We consider a wide class of solar models with mixed core. Most of these models can be excluded as the sound speed profile that they predict is in sharp disagreement with helioseismic constraints. All the remaining models predict (8)B and/or (7)Be neutrino fluxes of at least as large as those of SSMs. In conclusion, helioseismology shows that a mixed solar core cannot account for the neutrino deficit implied by the current solar neutrino experiments. (C) 1998 Elsevier Science B.V
The exclusion of astrophysical solution of the solar neutrino problem is reviewed and analysed. The ...
The present status of the solar neutrino problem is reviewed. The strongest motivation for new neutr...
International audienceSolar activity and helioseismology show the limitation of the standard solar m...
We consider a wide class of solar models with mixed core. Most of these models can be excluded as th...
INTRODUCTION The early attempts to explain the so-called solar neutrino problem, i.e., the discrepa...
Imposing a constraint of the sound-speed profile determined from helioseismology and updating the mi...
An inversion of the accurately measured frequencies of solar oscillations leads to a determination o...
The inside of the Sun is not directly accessible to observations. Nonetheless, it is possible to con...
Precise numerical standard solar models (SSMs) now agree with one another and with helioseismologica...
We consider the most general solar model, using the neutrino fluxes as free parameters constrained o...
Several decades of studies of solar neutrinos lead now to clear indications that oscillation between...
The neutrino fluxes calculated from 14 standard solar models published recently in refereed journals...
The interior of the sun is not directly accessible to observations. Nonetheless, it is possible to i...
Precise numerical standard solar models (SSMs) now agree with one another and with helio-seismologic...
We have used 4752 days of data collected by the Birmingham Solar Oscillations Network (BiSON) to det...
The exclusion of astrophysical solution of the solar neutrino problem is reviewed and analysed. The ...
The present status of the solar neutrino problem is reviewed. The strongest motivation for new neutr...
International audienceSolar activity and helioseismology show the limitation of the standard solar m...
We consider a wide class of solar models with mixed core. Most of these models can be excluded as th...
INTRODUCTION The early attempts to explain the so-called solar neutrino problem, i.e., the discrepa...
Imposing a constraint of the sound-speed profile determined from helioseismology and updating the mi...
An inversion of the accurately measured frequencies of solar oscillations leads to a determination o...
The inside of the Sun is not directly accessible to observations. Nonetheless, it is possible to con...
Precise numerical standard solar models (SSMs) now agree with one another and with helioseismologica...
We consider the most general solar model, using the neutrino fluxes as free parameters constrained o...
Several decades of studies of solar neutrinos lead now to clear indications that oscillation between...
The neutrino fluxes calculated from 14 standard solar models published recently in refereed journals...
The interior of the sun is not directly accessible to observations. Nonetheless, it is possible to i...
Precise numerical standard solar models (SSMs) now agree with one another and with helio-seismologic...
We have used 4752 days of data collected by the Birmingham Solar Oscillations Network (BiSON) to det...
The exclusion of astrophysical solution of the solar neutrino problem is reviewed and analysed. The ...
The present status of the solar neutrino problem is reviewed. The strongest motivation for new neutr...
International audienceSolar activity and helioseismology show the limitation of the standard solar m...