Gamma Rays, Electrons, Hard X-Rays, and the Central Parsec of the Milky
  Way
  The complex interplay of processes at the Galactic Center is at the heart of
numerous past, present, and (likely) future mysteries. We aim at a more
complete understanding of how spectra extending to >10 TeV result. We first
construct a simplified model to account for the peculiar energy and angular
dependence of the intense central parsec photon field. This allows for
calculating anisotropic inverse Compton scattering and mapping gamma-ray
extinction due to gamma gamma -> e^+ e^- attenuation. Coupling these with a
method for evolving electron spectra, we examine several clear and present
excesses, including the diffuse hard X-rays seen by NuSTAR and GeV gamma rays
by Fermi. We address further applications to cosmic rays, dark matter,
neutrinos, and gamma rays from the Center and beyond.
