We investigate the consequences of the acceleration of heavy nuclei (e.g., iron nuclei) by the Crab pulsar. Accelerated nuclei can photodisintegrate in collisions with soft photons produced in the pulsar's outer gap, injecting energetic neutrons which decay either inside or outside the Crab nebula. The protons from neutron decay inside the nebula accumulate, producing gamma rays and neutrinos in collisions with the matter in the nebula. Neutrons decaying outside contribute to the galactic cosmic rays. We compute the expected fluxes of gamma rays and neutrinos, and find that our model could account for the observed emission at high energies and may be tested by searching for high energy neutrinos with future neutrino telescopes currently in the design stage.

• Received 7 April 1997

DOI:https://doi.org/10.1103/PhysRevLett.79.2616