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Interacting Tsallis holographic dark energy in higher dimensional cosmology

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Abstract

We discuss Tsallis holographic dark energy (THDE) model in higher dimension. An interacting dark energy model is proposed with Generalized Chaplygin Gas (GCG) in the framework of Compact Kaluza-Klein gravity. It is shown that a stable configuration can be found in the present epoch which is also compatible with the observed value of the density parameter. It is noted that dark energy (DE) might have evolved from a phantom phase in the past. Nature of dark energy is found to depend on the coupling parameter of the interaction. Classical stability consideration is also found to put an upper bound on the model parameter.

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Acknowledgements

SG would like to acknowledge the kind hospitality provided by Harish-Chandra Research Institute, HBNI, Department of Atomic Energy, Government of India, for supporting his visit (during which a part of this research work has been carried out) through the plan budget of Cosmology and High Energy Astrophysics grant.

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Authors and Affiliations

  1. Physics Department, Jalpaiguri Government Engineering College, Jalpaiguri, West Bengal, 73510, India

    A. Saha

  2. HECRC, University of North Bengal, Rajarammohunpur, Darjeeling, West Bengal, 734013, India

    S. Ghose

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  1. A. Saha
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  2. S. Ghose
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Correspondence to S. Ghose.

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Saha, A., Ghose, S. Interacting Tsallis holographic dark energy in higher dimensional cosmology. Astrophys Space Sci 365, 98 (2020). https://doi.org/10.1007/s10509-020-03812-7

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