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Dark energy-dominated Universe in Lyra geometry

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Abstract

In this paper, we have investigated a spatially homogeneous and isotropic quintessence Universe in Lyra geometry that fits good with latest observations. We consider that the current Universe is filled with the binary mixture of dust and dark energy. We observe that there is a signature flipping from early decelerating to the present accelerating phase due to the appearance of dark energy which is in good agreement with the current observations. It has also been found that the displacement vector \(\beta \) is not responsible for late time acceleration of the Universe. Some physical and geometrical properties of the Universe are also discussed.

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Acknowledgements

We wish to place on record our sincere thanks to the editor and referee for illuminating suggestions that have significantly improved our work in terms of research quality and presentation.

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Authors and Affiliations

  1. Department of Physics, United College of Engineering and Research, Greater Noida, 201310, India

    Anil Kumar Yadav

  2. Department of Mathematics, Netaji Subhas University of Technology, Delhi, India

    G. K. Goswami

  3. Department of Mathematics, Institute of Applied Sciences and Humanities, G L A University, Mathura, 281 406, India

    Anirudh Pradhan

  4. Department of Mathematics, Janata Janardan Inter College, Gandhi Nagar, Ghazipur, 233 225, India

    Sudhir Kumar Srivastava

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  1. Anil Kumar Yadav
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  2. G. K. Goswami
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  3. Anirudh Pradhan
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  4. Sudhir Kumar Srivastava
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Correspondence to Anil Kumar Yadav.

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Yadav, A.K., Goswami, G.K., Pradhan, A. et al. Dark energy-dominated Universe in Lyra geometry. Indian J Phys 96, 1569–1575 (2022). https://doi.org/10.1007/s12648-021-02071-8

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  • DOI: https://doi.org/10.1007/s12648-021-02071-8

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