Feb 16, 2025

Study of Dynamic Structure of Galaxies

Study of Dynamic Structure of Galaxies
  • Tsutomu Kambe1,
  • Masanori Hashiguchi2
  • 1University of Tokyo (Former Professor);
  • 2Guest Scholar at MIMS, Meiji University, Tokyo, Japan.
  • Tsutomu Kambe: Guest Scholar at MIMS, Meiji University, Tokyo, Japan. MIMS=Meiji Institute for Advanced Study of Mathematical Science e-mail: [email protected];
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Protocol CitationTsutomu Kambe, Masanori Hashiguchi 2025. Study of Dynamic Structure of Galaxies. protocols.io https://dx.doi.org/10.17504/protocols.io.kqdg3qboqv25/v1
Manuscript citation:
License: This is an open access  protocol  distributed under the terms of the  Creative Commons Attribution License,  which permits unrestricted use, distribution, and reproduction in any medium, provided the original author and source are credited
Protocol status: Working
We use this protocol and it's working
Created: January 16, 2025
Last Modified: February 16, 2025
Protocol  Integer ID: 118544
Keywords: rotating galaxy, dynamical unfolding within galaxy, spiral galaxy, galaxy, galactic space, typical galaxy, outer parts of galaxy, dark matter effect, general relativity theory, general relativity, relativistic theory, existence of fluid lorentz force, fluid lorentz force, new force of fluid lorentz force, orbital hyperspeed of order, dynamical structure, matter effect, fluid dynamic, study of dynamic structure, dynamical unfolding, dynamic structure, orbital hyperspeed, flat rotation curve
Abstract
Present study investigates physical mechanisms and dynamical interplays of the galaxies, on the basis of the general theory of relativity and Fluid Mechanics. Before starting our study, the following two well-known facts are particularly noted:
Main part: Scenario of the present study and Theoretical formulation.