Normalization of the neutrino-deuteron cross section
Normalization of the neutrino-deuteron cross section
As is well known, the comparison of the solar neutrino fluxes measured in SuperKamiokande (SK) by $\ensuremath{\nu}{+e}^{\ensuremath{-}}\ensuremath{\rightarrow}\ensuremath{\nu}{+e}^{\ensuremath{-}}$ and in the Sudbury Neutrino Observatory (SNO) by ${\ensuremath{\nu}}_{e}+\stackrel{\ensuremath{\rightarrow}}{d}{e}^{\ensuremath{-}}+p+p$ can provide a ``smoking gun'' signature for neutrino oscillations as the solution to the solar neutrino puzzle. This occurs because SK has some sensitivity …