ThermodynamicPropertiesofNeutralRegularBlackHole SolutioninGeneralizedRastallGravity

In this paper, we propose to investigate the thermodynamics of the static and spherically symmetric regular black hole in a generalized Rastall gravity. Rastall gravity is a new theory of gravity which replaces energy-momentum conservation, present in the General Relativity (GR). However, instead of providing some range for the energy-momentum tensor. Studying thermodynamics of black holes in Rastall gravity enables us to see how this formalism modifies the usual understanding of classical notions and shed new light on the problems. Thus, in the present work we have concerned with black hole horizons, mass function, entropy, surface gravity, Hawking temperature through mathematical and graphical representation.