Resonant scattering of light in a near-black-hole metric
Y. V. Stadnik, G. H. Gossel, V. V. Flambaum, J. C. Berengut

TL;DR
This paper demonstrates that objects with radii just larger than their Schwarzschild radius can mimic black-hole absorption of light through resonant scattering, trapping photons for long durations and appearing black.
Contribution
It reveals that near-black-hole metrics can produce black-hole-like absorption via resonant states, even without a true event horizon.
Findings
Resonant states cause long-lived photon trapping.
The averaged cross-section matches black-hole absorption.
Objects can appear black without forming a true black hole.
Abstract
We show that low-energy photon scattering from a body with radius R slightly larger than its Schwarzschild radius r_s resembles black-hole absorption. This absorption occurs via capture to one of the many long-lived, densely packed resonances that populate the continuum. The lifetimes and density of these meta-stable states tend to infinity in the limit r_s -> R. We determine the energy averaged cross-section for particle capture into these resonances and show that it is equal to the absorption cross-section for a Schwarzschild black hole. Thus, a non-singular static metric may trap photons for arbitrarily long times, making it appear completely `black' before the actual formation of a black hole.
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