Ultra-high-energy cosmic rays from young neutron star winds

The long-held notion that the highest energy cosmic rays are of distant ext ragalactic origin is challenged by observations that events above similar t o 10(20) eV do not exhibit the expected high-energy cutoff from photopion p roduction off the cosmic microwave background. We suggest that these unexpe cted ultra-high-energy events are due to iron nuclei accelerated from young strongly magnetized neutron stars through relativistic MHD winds. We find that neutron stars whose initial spin periods are shorter than similar to 1 0 ms and whose surface magnetic fields are in the 10(12)-10(14) G range can accelerate iron cosmic rays to greater than similar to 10(20) eV. These io ns can pass through the remnant of the supernova explosion that produced th e neutron star without suffering significant spallation reactions or energy loss. For plausible models of the Galactic magnetic field, the trajectorie s of the iron ions curve sufficiently to be consistent with the observed, l argely isotropic arrival directions of the highest energy events.