Sub-MeV Bosonic Dark Matter, Misalignment Mechanism and Galactic Dark
  Matter Halo Luminosities
  We explore a scenario that the dark matter is a boson condensate created by
the misalignment mechanism, in which a spin 0 boson (an axion-like particle)
and a spin 1 boson (the dark photon) are considered, respectively. We find that
although the sub-MeV dark matter boson is extremely stable, the huge number of
dark matter particles in a galaxy halo makes the decaying signal detectable. A
galaxy halo is a large structure bounded by gravity with a typical
$\sim10^{12}$ solar mass, and the majority of its components are made of dark
matter. For the axion-like particle case, it decays via $\phi\to \gamma\gamma$,
therefore the photon spectrum is monochromatic. For the dark photon case, it is
a three body decay $A'\to\gamma\gamma\gamma$. However, we find that the photon
spectrum is heavily peaked at $M/2$ and thus can facilitate observation. We
also suggest a physical explanation for the three body decay spectrum by
comparing the physics in the decay of orthopositronium. In addition, for both
cases, the decaying photon flux can be measured for some regions of parameter
space using current technologies.
