Abstract
In this work, starting from a spherically symmetric scale-dependent black hole, a rotating solution is obtained by following the Newman–Janis algorithm without complexification. Besides studying the horizon, the static conditions and causality issues of the rotating solution, we get and discuss the shape of its shadow.
- Received 25 June 2019
- Revised 6 November 2019
- Accepted 29 February 2020
DOI:https://doi.org/10.1103/PhysRevD.101.064053
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