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Cosmic no-hair conjecture in scalar-tensor theories

dc.contributor.authorSingh T.; Chaubey R.
dc.date.accessioned2025-05-24T09:57:48Z
dc.description.abstractWe 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.doihttps://doi.org/10.1007/s12043-006-0021-1
dc.identifier.urihttp://172.23.0.11:4000/handle/123456789/22551
dc.relation.ispartofseriesPramana - Journal of Physics
dc.titleCosmic no-hair conjecture in scalar-tensor theories

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