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Chaotic Shadows of Black Holes: A Short Review

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arxiv 2205.05855 v2 pith:ZO4O5P4B submitted 2022-05-12 gr-qc astro-ph.GA

classification gr-qcastro-ph.GA
keywords blackholeshadowsshadowphotonintroducereviewcalculation
verification ladder T0 review T1 audit T2 compute T3 formal
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We give a brief review on the formation and the calculation of black hole shadow. Firstly, we introduce the conception of black hole shadow and the current works on a variety of black hole shadows. Secondly, we present main methods of calculating photon sphere radius and shadow radius, and then explain how the photon sphere affect the boundary of black hole shadow. We review the analytical calculation for black hole shadows which have analytic expressions for shadow boundary due to the integrable photon motion system. And we introduce the fundamental photon orbits which can explain the patterns of black hole shadow shape. Finally, we review the numerical calculation of black hole shadows with the backward ray-tracing method, and introduce some chaotic black hole shadows with self-similar fractal structures. Since the gravitational waves from the merger of binary black holes have been detected, we introduce a couple of shadows of binary black holes, which all have the eyebrowlike shadows around the main shadows with the fractal structures. We discuss the invariant phase space structures of photon motion system in black hole space-time, and explain the formation of black hole shadow is dominated by the invariant manifolds of certain Lyapunov orbits near the fixed points.

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Geodesics and shadows of the spindle-deformed Kerr black hole

    gr-qc 2026-07 accept novelty 6.0 of 10

    In the spindle-deformed Kerr black hole, null geodesics separate at O(B²) while timelike do not; the deformation shifts the ISCO, can create an OSCO, and enlarges the shadow versus Kerr.

  2. Chaotic imprints of dark matter in extreme mass-ratio inspirals

    gr-qc 2026-02 reject novelty 4.0 of 10

    A toy model shows that adding a hand-made angle-dependent force to dark-matter spacetimes produces visual chaos and irregular numerical-Kludge waveforms, but the force is not a realistic dark-matter perturbation.

  3. Variation in the size of the Photon Sphere and Black Hole Shadow in the Modified Gravity

    gr-qc 2025-06 reject novelty 2.0 of 10

    In f(R) gravity, the photon sphere and shadow radii are scaled by 1/F and further modified by the constant curvature R_dS, changing their size relative to general relativity.

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