic dipole moments with magnetic fields can give rise to the phenomenon of neutrino spin-flavour precession (SFP).
Evgeny Akhmedov, Pablo Martínez-Miravé
doaj +1 more source
19 pages, 2 figures (available on request), Coral Gables talk, UPR ...
openaire +5 more sources