Abstract
In this paper, we have found a D-dimensional static and spherically symmetric charged black hole solution with the quintessence matter surrounding in the context of the massive gravity. We studied the horizon properties of this black hole solution, which depend crucially on the sign of the coupling parameters of the massive gravity. In addition, we investigated the black hole thermodynamics in details from the local and global viewpoints at which various thermodynamic quantities are computed. The thermodynamic stability and phase transition of the black hole are analyzed by studying the behavior of the heat capacity at constant normalization factor which is related to the energy density of the quintessence matter.
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