Introduction to Black Hole Physics

By Valeri P. Frolov, A. Zelnikov. 2011

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Gravitational Lensing in Presence of Plasma: Strong Lens Systems, Black Hole Lensing and Shadow (2017, background): “Numerous analytical investigations and numerical simulations of the shadow are presented in literature (for example, see [90, 101, 95, 85, 86, 103, 104, 105, 94, 98, 99, 91, 106, 102, 97, 87, 88, 89, 93, 92, 96, 100, 110, 107, 108, 109, 111]).”
Calculating black hole shadows: Review of analytical studies (2021, methodology): “For a collection of Kerr shadow curves with different spins and viewing angles we also refer, e.g., to Fig.8.15 of Frolov and Zelnikov [87], Fig.5 of Chan et al [95] and Fig.1 of Takahashi [96].”
Rotating black holes in 4D Einstein-Gauss-Bonnet gravity and its shadow (2020, background): “and that corresponds to the Kerr black hole surface gravity [76].”
Parameter estimation of hairy Kerr black holes from its shadow and constraints from M87* (2021, background): “Applications of shadow in unravelling the useful information regarding the near horizon features of gravity have aroused a flurry of activities in the analytical investigations, and numerical simulation of shadows for black holes in GR (Falcke et al. 2000; de Vries 2000; Shen et al. 2005; Yumoto et ”