The Mathematical Formalism of the Deus Cosmological Model: Derivation of the Stress-Energy Tensor and Modified Friedmann Equations for a Viscoelastic Rotating Shell

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Authors: Charles Deus
Cited by: 0

Abstract

Abstract:The Deus Cosmological Model (DCM) proposes a paradigm shift from a vacuum-based geometry to a hydrodynamic topology, defining spacetime as a finite, rotating Viscoelastic Superfluid (“The Bulk”). While previous works have established the conceptual framework and phenomenological consequences of this model, this paper provides the rigorous field-theoretic derivation. We construct the specific Relativistic Stress-Energy Tensor (TDeus μν ) for a non-perfect fluid obeying a Kelvin-Voigt constitutive law with global vorticity. By solving the time-component of the Einstein Field Equations for this tensor, we derive the Deus-Friedmann Equation. We demonstrate that the cosmic expansion history H(t) is governed not by a cosmological constant, but by the thermodynamic pressure of a central singularity balanced by bulk viscosity and centrifugal support. Version 3: Corrected dimensional analysis and added rigorous definitions for the solid-state vacuum topology.

Fields of Study & Subjects

Cosmology and Gravitation Theories Relativity and Gravitational Theory Noncommutative and Quantum Gravity Theories

Publication details

Journal / source
Zenodo (CERN European Organization for Nuclear Research)
Publication date
28 January 2026
Language
EN
Document type
Preprint