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We review a proposed multicomponent model to explain the features of thepulsed emission and spectrum of the Crab Pulsar, on the light of the recentdetection of pulsed emission above 25 GeV from the MAGIC atmospheric Cherenkovtelescope. This model explains the evolution of the pulse shape and of thephase-resolved spectra, ranging from the optical/UV to the GeV energy band, onthe assumption that the observed emission is due to several components, whichhave spectra modelled as log-parabolic laws. We show that the new MAGIC dataare well consistent with the prevision of our model.

The multicomponent model of the Crab Pulsar at energies above 25 GeV