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Higher-dimensional Bianchi type-I dark energy models with barotropic fluid in Saez-Ballester scalar-tensor theory of gravitation

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Abstract

In this paper, we have explored the features of the five-dimensional Bianchi type-I cosmological universe filled with barotropic fluid and dark energy within the framework of Saez-Ballester theory of gravitation. Field equations have been solved by assuming the different functional forms of metric potentials, i.e., \( A=B=C=t^{n}\) and \(D=t^{n_{1}}\). The value of the equation of state parameter and other kinematical parameters have been obtained for both interacting and non-interacting scenarios. The characteristics of physicals parameters are also explained. The obtained results are compatible with the recent observational data.

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Authors and Affiliations

  1. Department of Mathematics and Statistics, University College of Science M.L. Sukhadia University, Udaipur, 313001, India

    Diksha Trivedi & A. K. Bhabor

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  1. Diksha Trivedi
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  2. A. K. Bhabor
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Correspondence to Diksha Trivedi.

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Trivedi, D., Bhabor, A.K. Higher-dimensional Bianchi type-I dark energy models with barotropic fluid in Saez-Ballester scalar-tensor theory of gravitation. Indian J Phys 97, 1317–1327 (2023). https://doi.org/10.1007/s12648-022-02448-3

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