A First-Order Eikonal Framework for Quasinormal Modes, Shadows, Strong Lensing, and Grey-Body Factors in a Scalarized Black-Hole Metric
Bekir Can L\"utf\"uo\u{g}lu, Javlon Rayimbaev, Sardor Murodov, Jakhongir Kurbanov, Muhammad Matyoqubov

TL;DR
This paper develops an analytic framework connecting black-hole metrics to observable phenomena like quasinormal modes, shadows, and lensing, using a first-order eikonal approximation applicable to scalarized black holes.
Contribution
It introduces a closed-form, first-order eikonal approach linking black-hole geometry to multiple observables, extending the standard shadow–ringdown correspondence.
Findings
Derived formulas for photon-sphere radius, orbital frequency, and Lyapunov exponent.
Established a universal relation between quasinormal modes and shadow/deflection observables.
Analyzed grey-body factors and damping ratios across different core sizes.
Abstract
We construct an analytic geodesic-optics description of quasinormal ringing, black-hole shadows, strong lensing, and grey-body factors for the static spherical metric introduced in [Bakopoulos, et. al. arXiv:2310.11919]. Working in a weak-hair regime, we derive closed first-order formulas for the photon-sphere radius, orbital frequency, and Lyapunov exponent. These invariants are then employed within the Schutz--Will WKB approach to obtain eikonal quasinormal frequencies, mapped to shadow and strong-deflection observables through exact identities for static spherical geometries, and used to build a closed analytic form for the transmission probability. At leading eikonal order, these relations are controlled by null geodesics and are therefore spin-universal for test scalar/electromagnetic/gravitational sectors, up to subleading corrections. Besides the standard ringdown--shadow…
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