The Remnant of a Rotating Regular Black Hole from the Generalized Entropy in the Final Stage of Evaporation

We express the generalized entropy (GE) of the Hawking radiation in the final stage of an evaporating rotating regular black hole (BH) by writing the mass of the BH as $m_{\rm ext} + α$, where $m_{\rm ext}$ represents the mass at the extremal limit and $α$ is a parameter. Generally, entropy is non-n