This talk summarizes the results of recent calculations of how fluctuations within the solar medium can influence resonant neutrino oscillations within the sun. Although initial calculations pointed to helioseismic waves as possibly producing detectable effects, recent more careful calculations show this not to be true. Those features of fluctuations which maximize their influence on neutrino propagation are identified, and are likely to have implications for supernovae and the early universe
We argue that solar neutrino observations have to be sensitive to the effects of magnetohydrodynamic...
We investigate the solar neutrino problem assuming the simultaneous presence of MSW transitions in t...
Taking into account the stringent limits from helioseismology observations on possible matter densit...
This review has two parts. The first part summarizes the current observational constraints on fluctu...
Abstract: This review has two parts. The rst part summarizes the current observa-tional constraints ...
We study some implications on standard matter oscillations of solar neutrinos induced by a backgroun...
We study some implications on standard matter oscillations of solar neutrinos induced by a backgroun...
We study some implications on standard matter oscillations of solar neutrinos induced by a backgroun...
The Mikheyev-Smirnov-Wolfenstein (MSW) resonant neutrino oscillation mechanism is investigated for t...
The Mikheyev-Smirnov-Wolfenstein (MSW) resonant neutrino oscillation mechanism is investigated for t...
The Mikheyev-Smirnov-Wolfenstein (MSW) resonant neutrino oscillation mechanism is investigated for t...
We analyze how solar neutrino experiments could detect time fluctuations of the solar neutrino flux ...
The Sun is fueled by a series of nuclear reactions that produce the energy that makes it shine. Neut...
Assuming a nonvanishing neutrino magnetic moment, we investigate the consequences of the appearance ...
We investigate the solar neutrino problem assuming the simultaneous presence of MSW transitions in t...
We argue that solar neutrino observations have to be sensitive to the effects of magnetohydrodynamic...
We investigate the solar neutrino problem assuming the simultaneous presence of MSW transitions in t...
Taking into account the stringent limits from helioseismology observations on possible matter densit...
This review has two parts. The first part summarizes the current observational constraints on fluctu...
Abstract: This review has two parts. The rst part summarizes the current observa-tional constraints ...
We study some implications on standard matter oscillations of solar neutrinos induced by a backgroun...
We study some implications on standard matter oscillations of solar neutrinos induced by a backgroun...
We study some implications on standard matter oscillations of solar neutrinos induced by a backgroun...
The Mikheyev-Smirnov-Wolfenstein (MSW) resonant neutrino oscillation mechanism is investigated for t...
The Mikheyev-Smirnov-Wolfenstein (MSW) resonant neutrino oscillation mechanism is investigated for t...
The Mikheyev-Smirnov-Wolfenstein (MSW) resonant neutrino oscillation mechanism is investigated for t...
We analyze how solar neutrino experiments could detect time fluctuations of the solar neutrino flux ...
The Sun is fueled by a series of nuclear reactions that produce the energy that makes it shine. Neut...
Assuming a nonvanishing neutrino magnetic moment, we investigate the consequences of the appearance ...
We investigate the solar neutrino problem assuming the simultaneous presence of MSW transitions in t...
We argue that solar neutrino observations have to be sensitive to the effects of magnetohydrodynamic...
We investigate the solar neutrino problem assuming the simultaneous presence of MSW transitions in t...
Taking into account the stringent limits from helioseismology observations on possible matter densit...