Phase transition of charged black holes in massive gravity through new methods

摘要: Motivated by providing preliminary steps to understand the conception of quantum gravity, in this paper, we study phase structure a semiclassical gravitational system. We investigate stability conditions and transition charged black holes massive gravity via canonical ensemble geometrical thermodynamic approaches. point out effects parameter on these show how coefficients affect points holes. also boundary topology thermodynamical behavior In addition, give some arguments regarding role higher dimensions highlight effect electric charge behavior. Then, extend our approach that it can be successful method for studying hole transition. At last, employing relation between pressure cosmological constant, critical system different parameters values are investigated.