Lagrangian reconstruction of Barrow holographic dark energy in interacting tachyon model

Abstract

We consider a correspondence between the tachyon dark energy model and Barrow holographic dark energy (BHDE). The latter is a modified scenario based on the application of the holographic principle with Barrow entropy instead of the usual Bekenstein-Hawking one. We reconstruct the dynamics of the tachyon scalar field $T$ in a curved Friedmann-Robertson-Walker Universe both in the presence and absence of interactions between dark energy and matter. As a result, we show that the tachyon field exhibits a non-trivial dynamics. In a flat Universe, ${\dot{T}}^2$ must always be vanishing, independently of the existence of interaction. This implies ${\omega }_D=-1$ for the equation-of-state parameter, which in turn can be used for modeling the cosmological constant behavior. On the other hand, for a non-flat Universe and various values of Barrow parameter, we find that ${\dot{T}}^2$ decreases monotonically for increasing $\cos (R_h/a)$ and $\cosh (R_h/a)$, where $R_h$ and $a$ are the future event horizon and the scale factor, respectively. Specifically, ${\dot{T}}^2\ge 0$ for a closed Universe, while ${\dot{T}}^2<0$ for an open one, which is physically not allowed. We finally comment on the inflation mechanism and Trans-Planckian Censorship Conjecture in BHDE and discuss observational consistency of our model.

arXiv comment16 pages, 5 figures (substantial changes to v2, including Fig.3, Fig.4 and Fig.5), accepted for publication on Symmetry, Special Issue "Noether Symmetries in Gravitation and Cosmology"

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