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

Thermodynamics and Phase Transition of Topological Dilatonic Lifshitz‐Like Black Holes