Neutrino-deuteron reactions at solar neutrino energies
  In interpreting the SNO experiments, accurate estimates of the \nu d reaction cross sections are of great importance. In our recent work, we have improved our previous calculation by updating some of its inputs and by incorporating the results of a recent effective-field-theoretical calculation. The new cross sections are slightly (\sim 1%) larger than the previously reported values. It is reasonable to assign 1% uncertainty to the \nu d cross sections reported here; this error estimate does not include radiative corrections. 
S. Nakamura (1), T. Sato (1,2), S. Ando (2), T.-S. Park (2), F. Myhrer   (2), V. Gudkov (2), K. Kubodera (2) ((1)Osaka Unive...