4.6 Article

Shadow casted by a Konoplya-Zhidenko rotating non-Kerr black hole

出版社

IOP PUBLISHING LTD
DOI: 10.1088/1475-7516/2017/10/051

关键词

astrophysical black holes; gravity

资金

  1. Hunan Provincial Education Department [17A124]
  2. National Natural Science Foundation of China [11475061]

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We have investigated the shadow of a Konoplya-Zhidenko rotating non-Kerr black hole with an extra deformation parameter. The spacetime structure arising from the deformed parameter affects sharply the black hole shadow. With the increase of the deformation parameter, the size of the shadow of black hole increase and its shape becomes more rounded for arbitrary rotation parameter. The D-shape shadow of black hole emerges only in the case a < 2 root 3/3 M with the proper deformation parameter. Especially, the black hole shadow possesses a cusp shape with small eye lashes in the cases with a > M, and the shadow becomes less cuspidal with the increase of the deformation parameter. Our result show that the presence of the deformation parameter yields a series of significant patterns for the shadow casted by a Konoplya-Zhidenko rotating non-Kerr black hole.

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