The Tensor Model in the Theory of Locally Relative Expansion (LRAE

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Auteur principal: Jung, Andreas
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Langue:anglais
Publié: Zenodo 2025
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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