Redefining Black Hole Entropy due to Proportionality to the Fine Structure Constant

In this article we propose a new definition of the entropy of black holes. For this we base ourselves on a reformulation of the Hawking-Bekenstein formula in such a way that, on the one hand, by introducing a new variable that represents the number of microstates and On the other hand, taking into account the mass of the black hole, we can conclude a new equation for the entropy of black holes.