Quantization of area for event and Cauchy horizons of the Kerr-Newman black hole
Matt Visser (Victoria University of Wellington)

TL;DR
This paper critically examines the idea that black hole horizon areas are quantized in specific integer-based patterns, highlighting physical constraints and limitations in applying such proposals to Kerr-Newman black holes.
Contribution
It provides a detailed analysis of the physical constraints on horizon area quantization proposals, especially in the context of Kerr-Newman black holes, challenging some string-inspired theories.
Findings
Integer-based quantization proposals often fail for Kerr-Newman black holes.
Physical constraints limit the applicability of certain horizon area quantization models.
Explicit spectra calculations suggest caution in assuming universal quantization patterns.
Abstract
Based on various string theoretic constructions, and various string-inspired generalizations thereof, there have been repeated suggestions that the areas of black hole event horizons might be quantized in a quite specific manner, in terms of linear combinations of square roots of positive integers. It is important to realise that there are significant physical constraints on such integer-based proposals when one (somewhat speculatively) attempts to extend them outside their original extremal and supersymmetric framework. Specifically, in their most natural and direct physical interpretations, some of the more speculative integer-based proposals for the quantization of horizon areas fail for the ordinary Kerr-Newman black holes in (3+1) dimensions, essentially because the fine structure constant is not an integer. A more baroque interpretation involves asserting the fine structure…
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