Unlocking Galactic Mysteries: Relativistic Insight into Orbital Hyper-Speeds and Dark Matter in Gas-Rich Galactic-Halos

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Tsutomu Kambe
Tsutomu Kambe
2
Masanori Hashiguchi
Masanori Hashiguchi

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GJSFR Volume 23 Issue A10

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Unlocking Galactic Mysteries: Relativistic Insight into Orbital Hyper-Speeds and Dark Matter in Gas-Rich Galactic-Halos Banner
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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.

Funding

No external funding was declared for this work.

Conflict of Interest

The authors declare no conflict of interest.

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No ethics committee approval was required for this article type.

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Not applicable for this article.

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): .

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Relativistic effects in orbit speeds.
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GJSFR Volume 23 Issue A10
Pg. 1- 13
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Crossref Journal DOI 10.17406/GJSFR

Print ISSN 0975-5896

e-ISSN 2249-4626

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GJSFR-A Classification: LCC Code: QB980-991
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v1.2

Issue date

December 25, 2023

Language

English

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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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Unlocking Galactic Mysteries: Relativistic Insight into Orbital Hyper-Speeds and Dark Matter in Gas-Rich Galactic-Halos

Tsutomu Kambe
Tsutomu Kambe
Masanori Hashiguchi
Masanori Hashiguchi

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