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| Format: | Preprint |
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2026
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| Online Access: | https://arxiv.org/abs/2602.07780 |
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| _version_ | 1866910015471747072 |
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| author | Chen, Wen-Xiang |
| author_facet | Chen, Wen-Xiang |
| contents | We investigate the possibility of photon halos (stable photon orbits) forming outside Schwarzschild-$f(R)$ black holes by analyzing null geodesics in these spacetimes. Using methods inspired by studies of spherical photon orbits around Kerr-Newman black holes, we derive conditions for the existence of such halos. We examine several f(R) gravity models, including quadratic, logarithmic, exponential, cubic, power-law, and hyperbolic forms, and find that multiple photon orbits -- both stable and unstable -- can appear outside the event horizon for certain parameter ranges. These additional orbits (halos) provide new insights into spacetime geometry and potential observational signatures of black holes in modified gravity. We present analytical expressions for the orbital radii, perform a numerical stability analysis, and discuss possible observational implications for black hole shadows. Our results indicate that while the standard Schwarzschild black hole admits only a single unstable light ring, Schwarzschild-$f(R)$ black holes can support an additional outer stable photon orbit (a halo) without triggering a black-hole bomb instability. This work deepens the understanding of photon-orbit structures in alternative theories of gravity and highlights how such effects could be detected through deviations in black hole shadow size or morphology. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2602_07780 |
| institution | arXiv |
| publishDate | 2026 |
| record_format | arxiv |
| spellingShingle | Existence of Halos Outside Schwarzschild-$f(R)$ Black Holes Chen, Wen-Xiang General Relativity and Quantum Cosmology We investigate the possibility of photon halos (stable photon orbits) forming outside Schwarzschild-$f(R)$ black holes by analyzing null geodesics in these spacetimes. Using methods inspired by studies of spherical photon orbits around Kerr-Newman black holes, we derive conditions for the existence of such halos. We examine several f(R) gravity models, including quadratic, logarithmic, exponential, cubic, power-law, and hyperbolic forms, and find that multiple photon orbits -- both stable and unstable -- can appear outside the event horizon for certain parameter ranges. These additional orbits (halos) provide new insights into spacetime geometry and potential observational signatures of black holes in modified gravity. We present analytical expressions for the orbital radii, perform a numerical stability analysis, and discuss possible observational implications for black hole shadows. Our results indicate that while the standard Schwarzschild black hole admits only a single unstable light ring, Schwarzschild-$f(R)$ black holes can support an additional outer stable photon orbit (a halo) without triggering a black-hole bomb instability. This work deepens the understanding of photon-orbit structures in alternative theories of gravity and highlights how such effects could be detected through deviations in black hole shadow size or morphology. |
| title | Existence of Halos Outside Schwarzschild-$f(R)$ Black Holes |
| topic | General Relativity and Quantum Cosmology |
| url | https://arxiv.org/abs/2602.07780 |