  The surface density $\Sigma$-map and the convergence $\kappa$-map of Bullet
Cluster 1E0657-558 show that the center of baryonic matters separates from the
center of gravitational force, and the distribution of gravitational force do
not possess spherical symmetry. This hints that a modified gravity with
difference to Newtonian inverse-square law at large scale, and less symmetry is
worth investigating. In this paper, we study the dynamics in Randers-Finsler
spacetime. The Newtonian limit and gravitational deflection of light in a
Rindler-type potential is focused in particular. It is shown that the
convergence in Finsler spacetime could account for the observations of Bullet
Cluster.
