2023
DOI: 10.1140/epjc/s10052-023-11418-w
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Observable features of charged Kiselev black hole with non-commutative geometry under various accretion flow

Abstract: The light passing near the black hole (BH) is deflected due to the gravitational effect, producing the BH shadow, a dark inner region that is often surrounded by a bright ring, whose optical appearance comes directly from BH’s mass and its angular momentum. We mainly study the shadow and observable features of non-commutative (NC) charged Kiselev BH, surrounded by various profiles of accretions. To obtain the BH shadow profile, we choose specific values of the model parameters and concluded that the variations… Show more

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Cited by 8 publications
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