The TeV Cosmic-Ray Anisotropy from Local Dark Matter Annihilation
  Several experiments have reported regions in the TeV sky with an excess of
cosmic rays. Here we consider the possibility that the excess cosmic rays are
coming from dark matter annihilation in nearby subhalos. We provide motivation
for dark matter as the source of the excess and show that dark matter
annihilations can naturally produce the cosmic ray anisotropy without the need
for exotic dark matter models. We show that viable dark matter explanations of
the cosmic ray excess are consistent with current measurements of antiprotons,
positrons, and gamma-rays. Additionally, we show that the dark matter
interpretation of the observed anisotropy predicts detections in several cosmic
ray channels by the next generation of experiments.
