Gravitational Field of a Self-gravitating Continuous Medium, Dark Matter and Disk Galaxies

A new representation for the field strength of the quasiclassical gravitational field of a continuous medium is proposed, which makes it possible to describe the effect of hidden mass or dark matter in a new way. The connection of the new representation with the properties of a continuous medium and the role of these properties in the formation of the hidden mass effect are discussed. Based on the results obtained, a new model of the structure of disk galaxies and their own evolution under dynamic equilibrium conditions is being investigated. A general classification of possible types of spatial structures of disk galaxies is given. The existence conditions of disk galaxies with bulges and jets, as well as ring structures, are considered. A qualitative analysis of possible variants of the galaxies’ own evolution and the conditions of their spatial oscillations is carried out.

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Publication Details

Journal
Gravitation and Cosmology
Published
2025-09-01
DOI
https://doi.org/10.1134/s0202289325700173
Citations
1
Primary Topic
Stellar, planetary, and galactic studies
Type
article
Field-Weighted Citation Impact
1.15
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article

Gravitational Field of a Self-gravitating Continuous Medium, Dark Matter and Disk Galaxies

V. M. Zhuravlev
1 citations
Gravitation and Cosmology
Stellar, planetary, and galactic studies
1.15
article

Gravitational Field of a Self-gravitating Continuous Medium, Dark Matter and Disk Galaxies

V. M. Zhuravlev
article en
1 citations

Abstract

A new representation for the field strength of the quasiclassical gravitational field of a continuous medium is proposed, which makes it possible to describe the effect of hidden mass or dark matter in a new way. The connection of the new representation with the properties of a continuous medium and the role of these properties in the formation of the hidden mass effect are discussed. Based on the results obtained, a new model of the structure of disk galaxies and their own evolution under dynamic equilibrium conditions is being investigated. A general classification of possible types of spatial structures of disk galaxies is given. The existence conditions of disk galaxies with bulges and jets, as well as ring structures, are considered. A qualitative analysis of possible variants of the galaxies’ own evolution and the conditions of their spatial oscillations is carried out.

Gravitation and CosmologyVol. 31(3)
Ulyanovsk State Pedagogical University (RU)
Openalex Percentile: Top 17%
Stellar, planetary, and galactic studies
1.15
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