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Extending the QMM Framework to the Strong and Weak Interactions

2025/02/02 by Florian Neukart, E. J. Marx, Eike Marx +2 · 1 voice · 9 citations
Mathematics · Physics and Astronomy · #Black Holes and Theoretical Physics #Computer science #Cosmology and Gravitation Theories #Mathematics #Noncommutative and Quantum Gravity Theories #Physics #Statistical physics #Theoretical computer science #physics.gen-ph

paper · pdf · doi:10.3390/e27020153

published in Entropy 27(2), 153 (Multidisciplinary Digital Publishing Institute)

openalex publication_date 2025/02/02 · arxiv published 2025/04/04 · arxiv updated 2025/04/04 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

We extend the Quantum Memory Matrix (QMM) framework, originally developed to reconcile quantum mechanics and general relativity by treating space–time as a dynamic information reservoir, to incorporate the full suite of Standard Model gauge interactions. In this discretized, Planck-scale formulation, each space–time cell possesses a finite-dimensional Hilbert space that acts as a local memory, or quantum imprint, for matter and gauge field configurations. We focus on embedding non-Abelian SU(3)c (quantum chromodynamics) and SU(2)L × U(1)Y (electroweak interactions) into QMM by constructing gauge-invariant imprint operators for quarks, gluons, electroweak bosons, and the Higgs mechanism. This unified approach naturally enforces unitarity by allowing black hole horizons, or any high-curvature region, to store and later retrieve quantum information about color and electroweak charges, thereby preserving subtle non-thermal correlations in evaporation processes. Moreover, the discretized nature of QMM imposes a Planck-scale cutoff, potentially taming UV divergences and modifying running couplings at trans-Planckian energies. We outline major challenges, such as the precise formulation of non-Abelian imprint operators and the integration of QMM with loop quantum gravity, as well as possible observational strategies—ranging from rare decay channels to primordial black hole evaporation spectra—that could provide indirect probes of this discrete, memory-based view of quantum gravity and the Standard Model.

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