which has $c=1$.\
In this paper we consider the holographic entanglement entropy for one or two strips in the boundary theory in presence of various types of black holes with non compact horizon in the bulk. For one strip, we focus on the divergence of the finite term when the strip becomes large and therefore the turning point of the minimal surface approaches the horizon. The degree of this divergence depends on the near horizon geometry, but the finite term scales like the width (and thus like the volume) of the strip for all the black holes we consider. This scaling is broken for the Lifshitz type backgrounds whose dynamical exponent occurs in the spatial part of the metric.\
For two parallel strips of equal width we mainly consider the transition of the mutual information in terms of the geometrical parameters, namely the width of the strips and the distance between them. For the charged black hole in four dimensions with fixed charge, we find that the transition of the mutual information leads to a characteristic finite distance between the strips as they become large. This distance depends on the temperature and it could be interpreted as a signal of 