The conversion of electron-neutrinos into muon-neutrinos within a star was recently proposed as a mechanism to explain the solar neutrino puzzle. We investigate the influence of density fluctuations on the conversion rate. Although the corrections can become large for suitable choices of parameters they are probably negligible for the sun
We consider the implications of solar matter density random noise upon resonant neutrino conversion....
We consider the effect on matter-enhanced neutrino flavor transformation of a randomly fluctuating, ...
The study of solar neutrinos has given since ever a fundamental contribution both to astroparticle a...
In this work we study the phenomenological consequences of the dependence of mass varying neutrinos ...
15 pages, 4 figures; final version: typos corrected, references added, matches published versionInte...
There are reasons to believe that the solar matter density fluctuates around an equilibrium profile....
I review the standard solar model, the disparities between its predictions and the solar neutrino fl...
A number of experiments have accumulated over the years a large amount of solar neutrino data. The d...
We propose that the solar neutrino deficit may be due to oscillations of mass-varying neutrinos (MaV...
What can we learn from solar neutrino observations? Is there any solution to the solar neutrino anom...
The Mikheyev-Smirnov-Wolfenstein (MSW) resonant neutrino oscillation mechanism is investigated for t...
The status of solar neutrino experiments and their implications for both nonstandard astrophysics ({...
Mikheyev and Smirnov have shown that the interactions of neutrinos with matter can result in the con...
Density and temperature conditions in the solar core suggest that the microscopic diffusion of elect...
Effects of the dense matter can induce the neutrino decay even if neutrinos are stable in vacuum. Th...
We consider the implications of solar matter density random noise upon resonant neutrino conversion....
We consider the effect on matter-enhanced neutrino flavor transformation of a randomly fluctuating, ...
The study of solar neutrinos has given since ever a fundamental contribution both to astroparticle a...
In this work we study the phenomenological consequences of the dependence of mass varying neutrinos ...
15 pages, 4 figures; final version: typos corrected, references added, matches published versionInte...
There are reasons to believe that the solar matter density fluctuates around an equilibrium profile....
I review the standard solar model, the disparities between its predictions and the solar neutrino fl...
A number of experiments have accumulated over the years a large amount of solar neutrino data. The d...
We propose that the solar neutrino deficit may be due to oscillations of mass-varying neutrinos (MaV...
What can we learn from solar neutrino observations? Is there any solution to the solar neutrino anom...
The Mikheyev-Smirnov-Wolfenstein (MSW) resonant neutrino oscillation mechanism is investigated for t...
The status of solar neutrino experiments and their implications for both nonstandard astrophysics ({...
Mikheyev and Smirnov have shown that the interactions of neutrinos with matter can result in the con...
Density and temperature conditions in the solar core suggest that the microscopic diffusion of elect...
Effects of the dense matter can induce the neutrino decay even if neutrinos are stable in vacuum. Th...
We consider the implications of solar matter density random noise upon resonant neutrino conversion....
We consider the effect on matter-enhanced neutrino flavor transformation of a randomly fluctuating, ...
The study of solar neutrinos has given since ever a fundamental contribution both to astroparticle a...