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Asymptotics and Universality in Black Holes: from the quasinormal Weyl's law to the binary merger waveform

José Luis Jaramillo, Lamis Al Sheikh, Jérémy Besson, Badri Krishnan, Michele Lenzi, Rodrigo Panosso Macedo, Oscar Meneses-Rojas, Bernard Raffaelli, Carlos F. Sopuerta, Corentin Vitel

TL;DR

The paper investigates why black-hole spacetimes and binary black-hole mergers exhibit striking simplicity and universality. It advocates an asymptotic reasoning framework that isolates key structures, notably through a quasinormal-mode Weyl-law analysis that links the counting of complex frequencies to the redshift (surface gravity $\kappa$) and light-trapping geometry (light-ring area), with a generalization to higher dimensions via phase-space volumes. It further proposes a dual mechanism for BBH waveform universality: (i) an Airy-diffraction pattern on caustics capturing universal linear dispersive behavior (Mechanism 1), and (ii) an integrability-driven background threaded by Painlevé-II transcendent guiding BBH dynamics across inspiral to ringdown (Mechanism 2). Finally, a hierarchical, Wave-Mean-Flow BBH program is outlined, coupling fast dispersive waves to slow integrable-like dynamics, aiming to produce a structured, asymptotic pathway toward understanding BBH simplicity and its potential connections to gravity's deeper integrable structures. This framework could illuminate universal patterns and even offer observational probes of spacetime dimensionality in strong gravity regimes.

Abstract

Current state-of-the-art approaches to black hole (BH) dynamics, encompassing several effective approximation schemes, offer a remarkable control of the quantitative aspects of strong gravity. They also provide key insights into some qualitative aspects of the problem. In spite of this, there remain blind spots that hinder the understanding of the mechanisms underlying some observed phenomena, in particular concerning simplicity and universality in BH spacetimes. Adopting an 'asymptotic reasoning' approach, by filtering non-essential degrees of freedom, can potentially unveil universality patterns by identifying key underlying structural stability mechanisms. We first illustrate such an asymptotic approach by focusing on a BH quasinormal (QNM) Weyl's law, that accounts for the universal asymptotics of the QNM "counting function". This permits to identify light-trapping and the (local) redshift effect as the underlying mechanisms, also offering a bridge to the universal patterns found in BH QNM spectral instability. As a by-product, Weyl's law universality formally opens an observational access to spacetime (effective) dimensionality. More heuristically, we sketch a program recently put forward to apply such 'asymptotic reasoning' to address the observed simplicity and universality patterns in binary BH merger dynamics. This program is built as a hierarchy of asymptotic models, potentially making contact with integrability theory in gravity, namely through the background sector in a "wave-mean flow" approach to BH binary dynamics.

Asymptotics and Universality in Black Holes: from the quasinormal Weyl's law to the binary merger waveform

TL;DR

The paper investigates why black-hole spacetimes and binary black-hole mergers exhibit striking simplicity and universality. It advocates an asymptotic reasoning framework that isolates key structures, notably through a quasinormal-mode Weyl-law analysis that links the counting of complex frequencies to the redshift (surface gravity ) and light-trapping geometry (light-ring area), with a generalization to higher dimensions via phase-space volumes. It further proposes a dual mechanism for BBH waveform universality: (i) an Airy-diffraction pattern on caustics capturing universal linear dispersive behavior (Mechanism 1), and (ii) an integrability-driven background threaded by Painlevé-II transcendent guiding BBH dynamics across inspiral to ringdown (Mechanism 2). Finally, a hierarchical, Wave-Mean-Flow BBH program is outlined, coupling fast dispersive waves to slow integrable-like dynamics, aiming to produce a structured, asymptotic pathway toward understanding BBH simplicity and its potential connections to gravity's deeper integrable structures. This framework could illuminate universal patterns and even offer observational probes of spacetime dimensionality in strong gravity regimes.

Abstract

Current state-of-the-art approaches to black hole (BH) dynamics, encompassing several effective approximation schemes, offer a remarkable control of the quantitative aspects of strong gravity. They also provide key insights into some qualitative aspects of the problem. In spite of this, there remain blind spots that hinder the understanding of the mechanisms underlying some observed phenomena, in particular concerning simplicity and universality in BH spacetimes. Adopting an 'asymptotic reasoning' approach, by filtering non-essential degrees of freedom, can potentially unveil universality patterns by identifying key underlying structural stability mechanisms. We first illustrate such an asymptotic approach by focusing on a BH quasinormal (QNM) Weyl's law, that accounts for the universal asymptotics of the QNM "counting function". This permits to identify light-trapping and the (local) redshift effect as the underlying mechanisms, also offering a bridge to the universal patterns found in BH QNM spectral instability. As a by-product, Weyl's law universality formally opens an observational access to spacetime (effective) dimensionality. More heuristically, we sketch a program recently put forward to apply such 'asymptotic reasoning' to address the observed simplicity and universality patterns in binary BH merger dynamics. This program is built as a hierarchy of asymptotic models, potentially making contact with integrability theory in gravity, namely through the background sector in a "wave-mean flow" approach to BH binary dynamics.

Paper Structure

This paper contains 9 sections, 7 equations.