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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| Format: | Recurso digital |
| Language: | English |
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2026
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| _version_ | 1866901188022108160 |
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| author | Deus, Charles |
| author_facet | Deus, Charles |
| contents | <p>Abstract:<br>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.</p> |
| format | Recurso digital |
| id | zenodo_https___doi_org_10_5281_zenodo_18413644 |
| institution | Zenodo |
| language | eng |
| publishDate | 2026 |
| publisher | Zenodo |
| record_format | zenodo |
| spellingShingle | The Mathematical Formalism of the Deus Cosmological Model: Derivation of the Stress-Energy Tensor and Modified Friedmann Equations for a Viscoelastic Rotating Shell Deus, Charles <p>Abstract:<br>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.</p> |
| title | The Mathematical Formalism of the Deus Cosmological Model: Derivation of the Stress-Energy Tensor and Modified Friedmann Equations for a Viscoelastic Rotating Shell |
| url | https://doi.org/10.5281/zenodo.18413644 |