“…Furthermore, many extensions of the standard model predict new, effective four-Fermi interactions involving neutrinos, on which we will focus in this paper. General phenomenological studies of these non-standard interactions (NSIs) have been conducted in [1,2,3,4,5,6,7,8], and specific models are discussed in [9,10]. After a work by Grossman [11], which pointed out the importance of NSIs for neutrino oscillation experiments, many authors have investigated their impact in the context of solar neutrinos [12,13,14,15], atmospheric neutrinos [16,17,18,19,20,21], conventional and upgraded neutrino beams [22,23,24,25,26,27,28], neutrino factories [8,23,29,30,31,32,33,34], beta beams [35], supernova neutrinos [36,37], cosmological relic neutrinos [38], e + e − colliders [39], neutrino-electron scattering [40], and neutrino-nucleus scattering [41,42].…”