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Dynamical aspects of anisotropic Bianchi type VI0 cosmological model with dark energy fluid and massive scalar field

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Abstract

In this article, we investigate a spatially homogeneous and anisotropic Bianchi type VI0 cosmological model in the presence of dark energy fluid and an attractive massive scalar field in Einstein’s theory of gravitation. The field equations are solved using the following conditions (1) scalar expansion is proportional to shear scalar of the space time and (2) a power law between the scalar field and the average scale factor of the universe. We have evaluated the cosmological parameters of the model and discussed their dynamical aspects with reference to the recent discovery of accelerated expansion of the universe.

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Acknowledgements

We thank the reviewers and the Editorial team for their positive and constructive comments, which have helped to improve the quality and presentation of the manuscript.

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Authors and Affiliations

  1. Department of Mathematics, GMR Institute of Technology, Rajam, 532127, India

    Y. Aditya

  2. Department of Mathematics, ANITS (A), Visakhapatnam, 531162, India

    K. Deniel Raju

  3. Department of Mathematics, Rajiv Gandhi Memorial College of Engineering and Technology, Nandyal, India

    P. J. Ravindranath

  4. Department of Applied Mathematics, Andhra University, Visakhapatnam, 530003, India

    K. Deniel Raju & D. R. K. Reddy

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  1. Y. Aditya
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  2. K. Deniel Raju
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  3. P. J. Ravindranath
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  4. D. R. K. Reddy
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Correspondence to D. R. K. Reddy.

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Aditya, Y., Raju, K.D., Ravindranath, P.J. et al. Dynamical aspects of anisotropic Bianchi type VI0 cosmological model with dark energy fluid and massive scalar field. Indian J Phys 95, 383–389 (2021). https://doi.org/10.1007/s12648-020-01722-6

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  • DOI: https://doi.org/10.1007/s12648-020-01722-6

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