Neutrino-deuteron reactions at solar neutrino energies
  In interpreting the SNO experiments, very accurate estimates of the \nu d reaction cross sections are of great importance. We improve the previous estimates of our group by updating some of its inputs and by taking into account the results of a recent effective-field-theoretical calculation. The new cross sections are slightly (\sim 1%) larger than the previously reported values. We present arguments that lead to the conclusion that it is reasonable to assign 1% uncertainty to the \nu d cross sections reported here. 
S. Nakamura (1), T. Sato (1 and 2), S. Ando (2), T.-S. Park (2), F.   Myhrer (2), V. Gudkov (2) and K. Kubodera (2) ((1) Osa...