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Reconstructing Tsallis holographic phantom

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Abstract

The current research considers the Tsallis holographic dark energy (THDE) with the Hubble horizon as an IR cut-off with a non-interacting flat Friedmann–Lemaitre–Robertson–Walker (FLRW) Universe. We investigate the evolutionary behaviour of deceleration and the equation of state parameter for the distinct Tsallis exponent \(\delta \) and noticed appropriate behaviour in the model. The scalar field of the phantom describes the non-interacting Tsallis holographic dark energy when \(\delta >2\), then we demonstrate the phantomic narration when \(\delta >2\) for the Tsallis holographic dark energy and reconstruct the scalar field potential of the phantom.

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Acknowledgements

The author would like to thank IUCAA, Pune, India for awarding the visiting associateship.

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Authors and Affiliations

  1. Department of Mathematics, Institute of Applied Sciences and Humanities, GLA University, Mathura, 281 406, India

    Umesh Kumar Sharma

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  1. Umesh Kumar Sharma
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Correspondence to Umesh Kumar Sharma.

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Sharma, U.K. Reconstructing Tsallis holographic phantom. Pramana - J Phys 96, 210 (2022). https://doi.org/10.1007/s12043-022-02460-6

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  • DOI: https://doi.org/10.1007/s12043-022-02460-6

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