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Superentropic AdS black hole shadows

A. BelhajDépartement de Physique, Equipe des Sciences de la matière et du rayonnement, ESMaR, Faculté des Sciences, Université Mohammed V de Rabat, Rabat, MoroccoH. BelmahiDépartement de Physique, Equipe des Sciences de la matière et du rayonnement, ESMaR, Faculté des Sciences, Université Mohammed V de Rabat, Rabat, MoroccoM. BenaliDépartement de Physique, Equipe des Sciences de la matière et du rayonnement, ESMaR, Faculté des Sciences, Université Mohammed V de Rabat, Rabat, Morocco
2021en
ABI

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We study shadow aspects of superentropic black holes in four dimensions. Using Hamilton-Jacobi formalism, we first get the null geodesic equations. In the celestial coordinate framework relying on with fixed positions of observers, we investigate the shadow behaviors in terms of the mass and the cosmological scale variation parameters. Among others, we obtain ellipse shaped geometries contrary to usual black hole solutions. Modifying the ordinary relations describing geometrical observables, we discuss the size and the shape deformation parameters of these non-trivial geometric forms. Due to horizonless limits associated whit certain mass values, we explore the shadow of the naked singularity of such black holes.

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