The Tensor Model in the Theory of Locally Relative Expansion (LRAE
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| Format: | Recurso digital |
| Langue: | anglais |
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2025
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| _version_ | 1866901467240071168 |
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| author | Jung, Andreas |
| author_facet | Jung, Andreas |
| contents | <p>This document introduces a structurally extended formulation of the classical energy-momentum tensor TμνT_{\mu\nu}Tμν, compatible with the Theory of Locally Relative Expansion (LRAE). Unlike the standard relativistic model, the LRAE tensor incorporates the local expansion field ϵ(xμ)\epsilon(x^\mu)ϵ(xμ) and the structural activation components of the structure field f(xμ)f(x^\mu)f(xμ). As a result, gravitational effects only persist where structural modifiability and temporal reference exist. This leads to a reformulated Einstein field equation in which gravitational decoupling of mass (e.g., in black holes) is structurally consistent and mathematically well-defined. The work bridges general relativity with the structural principles of the LRAE and contributes to the deeper understanding of non-interacting matter, such as Element 0.</p> <p> </p> <p>Autorschaft: Andreas Jung<br> Mit Unterstützung durch: KI (ChatGPT, OpenAI)<br> Lizenz: Creative Commons Attribution 4.0 International (CC BY 4.0)<br> Veröffentlichung: Juni 2025<br>Kontakt: andreasjung6502@gmail.com</p> |
| format | Recurso digital |
| id | zenodo_https___doi_org_10_5281_zenodo_15767150 |
| institution | Zenodo |
| language | eng |
| publishDate | 2025 |
| publisher | Zenodo |
| record_format | zenodo |
| spellingShingle | The Tensor Model in the Theory of Locally Relative Expansion (LRAE Jung, Andreas black holes, LRAE, structure field, gravitational decoupling, tensor field theory, spacetime structure, general relativity, Einstein field equations, non-interacting matter <p>This document introduces a structurally extended formulation of the classical energy-momentum tensor TμνT_{\mu\nu}Tμν, compatible with the Theory of Locally Relative Expansion (LRAE). Unlike the standard relativistic model, the LRAE tensor incorporates the local expansion field ϵ(xμ)\epsilon(x^\mu)ϵ(xμ) and the structural activation components of the structure field f(xμ)f(x^\mu)f(xμ). As a result, gravitational effects only persist where structural modifiability and temporal reference exist. This leads to a reformulated Einstein field equation in which gravitational decoupling of mass (e.g., in black holes) is structurally consistent and mathematically well-defined. The work bridges general relativity with the structural principles of the LRAE and contributes to the deeper understanding of non-interacting matter, such as Element 0.</p> <p> </p> <p>Autorschaft: Andreas Jung<br> Mit Unterstützung durch: KI (ChatGPT, OpenAI)<br> Lizenz: Creative Commons Attribution 4.0 International (CC BY 4.0)<br> Veröffentlichung: Juni 2025<br>Kontakt: andreasjung6502@gmail.com</p> |
| title | The Tensor Model in the Theory of Locally Relative Expansion (LRAE |
| topic | black holes, LRAE, structure field, gravitational decoupling, tensor field theory, spacetime structure, general relativity, Einstein field equations, non-interacting matter |
| url | https://doi.org/10.5281/zenodo.15767150 |