  We present a numerical model for the extended steep-spectrum radio sources
and the elongated X-ray structure in A3667 based on new 3-dimensional
MHD/N-body simulations. The X-ray and optical analyses of A3667 indicate that
it has undergone a recent subcluster merger event. We believe that the
Mpc-scale radio sources identified in A3667 are also a consequence of the
merger. Our previous numerical simulations show that mergers often produce
large-scale shocks and turbulence capable of both magnetic field amplification
and in-situ reacceleration of relativistic particles. Our model suggests that
these radio structures, separated by ~2.6 h^{-1}_100 Mpc, are in fact causally
linked via a slightly off-axis merger that occurred nearly in the plane of the
sky approximately 1 Gyr ago with a subcluster having a total mass equal to ~20%
of the primary cluster.
