Reuse & Permissions

It is not necessary to obtain permission to reuse this article or its components as it is available under the terms of the Creative Commons Attribution 4.0 International license. This license permits unrestricted use, distribution, and reproduction in any medium, provided attribution to the author(s) and the published article's title, journal citation, and DOI are maintained. Please note that some figures may have been included with permission from other third parties. It is your responsibility to obtain the proper permission from the rights holder directly for these figures.

Export citation

Export citation

Choose format for download:

Download Citation
  • Open Access
  • Access by Xinjiang University

Strong-deflection expansion of the deflection angle near a degenerate photon sphere

Takahisa Igata1,*, Tadashi Sasaki2,†, and Naoki Tsukamoto3,‡

  • *Contact author: takahisa.igata@gakushuin.ac.jp
  • Contact author: ta-sasaki@kumagaku.ac.jp
  • Contact author: tsukamoto@rikkyo.ac.jp

Phys. Rev. D 113, 104022 – Published 12 May, 2026

DOI: https://doi.org/10.1103/b47c-8rdg

Abstract

We present a strong-deflection expansion for the deflection angle of light rays scattered near a degenerate photon sphere in asymptotically flat, static, and spherically symmetric spacetimes. Our prescription isolates the divergent contribution to the deflection-angle integral arising from the ray’s passage near the marginal orbit in a way that remains nonsingular at marginality, thereby yielding a unique leading power-law term. When expressed in terms of the radius of closest approach, the leading coefficient in the strong deflection limit factorizes into a universal branch constant and a local factor determined by the third derivative of the effective potential at the degenerate photon sphere. When the expansion is rewritten in terms of the impact parameter, the coefficient is simply multiplied by an additional local conversion factor. We show that the local factor in the closest-approach expansion admits an invariant representation through the areal-radius derivative of a dimensionless tidal measure constructed from the electric part of the Weyl tensor. In general relativity, we further relate this quantity to the areal-radius derivative of a weighted null-energy density profile. Analytic examples validate this factorization and yield closed-form expressions for the leading divergent coefficients in representative marginal configurations.

View figure in article

Physics Subject Headings (PhySH)

See Also

Article Text

References (63)

