Black holes as random particles: entanglement dynamics in infinite range and matrix models
Javier M. Magan

TL;DR
This paper introduces a quantum toy model mimicking black hole dynamics, analyzing entanglement and thermalization, and extends the insights to large-N matrix models, challenging existing scrambling conjectures and exploring implications for black hole physics.
Contribution
It presents a novel unitary toy model of black hole dynamics with analytical solutions, and extends the framework to large-N matrix models, providing new insights into entanglement and thermalization.
Findings
Model exhibits quantum thermalization and information scrambling.
Entanglement depends on occupation densities and quasinormal frequencies.
Results challenge the fast scrambling conjecture and relate to black hole horizon physics.
Abstract
We first propose and study a quantum toy model of black hole dynamics. The model is unitary, displays quantum thermalization, and the Hamiltonian couples every oscillator with every other, a feature intended to emulate the color sector physics of large- matrix models. Considering out of equilibrium initial states, we analytically compute the time evolution of every correlator of the theory and of the entanglement entropies, allowing a proper discussion of global thermalization/scrambling of information through the entire system. Microscopic non-locality causes factorization of reduced density matrices, and entanglement just depends on the time evolution of occupation densities. In the second part of the article, we show how the gained intuition extends to large- matrix models, where we provide a gauge invariant entanglement entropy for `generalized free…
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