Are quantization rules for horizon areas universal?
Valerio Faraoni, Andres F. Zambrano Moreno (Bishop's University)

TL;DR
This paper investigates the universality of horizon area quantization rules in black holes, demonstrating through examples that these rules do not generally hold in dynamical, non-stationary black hole spacetimes.
Contribution
The study provides evidence that horizon area quantization rules are not universal and do not apply to realistic, time-dependent black holes in general relativity.
Findings
Quantization rules fail in dynamical black hole spacetimes
Rules may only hold at isolated moments in time
Quantization is not universal across different black hole models
Abstract
Doubts have been expressed on the universality of holographic/string-inspired quantization rules for the horizon areas of stationary black holes or the products of their radii, already in simple 4-dimensional general relativity. Realistic black holes are not stationary but time-dependent. Using two examples of 4D general-relativistic spacetimes containing dynamical black holes for at least part of the time, it is shown that the quantization rules (even counting virtual horizons) cannot hold, except possibly at isolated instants of time, and do not seem to be universal.
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