“…This is the basis of the SuSA model [1], which exploits the scaling and superscaling properties exhibited by electron scattering data in order to predict neutrino-nucleus observables. In its more recent version, SuSAv2 [2], the model also takes into account the behavior of the responses provided by the Relativistic Mean Field (RMF): in particluar, the natural enhancement of the transverse electromagnetic response provided by RMF, a genuine dynamical relativistic effect, is incorporated in the SuSAv2 approach. However, while the RMF approach works properly at low to intermediate values of the momentum transfer q, where the effects linked to the treatment of the final-state interactions (FSI) are significant, it fails at higher q due to the strong energy-independent scalar and vector RMF potentials, whose effects should instead become less and less important with increasing momentum transfer.…”