Axially symmetric non-static domain walls in scalar–tensor theories of gravitation |
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Authors: | K S Adhav A S Nimkar R L Naidu |
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Institution: | (1) Department of Mathematics, S.G.B. Amravati University, 444 602 Amravati, India;(2) Department of Mathematics, GMR Institute of Technology, Rajam, India |
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Abstract: | An axially symmetric non-static space-time is considered in the presence of thick domain walls in the scalar–tensor theories
formulated by Brans and Dicke (Phys. Rev. 124:925, 1961) and Saez and Ballester (Phys. Lett. A 113:467, 1985). Exact cosmological models, in both the theories, are presented with the help of special law of variation proposed by Berman
(Nuovo Cim. B 74:182, 1983), for Hubble’s parameter. Some physical and kinematical properties of the models are discussed.
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Keywords: | Scalar– tensor theories Domain walls Hubble’ s parameter |
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