We construct the time dependent hadronic-leptonic radiation model for the high energy processes inside the pulsar wind nebulae (PWNe). This model is based on the hypothesis that heavy nuclei are efficiently accelerated in the vicinity of young pulsars. Different energy loss processes of nuclei and accelerated by them leptons are considered in order to obtain the equilibrium spectra of these particles inside the nebula at an arbitrary time after the pulsar formation. We calculate the multiwavelength spectra from specific PWNe expected from different lep-tonic and hadronic processes. From normalization of the calculated synchrotron spectrum to the observed spectrum at low energies, the expected TeV gamma-ray fluxes from a few PWNe are predicted and its possible detectability by the future TeV telescopes is discussed.
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