Some anisotropic spatially-homogeneous cosmological models with electromagnetic field
| dc.contributor.author | Singh T.; Srivastava R.S. | |
| dc.date.accessioned | 2025-05-24T09:55:33Z | |
| dc.description.abstract | Considering Bianchi type-I metric, cosmological models of a perfect fluid with an electromagnetic field have been obtained, using a supplementary condition between the metric potentials. The four-current is either zero or space-like. The model has expanding and shearing but non-rotating fluid flow which is also geodetic. The requirement of positive conductivity imposes an additional restriction on the model. Various physical and mathematical properties of the model have been discussed. © 1989 Kluwer Academic Publishers. | |
| dc.identifier.doi | https://doi.org/10.1007/BF00640484 | |
| dc.identifier.uri | http://172.23.0.11:4000/handle/123456789/19942 | |
| dc.relation.ispartofseries | Astrophysics and Space Science | |
| dc.title | Some anisotropic spatially-homogeneous cosmological models with electromagnetic field |