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Shadow of a Kerr-like black hole

Farruh AtamurotovInstitute of Nuclear Physics, Ulughbek, Tashkent 100214, Uzbekistan
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Abstract The shadow of a Kerr-like black hole has been considered and it was shown that in addition to the specific angular momentum a , deformation parameter of Kerr-like space-time essentially deforms the shape of the black hole shadow. For a given value of the black hole spin parameter a , the presence of a deformation parameter ε reduces the shadow and enlarges its deformation with respect to the one in the Kerr space-time.

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