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The possibility to synthesize heavier superheavy elements in massive nucleireactions is strongly limited by the hindrance to complete fusion of reactingnuclei: due to the onset of the quasifission process in the entrance channel,which competes with complete fusion, and by strong increase of the fissionyield along the de-excitation cascade of the compound nucleus in comparison tothe evaporation residue formation. We present a wide and detailed procedureallowing us to describe the experimental results (evaporation residue nucleiand fissionlike products) in the mass asymmetric and symmetric reactions. Veryreliable estimations and perspectives for the synthesis of superheavy elementsin many massive nuclei reactions up to Z = 120 and eventually also for Z > 120have been obtained.

What perspectives for the synthesis of heavier superheavy nuclei? Results and comparison with models