Chaos and fractals of the black hole photon ring
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arXiv
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| Main Authors: | , , , , |
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| Format: | Preprint |
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2026
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| _version_ | 1866914380628623360 |
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| author | Berens, Roman Galison, Peter Gravely, Trevor Lupsasca, Alexandru Stein, Leo C. |
| author_facet | Berens, Roman Galison, Peter Gravely, Trevor Lupsasca, Alexandru Stein, Leo C. |
| contents | The photon ring of a Kerr black hole decomposes into a self-similar hierarchy of subrings. Here, we show that this self-similar structure persists in phase space. Moreover, near the photon shell of bound photon orbits, dynamics are controlled by a Lyapunov exponent $γ$, whose role we highlight by computing the first-return map for light rays close to an unstably bound orbit. Despite an exponential $e^γ$ sensitivity to initial conditions, nearly bound rays do not exhibit chaotic behavior. However, as the background spacetime is deformed away from the Kerr geometry, chaos sets in, with its first onset most visible near strongly resonant bound orbits in the photon shell. We display two animations: one illustrating the emergence of chaos near the photon shell, which results in a fractal phase-space structure, and another exhibiting how this chaotic, fractal, self-similar structure is encoded in the first-return map. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2603_08790 |
| institution | arXiv |
| publishDate | 2026 |
| record_format | arxiv |
| spellingShingle | Chaos and fractals of the black hole photon ring Berens, Roman Galison, Peter Gravely, Trevor Lupsasca, Alexandru Stein, Leo C. General Relativity and Quantum Cosmology Chaotic Dynamics The photon ring of a Kerr black hole decomposes into a self-similar hierarchy of subrings. Here, we show that this self-similar structure persists in phase space. Moreover, near the photon shell of bound photon orbits, dynamics are controlled by a Lyapunov exponent $γ$, whose role we highlight by computing the first-return map for light rays close to an unstably bound orbit. Despite an exponential $e^γ$ sensitivity to initial conditions, nearly bound rays do not exhibit chaotic behavior. However, as the background spacetime is deformed away from the Kerr geometry, chaos sets in, with its first onset most visible near strongly resonant bound orbits in the photon shell. We display two animations: one illustrating the emergence of chaos near the photon shell, which results in a fractal phase-space structure, and another exhibiting how this chaotic, fractal, self-similar structure is encoded in the first-return map. |
| title | Chaos and fractals of the black hole photon ring |
| topic | General Relativity and Quantum Cosmology Chaotic Dynamics |
| url | https://arxiv.org/abs/2603.08790 |