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Discrete Holographic Reduction of the Three-Body Problem: Tripartite Frustration and the Pesin-Landauer Isomorphism

Robert Rode

Published Jun 7, 2026• 0 citations
Publisher

Abstract

We propose a discrete holographic framework for analyzing the thermodynamic origins of classical chaos in the three-body problem. By representing interacting point masses as localized Bekenstein horizons on a unitary MERA tensor network, we propose that classical Lyapunov divergence is an emergent kinematic projection of epistemic coarse-graining. At the discrete zero-dissipation limit, Node Symmetry Invariance (NSI) dictates strictly unitary evolution and exact Poincaré recurrence. The mapping of this network into a continuous macroscopic phase space requires the continuous truncation of Schmidt coefficients due to the Coffman-Kundu-Wootters (CKW) monogamy bound of tripartite entanglement. By invoking Pesin's Identity, we mathematically map the observed continuous Lyapunov exponent directly to the thermodynamic integration of this Landauer boundary erasure over time. Finally, we demonstrate that the fractal geometries of macroscopic strange attractors correspond to generalized Ryu-Takayanagi minimal surfaces, indicating that chaotic orbits are thermodynamic geodesics minimizing the continuous projection of discrete quantum noise.

DOI
10.5281/zenodo.20583892

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We propose a discrete holographic framework for analyzing the thermodynamic origins of classical chaos in the three-body problem. By representing interacting point masses as localized Bekenstein horizons on a unitary MERA tensor network, we propose that classical Lyapunov divergence is an emergent kinematic projection of epistemic coarse-graining. At the discrete zero-dissipation limit, Node Symmetry Invariance (NSI) dictates strictly unitary evolution and exact Poincaré recurrence. The mapping of this network into a continuous macroscopic phase space requires the continuous truncation of Schmidt coefficients due to the Coffman-Kundu-Wootters (CKW) monogamy bound of tripartite entanglement. By invoking Pesin's Identity, we mathematically map the observed continuous Lyapunov exponent directly to the thermodynamic integration of this Landauer boundary erasure over time. Finally, we demonstrate that the fractal geometries of macroscopic strange attractors correspond to generalized Ryu-Takayanagi minimal surfaces, indicating that chaotic orbits are thermodynamic geodesics minimizing the continuous projection of discrete quantum noise.
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Extending the holographic principle to de Sitter (dS) spacetimes remains one of the most vital open frontiers in quantum gravity, where a microscopic, bottom-up tensor-network framework that relates boundary quantum data to emergent de Sitter spacetime is still lacking. In this work, we first show the emergence of de Sitter spacetime from boundary entanglement by formulating a non-unitary continuous multi-scale entanglement renormalization ansatz (cMERA) for a concrete non-Hermitian critical fermion chain. Within this emergent spacetime, we analyze the associated geodesics and show that they act as extremal Ryu-Takayanagi (RT) surfaces undergoing a smooth timelike-to-null transition. Remarkably, we demonstrate that this continuum trajectory suggests a distinct tensor-network architecture in which the bond-counting contribution naturally truncates at the discrete timelike-to-null transition toward the deep infrared. In the resulting architecture, the null ray along the horizon is represented by zero-cost links, since the associated cut severs no tensor legs. This network structure successfully reproduces the logarithmic scaling of non-unitary critical entanglement entropy, offering a bond-counting picture for the de Sitter RT formula. Our results provide the long-sought dS/(c)MERA correspondence at the level of both emergent spacetime and discrete holographic entanglement.
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