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arXiv · 2308.00342

Reconstruction of aether scalar tensor theory for various cosmological scenarios

Qi-Ming Fu·Meng-Ci He·Tao-Tao Sui·Xin Zhang
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Abstract

In this paper, we present several explicit reconstructions for {the aether scalar tensor (AeST) theory} derived from the background of Friedmann-Lema$\hat{\text{\i}}$tre-Robertson-Walker cosmological evolution. It is shown that the Einstein-Hilbert Lagrangian with a positive cosmological constant is the only Lagrangian capable of accurately replicating the exact expansion history of the $\Lambda$ cold dark matter ($\Lambda$CDM) universe filled solely with dust-like matter. However, the $\Lambda$CDM-era can be produced within the framework of the AeST theory for some other fluids, including a perfect fluid with $p=-(1/3)\rho$, multifluids, and nonisentropic perfect fluids. Moreover, we demonstrate that the $\Lambda$CDM-era also can be replicated with no real matter field for the AeST theory. The cosmic evolution resulting from both the power-law and de-Sitter solutions also can be obtained.

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Qi-Ming Fu, Meng-Ci He, Tao-Tao Sui, Xin Zhang. 2023-08-01. Reconstruction of aether scalar tensor theory for various cosmological scenarios. https://arxiv.org/abs/2308.00342

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