http://arxiv.org/abs/2006.01618
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.
A. Saha and S. Ghose
Wed, 3 Jun 20
76/83
Comments: 7 pages, 7 figures, prepared for Astronomy and Space Science. To be published on Astronomy and Space Science