A Solution of the solar neutrino problem
Jun, 199011 pages
Published in:
- Phys.Rev.Lett. 65 (1990) 2233-2235
Report number:
- IASSNS-AST-90/14
Citations per year
Abstract: (APS)
Comparison of the results from the Kamiokande neutrino-electron scattering experiment with those from the chlorine experiment and with solar models shows that the explanation of the solar-neutrino problem probably requires physics beyond the standard electroweak model with zero neutrino masses. The experimental results, including the shape of the electron-recoil energy spectrum measured by Kamiokande, are in excellent agreement with a nonadiabatic solution of the Mikheyev-Smirnov-Wulfenstein effect, yielding a neutrino mass difference of Δm2=1×10−8 sin−2ΘV eV2.- neutrino: solar
- model: solar
- neutrino nucleus: nuclear reaction
- chlorine
- neutrino electron: elastic scattering
- elastic scattering: neutrino electron
- energy spectrum: (electron)
- (electron): energy spectrum
- neutrino: flux
- flux: neutrino
References(16)
Figures(0)