Properties of a deformed Myers-Perry black hole
General Relativity and Quantum Cosmology
2025-09-17 v1
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.
Keywords
Cite
@article{arxiv.2509.13050,
title = {Properties of a deformed Myers-Perry black hole},
author = {Shohreh Abdolrahimi and Matin Tavayef},
journal= {arXiv preprint arXiv:2509.13050},
year = {2025}
}