Yukawa vs. Newton: gravitational forces in a cubic cosmological
  simulation box
  We study the behaviour of Yukawa and Newtonian gravitational forces in a
cubic box with fully periodic boundaries commonly encountered in N-body
simulations of the structure formation. Placing a single gravitating body at
the origin of coordinates, we reveal the scales at which non-negligible
deviation from the Yukawa law occurs when the Newtonian approximation is
employed. We discuss the results in terms of the corresponding physical
distances today as well as earlier, back at the matter-dominated stage.
Revisiting the problem for free boundaries, we also compare the periodic and
plain gravitational forces for Yukawa-type interactions.
