Boron abundance and solar neutrino spectrum distortion
نویسنده
چکیده
The presence of neutrinos from Boron decay in the flux observed on Earth is attested by the observation of their energy spectrum. Possible distortions of the spectrum investigated in current detectors are often interpreted in terms of evidence in favour or against various schemes of neutrino oscillations. We stress here that a distortion of the spectrum at high energies could also result from an increase in the ratio of neutrinos originating from (He+p) and B reactions. While a B neutrino depletion would contribute to this effect, an increase in the Hep contribution seems also needed to reproduce the preliminary data. Chercheur IISN. Directeur de recherches du FNRS.
منابع مشابه
Vacuum oscillations and the distorted solar neutrino spectrum observed by Superkamiokande
The excess of solar-neutrino events above 13 MeV that has been recently observed by Superkamiokande can be explained by vacuum oscillations (VO). If the boron neutrino flux is 20% smaller than the standard solar model (SSM) prediction and the chlorine signal is assumed 30% (or 3.5σ) higher than the measured one, there exists a VO solution that reproduces both the observed boron neutrino spectru...
متن کاملVacuum oscillations of solar neutrinos: correlation between spectrum distortion and seasonal variations
Long length vacuum oscillations solution of the solar neutrino problem is discussed. We show that there is a strict correlation between a distortion of the neutrino energy spectrum and an amplitude of seasonal variations of the neutrino flux. The slope parameter which characterizes a distortion of the recoil electron energy spectrum in the Super-Kamiokande experiment and the seasonal asymmetry ...
متن کاملVacuum oscillations and excess of high energy solar neutrino events observed in Superkamiokande
The excess of solar-neutrino events above 13 MeV that has been recently observed by Superkamiokande can be explained by the vacuum oscillation solution to the Solar Neutrino Problem (SNP). If the boron neutrino flux is 20% smaller than the standard solar model (SSM) prediction and the chlorine signal is assumed 30% (or 3.4σ) higher than the measured one, there exists a vacuum oscillation soluti...
متن کاملGlobal Analysis with SNO: Toward the Solution of the Solar Neutrino Problem
We perform a global analysis of the latest solar neutrino data including the Solar Neutrino Observatory (SNO) result on the CC−event rate. This result further favors the LMA MSW solution of the solar neutrino problem. The best fit values of parameters we find are: ∆m = (4.8− 5.0) · 10 eV, tan θ = 0.35− 0.38, fB = 1.08− 1.12, and fhep = 1− 4, where fB and fhep are the boron and hep− neutrino flu...
متن کاملDoe/er/40561-137-int94-13-02 Boron Neutrino Flux and the Msw Solution of the Solar Neutrino Problem
There are large uncertainties in the predictions of the boron neutrino ux from the Sun which cannot be considered as being of purely statistical origin. We treat the magnitude of this ux, B , as a parameter to be found from experiment. The properties of the MSW solution to the solar neutrino problem for diierent values of B are studied. Present data give the bounds: 0:38 < B = 0 B < 3:1 (2), wh...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
عنوان ژورنال:
دوره شماره
صفحات -
تاریخ انتشار 1998