Quantum black holes, partition of integers and self-similarity
Paolo Castorina, Alfredo Iorio, Luca Smaldone

TL;DR
This paper explores the quantization of black hole horizons, linking their configurations to integer partitions, revealing self-similarity properties, and analyzing quantum corrections to entropy within a finite fermionic degrees of freedom framework.
Contribution
It introduces a novel connection between black hole configurations and integer partitions, demonstrating self-similarity and providing insights into quantum entropy corrections.
Findings
Black hole horizon area quantized as $A = l_P^2 (4 \, \ln 2) N$
A two-to-one mapping between configurations and integer partitions of N
Self-similarity of black hole configurations derived from partition properties
Abstract
We take the view that the area of a black hole's event horizon is quantized, , and the associated degrees of freedom are finite in number and of fermionic nature. We then investigate general aspects of the entropy, , our main focus being black-hole self-similarity. We first find a two-to-one map between the black hole's configurations and the ordered partitions of the integer . Hence we construct from there a composition law between the sub-parts making the whole configuration space. This gives meaning to black hole self-similarity, entirely within a single description, as a phenomenon stemming from the well known self-similarity of the ordered partitions of . Finally, we compare the above to the well-known results on the subleading (quantum) corrections, that necessarily require different (quantum) statistical weights for the various…
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Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Statistical Mechanics and Entropy
