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Hypercomplex General Relativity (HGR): A symplectic and geometric reformulation of Weyl, hypercomplex numbers with late cosmological applications.

Besson, Laurent · Zenodo (CERN)
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dark-mattergeneral-relativity-extensionsymplectic-formulation-of-gravityweyl-geometry-and-scale-invariance
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Hypercomplex General Relativity (HGR): A symplectic and geometric reformulation of Weyl, hypercomplex numbers with late cosmological applications. | Zenodo Skip to main Communities My dashboard Log in Sign up Zenodo is currently experiencing slowness and intermittent outages due to heavy automated traffic from bots and AI crawlers. We are aware of the problem, and our team is focused on stabilizing the service. Thank you for your patience. Advanced Theoretical Physics and Mathematics There is a newer version of the record available. Published May 10, 2026 | Version v32 Journal article Open Hypercomplex General Relativity (HGR): A symplectic and geometric reformulation of Weyl, hypercomplex numbers with late cosmological applications. Authors/Creators Besson, Laurent (Contact person) Description Hypercomplex General Relativity (HGR), also referred to as Relativité Générale Hypercomplexe (HGR) in French, is a unified theoretical framework... This deposit gathers and documents the complete body of work related to Hypercomplex General Relativity (HGR), an extension of General Relativity developed by Laurent Besson. HGR introduces an internal hypercomplex structure within the spacetime metric, allowing a reformulation of gravity that preserves local consistency and the standard relativistic limit while avoiding Ostrogradsky-type instabilities. The present record synthesizes successive versions of the model, including the initial formulation (2015), a comprehensive theoretical update (2025), and recent additions addressing critical discussions. In a cosmological context, the model leads to a holographic-like behavior characterized by a late-time geometric component compatible with current observational constraints from the Cosmic Microwave Background and large-scale structure data. This deposit includes the Lagrangian formulation, the field equations, and numerical implementations based on a modified version of standard cosmology codes, and is released within an open science framework to ensure long-term accessibility, reproducibility, and citation. Keywords: general relativity, modified gravity, hypercomplex geometry, cosmology, theoretical physics. Objective The goal of this development is to refine the internal structure of Hypercomplex General Relativity and determine whether quantization of the internal sector is physically necessary or conceptually supportive. The previous classical formulation introduced a curvature-dependent threshold controlling local gravitational corrections. The present work reinterprets this threshold in terms of a canonical internal gauge structure. 1. Canonical Structure of the Internal Sector The hypercomplex connection is modeled as a non-abelian gauge field. A full Hamiltonian analysis is performed, including: 3+1 decomposition, identification of canonical variables, Gauss constraint implementation, well-defined phase space. The non-commutative structure emerges from the symplectic form and canonical commutation relations, rather than being assumed. This establishes that the internal HGR sector possesses a legitimate gauge-theoretic foundation. 2. Construction of a Gauge-Invariant Internal Observable A scalar observable is constructed from quadratic electric-like and magnetic-like internal invariants. This observable: is locally gauge invariant, is positive definite, can be promoted to an operator, controls the effective gravitational correction threshold. The threshold becomes state-dependent via expectation values, introducing a statistical interpretation of rebound domains. 3. Semi-Classical Regime In a semi-classical approximation, fluctuations of the internal observable modify the effective threshold. This implies that: internal quantum variance may broaden the population of rebound-triggering domains, the mechanism admits a probabilistic interpretation at high curvature. However, the core rebound mechanism does not rely strictly on quantization. 4. Internal Saturation Mechanism A critical issue arises: without regulation, the internal scalar could grow unbounded at high curvature. To ensure stability, a saturation function is introduced: the internal response becomes bounded, corrections remain finite, ultraviolet divergence is avoided, local activation remains possible. This mechanism stabilizes the theory without requiring full quantum gravity. 5. Conceptual Status at the End of This Stage Established: Canonical internal gauge structure. Well-defined observable controlling corrections. Dynamically bounded internal response. Stabilized domain-triggered rebound mechanism. Not yet addressed: Full quantization of gravity. Complete cosmological perturbation analysis. Weak-field post-Newtonian constraints. Strategic Insight Quantization of the internal sector provides micro-structural grounding and theoretical elegance. However, the macroscopic consistency of HGR does not depend on full gravitational quantization. The saturation mechanism alone is sufficient to ensure stability and physical viability. This stage transforms HGR from an intuitive hypercomplex extension into a symplectically structured, dynamically regulated gravitational framework. ========================================== Appendix: HGR: Beginning of quantization. Appendix: Dark matter galaxies or halos and rotation speed, Dark matter-dominated galaxies, Hypercomplex halos in HGR. Weakless interaction between dark matter H0 equation. 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Programming language Python Development Status Active 4K Views 16K Downloads Show more details All versions This version Views Total views 3,926 54 Downloads Total downloads 16,004 910 Data volume Total data volume 15.9 GB 581.3 MB More info on how stats are collected.... Versions External resources Indexed in OpenAIRE Communities Keywords and subjects Keywords Hypercomplex and quaternionic geometric structures General relativity extension Symplectic formulation of gravity Weyl geometry and scale invariance Hamiltonian consistency of modified gravity Geometric stability of higher-order theories Cosmological solutions in extended relativistic frameworks Dark matter Hubble calculation Details DOI DOI Badge DOI 10.5281/zenodo.20106777 Markdown [![DOI](https://zenodo.org/badge/DOI/10.5281/zenodo.20106777.svg)](https://doi.org/10.5281/zenodo.20106777) reStructuredText .. image:: https://zenodo.org/badge/DOI/10.5281/zenodo.20106777.svg :target: https://doi.org/10.5281/zenodo.20106777 HTML <a href="https://doi.org/10.5281/zenodo.20106777"><img src="https://zenodo.org/badge/DOI/10.5281/zenodo.20106777.svg" alt="DOI"></a> Image URL https://zenodo.org/badge/DOI/10.5281/zenodo.20106777.svg Target URL https://doi.org/10.5281/zenodo.20106777 Resource type Journal article Publisher Zenodo Published in Hypercomplex General Relativity (HGR): A symplectic and geometric reformulation of Weyl, hypercomplex numbers with late cosmological applications., 2026. Conference 371 Relativité générale hypercomplexe (RGH) : une reformulation symplectique et géométrique de Weyl, nombres hypercomplexes et applications cosmologiques récentes. Annexe : RGH : début de la quantification. Annexe : Galaxies ou halos de matière noire et vitesse de rotation, galaxies dominées par la matière noire et halos hypercomplexes en RGH. Interaction faible entre la matière noire et l'équation H₀. Languages French Rights License Creative Commons Attribution 4.0 International The Creative Commons Attribution license allows re-distribution and re-use of a licensed work on the condition that the creator is appropriately credited. 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