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.
CITATION STYLE
Ghosh, S. G., & Maharaj, S. D. (2015). Radiating Kerr-like regular black hole. European Physical Journal C, 75(1). https://doi.org/10.1140/epjc/s10052-014-3222-7
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