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