We construct the time dependent radiation model for the pulsar wind nebulae(PWNe),assuming that leptons are accelerated in resonant scattering with heavy nuclei,which are injected into the nebula by the pulsar.We calculate the equilibrium spectra of these particles inside the nebula taking into account their radiation and adiabatic energy losses.The spectra of gamma-rays are compared with the observations of the PWNe emitting TeV 7-rays and predictions are made for the expected gamma-ray fluxes from other PWNe.Expected neutrino fluxes and neutrino event rates in a 1 km~2 neutrino detector from these nebulae are also calculated.It is found that only the Crab Nebula,and possibly the Vela nebula and MSH15-52,can produce detectable neutrino event rates.
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