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We have developed a specifically tailored relativistic,radiation-hydrodynamics Lagrangian code, that enables us to simulate theevolution of the main observables (light curve, evolution of photosphericvelocity and temperature) in core-collapse supernova (CC-SN) events. The codefeatures, some simulations as well as the implications of our results inconnection with a possible "standardization" of the hydrogen-rich CC-SNe arebriefly discussed. The possible role of this code in the development of a"CC-SNe Laboratory" for describing the evolution of a CC-SN event in a"self-consistent" way (from the main sequence up to the post-explosive phases)from a model/data comparison of light curves and spectra is also addressed.

Radiation hydrodynamics of core-collapse supernovae: the "key" asset for a self-consistent modelling of these events