Results 1 to 10 of about 24,655 (229)
Two-Loop Neutrino Masses and the Solar Neutrino Problem [PDF]
The addition of $m$ singlet right-handed neutrinos to the Standard Model leads to radiatively generated mass corrections for the $SU(2)_L $ doublet neutrinos.
A. B. Lahanes +31 more
core +9 more sources
The Simplest Resonant Spin--Flavour Solution to the Solar Neutrino Problem [PDF]
We re-analyse the resonant spin-flavour (RSF) solutions to the solar neutrino problem in the framework of analytic solutions to the solar magneto-hydrodynamics (MHD) equations.
Akhmedov +57 more
core +4 more sources
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 ...
Shibahashi, Hiromoto, Watanabe, Satoru
core +5 more sources
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
doaj +1 more source
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
core +2 more sources
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

