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- W3105223837 endingPage "046" @default.
- W3105223837 startingPage "046" @default.
- W3105223837 abstract "In this paper, the shadows cast by non-rotating and rotating modified gravity black holes are investigated. In addition to the black hole spin parameter $a$ and the inclination angle $theta$ of observer, another parameter $alpha$ measuring the deviation of gravitational constant from the Newton one is also found to affect the shape of the black hole shadow. The result shows that, for fixed values of $a/M$ and $theta$, the size and perimeter of the shadows cast by the non-rotating and rotating black holes significantly increase with the parameter $alpha$, while the distortions decrease with $alpha$. Moreover, the energy emission rate of the black hole in high energy case is also investigated, and the result shows that the peak of the emission rate decreases with the parameter $alpha$." @default.
- W3105223837 created "2020-11-23" @default.
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- W3105223837 date "2019-03-29" @default.
- W3105223837 modified "2023-10-17" @default.
- W3105223837 title "Shadows of Kerr-like black holes in a modified gravity theory" @default.
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- W3105223837 doi "https://doi.org/10.1088/1475-7516/2019/03/046" @default.
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