Dynamics and Observational Signatures of Shell-like Black Hole Mimickers

TL;DR

This paper explores the dynamics of shell-like black hole mimickers called AdS black bubbles, developing numerical methods to study their stability, accretion behavior, and potential observational signatures as alternatives to traditional black holes.

Contribution

It introduces a new formalism and numerical models for analyzing the non-linear dynamics of quantum gravity motivated black hole mimickers, specifically focusing on AdS black bubbles and their stability.

Findings

Identified parameter regions allowing stable black bubbles.

Developed a generalized flux model for stability in dynamical settings.

Proposed observational implications of black bubbles as black hole alternatives.

Abstract

We undertake the task of studying the non-linear dynamics of quantum gravity motivated alternatives to black holes that in the classical limit appear as ultra-compact shells of matter. We develop a formalism that should be amenable to numerical solution in generic situations. For a concrete model we focus on the spherically symmetric AdS black bubble -- a shell of matter at the Buchdahl radius separating a Schwarzschild exterior from an AdS interior. We construct a numerical code to study the radial dynamics of and accretion onto AdS black bubbles, with exterior matter provided by scalar fields. In doing so we develop numerical methods that could be extended to future studies beyond spherical symmetry. Regarding AdS black bubbles in particular, we find that the original prescription for the internal matter fluxes needed to stabilize the black bubble is inadequate in dynamical settings, and we propose a two parameter generalization of the flux model to fix this. To allow for more efficient surveys of parameter space, we develop a simpler numerical model adapted to spherically symmetric bubble dynamics. We identify regions of parameter space that do allow for stable black bubbles, and moreover allow control to a desired end-state after an accretion episode. Based on these results, and evolution of scalar fields on black bubble backgrounds, we speculate on some observational consequences if what are currently presumed to be black holes in the universe were actually black bubbles.