Integrability in Perturbed Black Holes: Background Hidden Structures
Jos\'e Luis Jaramillo, Michele Lenzi, Carlos F. Sopuerta

TL;DR
This paper explores hidden integrable structures in perturbed non-rotating black holes, revealing potential for a new understanding of black hole dynamics through symmetry and hierarchy analysis.
Contribution
It systematically investigates integrable structures in black hole perturbation theory, linking wave equations to infinite hierarchies of symmetries and slow-fast degrees of freedom.
Findings
Wave master equations possess infinite symmetries related to KdV hierarchies.
Structural relations between bulk and boundary contributions reveal slow and fast DoFs.
Extension of analysis from Cauchy slices to hyperboloidal foliations uncovers underlying integrable structures.
Abstract
In this work we investigate the presence of integrable hidden structures in the dynamics of perturbed non-rotating black holes (BHs). This can also be considered as a first step in a wider program of an effective identification of ``slow'' and ``fast'' degrees of freedom (DoFs) in the (binary) BH dynamics, following a wave-mean flow perspective. The slow DoFs would be associated with a nonlinear integrable dynamics, on which the fast ones propagate following an effective linear dynamics. BH perturbation theory offers a natural ground to test these properties. Indeed, the decoupling of Einstein equations into wave master equations with a potential provides an instance of such splitting into (frozen) slow DoFs (background potential) over which the linear dynamics of the fast ones (perturbation master functions) evolve. It has been recently shown that these wave equations possess an…
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Nonlinear Waves and Solitons
