Black-hole entropy and minimal diffusion
Michele Arzano, Gianluca Calcagni

TL;DR
This paper models black-hole entropy using a nonlocal field theory, revealing a minimal diffusion scale where the spectral dimension diverges, impacting holographic entropy bounds.
Contribution
It introduces a diffusion process based on a nonlocal theory that exhibits a finite minimal scale and unusual spectral dimension flow, linking quantum gravity and holography.
Findings
Spectral dimension asymptotes four in the infrared
Diverges at a finite Planckian scale in the ultraviolet
Implications for entropy bounds and spacetime structure
Abstract
The density of states reproducing the Bekenstein-Hawking entropy-area scaling can be modeled via a nonlocal field theory. We define a diffusion process based on the kinematics of this theory and find a spectral dimension whose flow exhibits surprising properties. While it asymptotes four from above in the infrared, in the ultraviolet the spectral dimension diverges at a finite (Planckian) value of the diffusion length, signaling a breakdown of the notion of diffusion on a continuum spacetime below that scale. We comment on the implications of this minimal diffusion scale for the entropy bound in a holographic and field-theoretic context.
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