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.
| Original language | English |
|---|---|
| Article number | 064053 |
| Journal | Physical Review D |
| Volume | 101 |
| Issue number | 6 |
| DOIs | |
| State | Published - 2020 |
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