Neural Networks and Rules-based Systems used to Find Rational and Scientific Correlations between being Here and Now with Afterlife Conditions
Neural Networks and Rules-based Systems used to Find Rational and
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This study is a novel approach to the cosmological issue of the dark matter effect observed in gas-dominated galaxies in rotation. A possible physical mechanism is investigated to produce the hyper orbital-speeds in outer halo parts of galaxies. In the galactic space, gas clouds are abundant. Motion of the gas-clouds is viewed as a flow of a continuous fluid in curved space with gravity. Dynamical motions of the space-fluid are studied by Fluid Dynamics extended to the one of a relativistic gravitational field. The fluid flow to be studied in relativistic gravity field is reinforced by the fluid gauge theory equipped with a background (dark) gauge field. The stress-energy tensor in the general relativity is revised to take account of intrinsic nature of stress field by generalizing the isotropic pressure to an anisotropic stress field. Present study takes a new double-sided approach both dynamically and physically. Namely a gauge-field is newly incorporated in the system as a dynamical term, and the system is studied under a new mechanism of the anisotropic stress fields.
Tsutomu Kambe. 2026. \u201cUnlocking Galactic Mysteries: Relativistic Insight into Orbital Hyper-Speeds and Dark Matter in Gas-Rich Galactic-Halos\u201d. Global Journal of Science Frontier Research - A: Physics & Space Science GJSFR-A Volume 23 (GJSFR Volume 23 Issue A10): .
Crossref Journal DOI 10.17406/GJSFR
Print ISSN 0975-5896
e-ISSN 2249-4626
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Total Score: 147
Country: Japan
Subject: Global Journal of Science Frontier Research - A: Physics & Space Science
Authors: Tsutomu Kambe, Masanori Hashiguchi (PhD/Dr. count: 0)
View Count (all-time): 135
Total Views (Real + Logic): 1037
Total Downloads (simulated): 29
Publish Date: 2026 01, Fri
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This study is a novel approach to the cosmological issue of the dark matter effect observed in gas-dominated galaxies in rotation. A possible physical mechanism is investigated to produce the hyper orbital-speeds in outer halo parts of galaxies. In the galactic space, gas clouds are abundant. Motion of the gas-clouds is viewed as a flow of a continuous fluid in curved space with gravity. Dynamical motions of the space-fluid are studied by Fluid Dynamics extended to the one of a relativistic gravitational field. The fluid flow to be studied in relativistic gravity field is reinforced by the fluid gauge theory equipped with a background (dark) gauge field. The stress-energy tensor in the general relativity is revised to take account of intrinsic nature of stress field by generalizing the isotropic pressure to an anisotropic stress field. Present study takes a new double-sided approach both dynamically and physically. Namely a gauge-field is newly incorporated in the system as a dynamical term, and the system is studied under a new mechanism of the anisotropic stress fields.
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