  The neutrino-nucleus reactions are studied at energies from 0 to 3 GeV, using
the CRISP program. To simulate these reactions, CRISP uses the Monte Carlo
method through an intranuclear cascade model. Quase-elastic and baryonic
resonance formation channels for the neutrino-nucleon interaction are
considered. The total and differential particle emission cross-sections were
obtained, obtaining a good agreement with the values reported by the MiniBooNE
experiment. The influence of nuclear effects on the studied reactions, such as
fermionic motion, the Pauli blocking mechanism, and the nucleonic separation
energy, was shown. It was not possible to simultaneously reproduce the $\nu_\mu
+ D$ and $\nu_\mu + ^{12}C$ reactions using the same axial mass value. For the
charged current quasi-elastic channel, $M_A = 0.95 \ GeV$ for the $\nu_\mu + D$
reaction, and $M_A = 1.35 \ GeV$ for the $\nu_\mu + ^{12}C$ reaction. This can
be solved if one considers, in addition to the neutrino-nucleon interaction,
the neutrino interaction with a pair of nucleons, just as we demonstrate in the
last part of this work.
