Properties of a deformed Myers-Perry black hole
Published: Sep 16, 2025
Last Updated: Sep 16, 2025
Authors:Shohreh Abdolrahimi, Matin Tavayef
Abstract
Considering an exact solution of the five-dimensional Einstein equations in vacuum space, which represents a distorted Myers-Perry black hole with a single angular momentum, we investigate how the distortion affects the horizon surface of this black hole. We illustrate a special case where we have a bumpy deformed black hole horizon that feels the presence of the external sources. However, the ergosphere is oblivious to the presence of external sources.