TL;DR
This paper introduces a random matrix model for black holes derived from Gaussian complex ensembles, capturing spacetime dynamics and aligning with key principles like asymptotic freedom and holography.
Contribution
It presents a novel random matrix framework for black holes that incorporates spacetime freedoms and reproduces fundamental physical principles.
Findings
Model computes classical black hole observables
Satisfies asymptotic freedom
Aligns with holographic principle
Abstract
A random matrix model of black holes is given based on analysis of Gaussian complex ensembles, based on the generalization of chRMT of QCD. Spacetime freedoms are incorporated in terms of eigenvalues of the ensemble. Classical observables of black holes can be computed using this model and it satisfies asymptotic freedom and holographic principle.
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Noncommutative and Quantum Gravity Theories