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Bianchi-type cosmological models in Lyra's geometry with constant deceleration parameter
| dc.contributor.author | Singh T.; Agrawal A.K. | |
| dc.date.accessioned | 2025-05-24T09:57:19Z | |
| dc.description.abstract | The Bianchi-type cosmological models have been studied in Lyra's geometry for a law of variation of Hubble's parameter presented by Berman (1983) that yields constant deceleration parameter models of the universe. All the models have a singular origin (t = 0) and evolve with time. The gauge function \(t) is an arbitrary function of time. © 1993 Società Italiana di Fisica. | |
| dc.identifier.doi | https://doi.org/10.1007/BF02742810 | |
| dc.identifier.uri | http://172.23.0.11:4000/handle/123456789/22035 | |
| dc.relation.ispartofseries | Il Nuovo Cimento B Series 11 | |
| dc.title | Bianchi-type cosmological models in Lyra's geometry with constant deceleration parameter |