<p>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.</p>

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Properties of a deformed Myers-Perry black hole

  • Shohreh Abdolrahimi,
  • Matin Tavayef

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.