Dependence of the WIMP Angular Kinetic-Energy Distribution on the Solar
  Galactic Orbital Velocity
  In this article, we study in a little more detail the angular kinetic-energy
distribution of halo Weakly Interacting Massive Particles (WIMPs) and consider
two simple modifications with the Solar Galactic orbital velocity in our Monte
Carlo simulations of the 3-dimensional WIMP velocity as the first trial of
future investigations on distinguishing models of the Galactic structure of
Dark Matter particles by using directional direct detection data.
