Constraints on Cosmological Dark Matter Annihilation from the Fermi-LAT
  Isotropic Diffuse Gamma-Ray Measurement
  The first published Fermi large area telescope (Fermi-LAT) measurement of the
isotropic diffuse gamma-ray emission is in good agreement with a single power
law, and is not showing any signature of a dominant contribution from dark
matter sources in the energy range from 20 to 100 GeV. We use the absolute size
and spectral shape of this measured flux to derive cross section limits on
three types of generic dark matter candidates: annihilating into quarks,
charged leptons and monochromatic photons. Predicted gamma-ray fluxes from
annihilating dark matter are strongly affected by the underlying distribution
of dark matter, and by using different available results of matter structure
formation we assess these uncertainties. We also quantify how the dark matter
constraints depend on the assumed conventional backgrounds and on the
Universe's transparency to high-energy gamma-rays. In reasonable background and
dark matter structure scenarios (but not in all scenarios we consider) it is
possible to exclude models proposed to explain the excess of electrons and
positrons measured by the Fermi-LAT and PAMELA experiments. Derived limits also
start to probe cross sections expected from thermally produced relics (e.g. in
minimal supersymmetry models) annihilating predominantly into quarks. For the
monochromatic gamma-ray signature, the current measurement constrains only dark
matter scenarios with very strong signals.