  1. J. M. Bardeen, Timelike and null geodesics in the Kerr metric, in Black Holes (Les Astres Occlus), edited by C. DeWitt and B. S. DeWitt (Gordon and Breach, New York, 1973), pp. 215–239.
  2. K. Akiyama et al. (Event Horizon Telescope Collaboration), Astrophys. J. Lett. 875, L1 (2019).
  3. K. Akiyama et al. (Event Horizon Telescope Collaboration), Astrophys. J. Lett. 930, L12 (2022).
  4. J. P. Luminet, Astron. Astrophys. 75, 228 (1979), https://ui.adsabs.harvard.edu/abs/1979A&A....75..228L/abstract.
  5. J. Fukue and T. Yokoyama, Publ. Astron. Soc. Jpn. 40, 15 (1988).
  6. H. Falcke, F. Melia, and E. Agol, Astrophys. J. Lett. 528, L13 (2000).
  7. R. Takahashi, J. Korean Phys. Soc. 45, S1808 (2004); Astrophys. J. 611, 996 (2004).
  8. K. Hioki and K. i. Maeda, Phys. Rev. D 80, 024042 (2009).
  9. T. Igata, H. Ishihara, and Y. Yasunishi, Phys. Rev. D 100, 044058 (2019).
  10. S. E. Gralla, D. E. Holz, and R. M. Wald, Phys. Rev. D 100, 024018 (2019).
  11. S. E. Gralla, A. Lupsasca, and D. P. Marrone, Phys. Rev. D 102, 124004 (2020).
  12. C. Darwin, Proc. R. Soc. A 249, 180 (1959).
  13. V. Bozza, S. Capozziello, G. Iovane, and G. Scarpetta, Gen. Relativ. Gravit. 33, 1535 (2001).
  14. K. S. Virbhadra and G. F. R. Ellis, Phys. Rev. D 62, 084003 (2000).
  15. V. Perlick, Living Rev. Relativity 7, 9 (2004).
  16. V. Bozza, Phys. Rev. D 66, 103001 (2002).
  17. V. Bozza, Gen. Relativ. Gravit. 42, 2269 (2010).
  18. C. M. Claudel, K. S. Virbhadra, and G. F. R. Ellis, J. Math. Phys. (N.Y.) 42, 818 (2001).
  19. M. Cvetic, G. W. Gibbons, and C. N. Pope, Phys. Rev. D 94, 106005 (2016).
  20. R. Kudo and H. Asada, Phys. Rev. D 105, 084014 (2022).
  21. S. Hod, Phys. Lett. B 776, 1 (2018).
  22. P. V. P. Cunha, E. Berti, and C. A. R. Herdeiro, Phys. Rev. Lett. 119, 251102 (2017).
  23. N. Tsukamoto, Eur. Phys. J. C 84, 1325 (2024).
  24. J. Zhang and Y. Xie, Phys. Rev. D 109, 043032 (2024).
  25. N. Tsukamoto, Phys. Rev. D 102, 104029 (2020).
  26. N. Tsukamoto, arXiv:2512.01688.
  27. T. Chiba and M. Kimura, Prog. Theor. Exp. Phys. 2017, 043E01 (2017).
  28. T. Damour and S. N. Solodukhin, Phys. Rev. D 76, 024016 (2007).
  29. N. Tsukamoto, Phys. Rev. D 101, 104021 (2020); 106, 049901(E) (2022).
  30. Q. M. Fu and X. Zhang, Phys. Rev. D 105, 064020 (2022).
  31. M. Patil, P. Mishra, and D. Narasimha, Phys. Rev. D 95, 024026 (2017).
  32. T. Sasaki, Phys. Rev. D 112, 024072 (2025).
  33. E. F. Eiroa, G. E. Romero, and D. F. Torres, Phys. Rev. D 66, 024010 (2002).
  34. N. Tsukamoto, Phys. Rev. D 95, 064035 (2017).
  35. T. Igata, Phys. Rev. D 113, 044042 (2026).
  36. I. Z. Stefanov, S. S. Yazadjiev, and G. G. Gyulchev, Phys. Rev. Lett. 104, 251103 (2010).
  37. B. Raffaelli, Gen. Relativ. Gravit. 48, 16 (2016).
  38. T. Igata and Y. Takamori, arXiv:2603.09946.
  39. T. Igata, Phys. Rev. D 113, 024036 (2026).
  40. T. Igata, arXiv:2505.01848.
  41. R. M. Wald, General Relativity (University of Chicago Press, Chicago, 1984).
  42. C. W. Misner and D. H. Sharp, Phys. Rev. 136, B571 (1964).
  43. S. A. Hayward, Phys. Rev. D 53, 1938 (1996).
  44. S. Kinoshita, Phys. Rev. D 110, 044056 (2024).
  45. R. Shaikh, P. Banerjee, S. Paul, and T. Sarkar, Phys. Rev. D 99, 104040 (2019).
  46. N. Tsukamoto, Phys. Rev. D 104, 124016 (2021).
  47. S. A. Hayward, Phys. Rev. Lett. 96, 031103 (2006).
  48. J. M. Bardeen, in Proceedings of the 5th International Conference on Gravitation and the Theory of Relativity (GR5), edited by V. A. Fock et al. (Tbilisi University Press, Tbilisi, 1968), p. 174.
  49. E. Ayon-Beato and A. Garcia, Phys. Lett. B 493, 149 (2000).
  50. E. F. Eiroa and C. M. Sendra, Classical Quantum Gravity 28, 085008 (2011).
  51. J. P. S. Lemos and O. B. Zaslavskii, Phys. Rev. D 78, 024040 (2008).
  52. E. Berti, V. Cardoso, and A. O. Starinets, Classical Quantum Gravity 26, 163001 (2009).
  53. R. A. Konoplya and A. Zhidenko, Rev. Mod. Phys. 83, 793 (2011).
  54. V. Ferrari and B. Mashhoon, Phys. Rev. D 30, 295 (1984).
  55. V. Cardoso, A. S. Miranda, E. Berti, H. Witek, and V. T. Zanchin, Phys. Rev. D 79, 064016 (2009).
  56. H. Yang, F. Zhang, A. Zimmerman, D. A. Nichols, E. Berti, and Y. Chen, Phys. Rev. D 87, 041502 (2013).
  57. H. Yang, D. A. Nichols, F. Zhang, A. Zimmerman, Z. Zhang, and Y. Chen, Phys. Rev. D 86, 104006 (2012).
  58. S. Iyer and C. M. Will, Phys. Rev. D 35, 3621 (1987).
  59. Y. Hatsuda and M. Kimura, Universe 7, 476 (2021).
  60. R. A. Konoplya and Z. Stuchlík, Phys. Lett. B 771, 597 (2017).
  61. G. Guo, P. Wang, H. Wu, and H. Yang, J. High Energy Phys. 06 (2022) 060.
  62. G. Guo, P. Wang, H. Wu, and H. Yang, J. High Energy Phys. 10 (2023) 076.
  63. E. Teo, Gen. Relativ. Gravit. 35, 1909 (2003).

Outline

Information

Sign In to Your Journals Account

Filter

Filter

Article Lookup

Enter a citation