We use the suite of Milky Way-like galaxies in Auriga simulations to determine contribution annihilation radiation from dark matter subhalos three velocity-dependent models: Sommerfeld, p-wave, and d-wave models. compare these corresponding distribution velocity-independent s-wave model. For both hydrodynamical dark-matter-only simulations, only case Sommerfeld-enhanced does total flux exceed s...

Dynamic perturbations of reaching movements are an important technique for studying motor learning and adaptation. Adaptation to non-contacting, velocity-dependent inertial Coriolis forces generated by arm movements during passive body rotation is very rapid, and when complete the Coriolis forces are no longer sensed. Adaptation to velocity-dependent forces delivered by a robotic manipulandum t...