Black holes as frozen stars
Ram Brustein, A.J.M. Medved, Tamar Simhon

TL;DR
This paper develops a classical model of ultra-compact objects with a transitional layer, demonstrating that perturbations are frozen in this layer, supporting the stability of the proposed black hole alternative.
Contribution
It introduces a detailed analysis of the transitional layer in a regular black hole model, showing stability and frozen perturbations at linear order.
Findings
The transitional layer smoothly connects the interior to the Schwarzschild exterior.
Perturbations are perfectly frozen in the transitional layer at linear order.
The model supports the stability of the ultra-compact object against small disturbances.
Abstract
We have recently proposed a model for a regular black hole, or an ultra-compact object, that is premised on having maximally negative radial pressure throughout the entirety of the object's interior. This model can be viewed as that of a highly entropic configuration of fundamental, closed strings near the Hagedorn temperature, but from the perspective of an observer who is ignorant about the role of quantum physics in counteracting against gravitational collapse. The advantage of this classical perspective is that one can use Einstein's equations to define a classical geometry and investigate its stability. Here, we complete the model by studying an important aspect of this framework that has so far been overlooked: The geometry and composition of the outermost layer of the ultra-compact object, which interpolates between the bulk geometry of the object and the standard Schwarzschild…
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