  In this work we consider a spacial kind of spacetime called AdS accelerating
black holes. This is a kind of black holes which contain a stringlike
singularity along polar axises attached to the black hole and it accelerates
the black hole. In these kind of spacetimes the growth of Einstein-Hilbert
action is independent of the acceleration as found in the previous works.
  By using a string as a probe, we found the effect of the acceleration is
captured by the string prove in our previous work. Here in this work we
consider the case of rotating black holes. By the prove string we clearly
describe the effect of the acceleration and its relation to the rotation of the
black holes.
