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Photon-sphere jet equivalence and the non-uniqueness of black-hole thermodynamics

Year: 2026
Type: article
Abstract: We examine whether scalar eikonal quasinormal-mode data determine black-hole thermodynamics. For static, spherically symmetric, asymptotically flat, nonextremal geometries, we prove that the formal fixed-overtone expansion of a neutral, minimally coupled, massless scalar through order L − N depends only on the ( 2 N + 2 ) jet of the lapse at the unstable photon sphere. For every finite N , real-analytic deformations can preserve this jet and the asymptotic Reissner–Nordström coefficients while changing the surface gravity and Hawking temperature. We also construct a nonanalytic C ∞ deformation that is flat at the photon sphere. This deformation preserves the complete formal eikonal series to every algebraic order but changes the horizon position, temperature, and Einstein area entropy. A nonempty charged subfamily satisfies the weak energy condition as an effective Einstein source. Together, these four results establish the new finite-jet and all-orders thermodynamic obstruction. To separate geometric information from action-dependent information, we incorporate a previously established Reissner–Nordström–MOG comparison. The mapped backgrounds have identical normalized metrics, neutral-scalar boundary-value problems, exact scalar spectra, and Hawking temperatures, yet their Wald entropies differ because their curvature couplings differ. The resulting hierarchy shows that local photon-sphere data do not determine horizon thermodynamics and that even exact action-blind scalar data do not determine gravitational entropy. Agreement of the formal eikonal expansions for the deformed metrics does not imply exact finite- ℓ isospectrality. Global differences may appear beyond every algebraic order. Thermodynamic reconstruction from eikonal ringdown is therefore conditional on assumptions about the global metric and the gravitational action.
Language: English
Open Access status: green
OpenAlex ID: W7223096579
FWCI:
Cites: 22
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Related to: 10