  It is known that scalar-tensor gravity models can be studied in Einstein and
Jordan frames. In this paper, we consider a model of scalar-tensor gravity in
Einstein's frame to calculate the Lifshitz-like black hole solutions with
different horizon topologies. We study thermodynamic properties and first order
van der Waals like phase transition, and find that the Lifshitz parameter
affects the phase structure. In addition, we investigate thermal stability by
using the behavior of heat capacity and various methods of geometrical
thermodynamics.
