Black Hole Greybody Factors from Korteweg-de Vries Integrals: Computation
Michele Lenzi, Carlos F. Sopuerta

TL;DR
This paper introduces a semi-analytical, efficient method using KdV integrals and Padé approximants to accurately compute black hole greybody factors, validated against known solutions and WKB approximations.
Contribution
It develops a novel semi-analytical approach leveraging KdV integrals and Padé approximants to determine black hole greybody factors from conserved quantities.
Findings
Accurate greybody factors for Schwarzschild black holes across all frequencies.
Method validated against analytical Pöschl-Teller potential results.
Computationally efficient compared to traditional WKB methods.
Abstract
It has recently been shown that the dynamics of perturbed non-rotating black holes (BHs) admits an infinite number of symmetries that are generated by the flow of the Korteweg-de Vries (KdV) equation. These symmetries lead to an infinite number of conserved quantities that can be obtained as integrals of differential polynomials in the potential appearing in the gauge-invariant master equations describing the BH perturbations, the KdV integrals. These conserved quantities are the same for all the possible potentials, which means that they are invariant under Darboux transformations, and they fully determine the BHs transmission amplitudes, or greybody factors, via a moment problem. In this paper we introduce a new semi-analytical method to obtain the greybody factors associated with BH scattering processes by solving the moment problem using only the KdV integrals. The method is based…
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Taxonomy
TopicsNonlinear Waves and Solitons · Advanced Fiber Optic Sensors · Image and Signal Denoising Methods
