Slowly rotating universes with radiating perfect fluid distribution coupled with a scalar field in general relativity (Q1907070)
From MaRDI portal
| This is the item page for this Wikibase entity, intended for internal use and editing purposes. Please use this page instead for the normal view: Slowly rotating universes with radiating perfect fluid distribution coupled with a scalar field in general relativity |
scientific article; zbMATH DE number 839098
| Language | Label | Description | Also known as |
|---|---|---|---|
| English | Slowly rotating universes with radiating perfect fluid distribution coupled with a scalar field in general relativity |
scientific article; zbMATH DE number 839098 |
Statements
Slowly rotating universes with radiating perfect fluid distribution coupled with a scalar field in general relativity (English)
0 references
28 July 1996
0 references
The author generalizes the work of \textit{K. D. Krori} and \textit{A. R. Sheikh} [Can. J. Phys. 61, No. 9, 1324--1327 (1983; Zbl 1371.83042)] for rotating Friedman universes. The effects of radiation and scalar fields on the rotation of models are discussed. Most of the rotating models obtained here turn out to be expanding ones as well.
0 references
rotating Friedman universes
0 references
radiation
0 references
scalar fields
0 references
0 references
0 references