Abstract
Axially symmetric cosmological models are obtained in a scalar tensor theory proposed by Sen (Z. Phys. 149:311, 1957) based on Lyra manifold with time dependent β in the presence of string source, perfect fluid distribution, dust distribution and thick domain walls. Some physical and geometrical properties of these models are discussed.
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Rao, V.U.M., Vinutha, T. Axially symmetric cosmological models in a scalar tensor theory based on Lyra manifold. Astrophys Space Sci 319, 161–167 (2009). https://doi.org/10.1007/s10509-008-9971-8
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DOI: https://doi.org/10.1007/s10509-008-9971-8