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Current status of the resonant spin-flavor precession solution to the solar neutrino problem [PDF]
We discuss the current status of the resonant spin-flavor precession (RSFP) solution to the solar neutrino problem. We perform a fit to all the latest solar neutrino data for various assumed magnetic field profiles in the sun.
M. M. Guzzo, H. Nunokawa
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Solar Models with Helioseismic Constraints and the Solar Neutrino Problem [PDF]
Imposing a constraint of the sound-speed profile determined from helioseismology and updating the microphysics, we have revised our seismic solar model, constructed with the assumption of a homogeneous metal abundance distribution, and have shown that ...
Satoru Watanabe, Hiromoto Shibahashi
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MSW mediated neutrino decay and the solar neutrino problem [PDF]
We investigate the solar neutrino problem assuming simultaneous presence of MSW transitions in the sun and neutrino decay on the way from sun to earth.
Abhijit Bandyopadhyay +2 more
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The Relevance of Nuclear Reactions for Standard Solar Models Construction
The fundamental processes by which nuclear energy is generated in the Sun have been known for many years. However, continuous progress in areas such as neutrino experiments, stellar spectroscopy and helioseismic data and techniques requires ever more ...
Francesco L. Villante +3 more
doaj +1 more source
We evaluate the statistical significance of the 3+1 sterile-neutrino hypothesis using ν e and ν ¯ $$ \overline{\nu} $$ e disappearance data from reactor, solar and gallium radioactive source experiments.
Jeffrey M. Berryman +4 more
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Implications of the Dark-LMA solution for neutrino mass matrices
In this work we have re-investigated two different kinds of texture zero ansatz of the low energy neutrino mass matrix in view of the Dark-Large-Mixing-Angle (DLMA) solution of the solar neutrino problem which can arise in the presence of non-standard ...
Monojit Ghosh +2 more
doaj +1 more source
Neutrinos and Asteroseismology of Stars over the Helium Flash
The helium flash, occurring in stars of 0.6–2.0 M _⊙ at the end of the red giant branch, is not observable via optical means due to the energy of the process being used to lift the core out of degeneracy.
Diogo Capelo, Ilídio Lopes
doaj +1 more source
Is bi-maximal mixing compatible with the large angle MSW solution of the solar neutrino problem? [PDF]
It is shown that the large angle MSW solution of the solar neutrino problem with a bi-maximal neutrino mixing matrix implies an energy-independent suppression of the solar nu_e flux.
A.J. Baltz +27 more
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Standard Solar Neutrinos [PDF]
An improved standard solar model has been used to calculate the fluxes of standard solar neutrinos. It includes premain sequence evolution, element diffusion, partial ionization effects, and all the possible nuclear reactions between the main elements ...
Anders +47 more
core +2 more sources
Constraints on decay plus oscillation solutions of the solar neutrino problem [PDF]
We examine the constraints on non-radiative decay of neutrinos from the observations of solar neutrino experiments. The standard oscillation hypothesis among three neutrinos solves the solar and atmospheric neutrino problems.
A. Acker +31 more
core +2 more sources

