Black hole shadow of a rotating scale--dependent black hole

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.

Accepted version. arXiv admin note: text overlap with arXiv:1905.11443

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