Radiating Kerr-like regular black hole

TL;DR

This paper derives a new radiating Kerr-like regular black hole solution using a complex transformation, extending regular black hole models to include radiation effects and analyzing horizon structures.

Contribution

It introduces a novel radiating Kerr-like regular black hole solution derived from the Hayward regular black hole using Newman-Janis transformation.

Findings

The solution reduces to Kerr and Kerr-like regular black holes in specific limits.

Horizon-like surface structures are characterized.

The model incorporates radiation into regular black hole metrics.

Abstract

We derive a radiating regular rotating black hole solution, radiating Kerr-like regular black hole solution. We achieve this by starting from the Hayward regular black hole solution via a complex transformation suggested by Newman-Janis. The radiating Kerr metric, the Kerr-like regular black hole and the standard Kerr metric are regained in the appropriate limits. The structure of the horizon-like surfaces are also determined.