Abstract
In this paper, we study the Tours-like black hole solution in the regularized self-energy of the electrostatic field in the context of thermodynamics, energy emission, and Gibbs free energy. For this purpose, we calculate the Hawking temperature, and heat capacity, as well as the local and global thermodynamic stability of the black hole. We calculate the mass of the black hole by using the first law of thermodynamics and also compute the energy emission rate and show that the emission rate is proportional to the zero-point length parameter. We calculate the Gibbs free energy to discuss the phase transition of regularly charged torus-like black holes. It is considered that the length scale parameter represents the thermodynamic pressure and the effects of pressure, charge, and zero point length on the thermodynamic properties.
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