Exploring the superwind mechanism for generating ultrahigh-energy cosmic
  rays using large-scale modeling of starbursts
  The Pierre Auger Collaboration has provided a compelling indication for a
possible correlation between the arrival directions of ultrahigh-energy cosmic
rays and nearby starburst galaxies. Herein we show how the latest large-scale
modeling of starburst galaxies is compatible with the cosmic rays producing the
anisotropy signal being accelerated at the terminal shock of superwinds.
