Properties of a deformed Myers-Perry black hole
摘要
Considering an exact solution of the five-dimensional vacuum Einstein equations, 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 a bumpy deformed black hole horizon feels the presence of the external sources. However, the ergosphere is oblivious to the presence of external sources.