Cosmic no-hair conjecture in scalar-tensor theories
| dc.contributor.author | Singh T.; Chaubey R. | |
| dc.date.accessioned | 2025-05-24T09:57:48Z | |
| dc.description.abstract | We have shown that, within the context of scalar-tensor theories, the anisotropic Bianchi-type cosmological models evolve towards de Sitter Universe. A similar result holds in the case of cosmology in Lyra, manifold. Thus the analogue of cosmic no-hair theorem of Wald [1] hold in both the cases. In fact, during inflation there is no difference between scalar-tensor theories, Lyra's manifold and general relativity (GR). © Indian Academy of Sciences. | |
| dc.identifier.doi | https://doi.org/10.1007/s12043-006-0021-1 | |
| dc.identifier.uri | http://172.23.0.11:4000/handle/123456789/22551 | |
| dc.relation.ispartofseries | Pramana - Journal of Physics | |
| dc.title | Cosmic no-hair conjecture in scalar-tensor theories |