We use the Renormalization Group method to study the magnetic field influence on the Bose-Einstein condensation of interacting dilute magnons in three dimensional spin systems. We first considered a model with SU(2) symmetry (universality class ) and we obtain for the critical magnetic field a power law dependence on the critical temperature, . In the case of U(1) symmetry (universality class ) the dependence is different, and the magnetic critical field depends linearly on the critical temperature, . By considering a more relevant model, which includes also the system’s anisotropy, we obtain for the same symmetry class a dependence of the magnetic critical field on the critical temperature. We discuss these theoretical predictions of the renormalization group in connection with experimental results reported in the literature.

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