Theoretical analysis demonstrates universal scaling laws in degenerate circular null orbits, highlighting new critical dynamics in relativistic gravitational lensing.
Circular null orbits are fundamental structures in relativistic gravitational lensing, photon trapping, black-hole shadows, and the propagation of high-frequency radiation. For an ordinary unstable photon sphere, the associated radial potential possesses a nondegenerate maximum, producing exponential approach to the critical orbit and the familiar logarithmic divergence of the strong-deflection angle. A marginally unstable photon sphere occurs when the quadratic curvature of the effective potential vanishes, producing instead algebraic critical dynamics and power-law divergence of the deflection angle. In this work, we develop a systematic higher-order classification of degenerate circular null orbits based on the order of the first nonvanishing derivative of the photon effective potential. If the first nonzero derivative occurs at order n > 2, we show locally that the critical trajectory obeys the universal algebraic law r − r꜀ ∼ |φ|⁻²ⁿ⁻² (that is, r − r꜀ ∼ |φ| raised to the power −2/(n−2)), while, under the appropriate scattering assumptions, the strong-deflection angle scales with impact parameter as α_div ∼ |b − b꜀| raised to the power −(n−2)/(2n). These exponents satisfy the universal relation χₙηₙ = 1/n, where χₙ = 2/(n − 2) characterizes critical-orbit relaxation and ηₙ = (n − 2)/(2n) characterizes strong-deflection divergence. The familiar logarithmic case is recovered as the nondegenerate n = 2 limit in a singular rather than algebraic sense, while the established cubic marginal case corresponds to n = 3. We then construct an explicit asymptotically flat, static, spherically symmetric spacetime realizing the quartic class (n = 4), A₄(r) = 1 − 2/r + 3/(2r²) − 2/(5r³), for which the photon potential possesses an exact quartic maximum at r꜀ = 1. The corresponding critical trajectory obeys r − r꜀ ∼ |φ|⁻¹, and the strong-deflection angle exhibits the new power law α_div ∼ |b − b꜀|⁻¹ᐟ⁴. The model is asymptotically flat, possesses a regular exterior region r ≥ 1, and its effective stress-energy tensor satisfies the null, weak, strong, and dominant energy conditions throughout that exterior. The results establish a hierarchy of universality classes for degenerate circular null trapping and identify the quartic class as the first even-order extension beyond the currently established cubic marginal case.
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Nazat Md. Shaikhul Hadis (2026) studied this question.
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