“…Neutrino non-standard interactions (NSI) were originally proposed [1] as a mechanism to produce neutrino flavour conversion in matter and considered as a possible explanation for the solar and atmospheric neutrino deficits [1,2,3,4,5,6,7,8,9]. Although it is now clear that such NSI cannot fully account for the observed neutrino flavour conversion, the increasing sensitivity of neutrino oscillation experiments to sub-leading effects has triggered a new interest in them and their interference with neutrino oscillations at present (e.g., K2K, MINOS, OPERA [10,11,12,13,14,15,16,17]) and future (e.g., SuperBeams, βBeams or Neutrino Factories [18,19,20,21,22,23,24,25,26,27,28,29,30]) facilities. In particular, the determination of the leptonic mixing angle θ 13 could be severely affected by degeneracies with the non-standard parameters [31,32,33].…”