The standard nuclear physics approach and effective field theory approach for calculations of neutrino–deuteron cross sections for the solar neutrino energies are considered. Their main features, the level of accuracy and problems to be addressed for further developments are discussed.
Published in Journal of Physics G: Nuclear and Particle Physics, Volume 29, Issue 11, 2003, pages 2597-2613.
Gudkov, V. and Kubodera, K. (2003). Solar neutrinos, SNO and neutrino-deuteron reactions. Journal of Physics G: Nuclear and Particle Physics, 29(11), 2597-2613. doi: 10.1088/0954-3899/29/11/011
© 2003 IOP Publishing Ltd.