Interacting Tisallis holographic dark energy: the explanation of the accelerated universe

Document Type : Full length research Paper

Author

1Department of Physics, Sirjan University of Technology, P.O. Box 7813733385, Sirjan, Iran

Abstract

Holographic dark energy model with the particle horizon, , as the infrared (IR) cutoff cannot explain an accelerated universe and it is in contradiction with cosmological data. However, this problem will be solved if the particle horizon is replaced by the future event horizon. In this paper, we show that the Tsallis holographic dark energy model with the future event horizon as the IR cutoff can reproduce the accelerated universe and it is one of the main features of the Tsallis holographic dark energy model compared to the usual holographic dark energy model. We study the cosmological perturbation theory for this dark energy model and find it to be stable against perturbation. Since the Tsallis holographic dark energy with assuming interaction between dark energy and dark matter can solve the coincidence problem, we consider the interacting Tsallis dark energy model and investigate the evolution of cosmological parameters. We also find out that the considered model can describe the accelerated expansion of the universe and show that the universe transit from the decelerated to the accelerated phase which is consistent with the cosmological observations.

Keywords

References

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Journal of Research on Many-body Systems
Volume 12, Issue 1 - Serial Number 32
spring 2022
June 2022
Pages 147-163

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History

  • Receive Date: 04 September 2021
  • Revise Date: 30 October 2021
  • Accept Date: 23 November 2021

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