The distinctions between $\Lambda$CDM and $f(T)$ gravity according Noether symmetry
Han Dong, Jiaxin Wang, Xinhe Meng

TL;DR
This paper uses Noether symmetry to analyze different $f(T)$ gravity models, finding that the optimal form closely resembles $ ext{Lambda}$CDM but with notable differences, especially in conserved quantities and symmetries.
Contribution
It introduces a systematic Noether symmetry approach to identify the most suitable $f(T)$ models that mimic $ ext{Lambda}$CDM and highlights key differences in symmetries and conserved quantities.
Findings
The optimal $f(T)$ form is $ ext{alpha} T + eta T^{-1}$.
Power-law and exponential forms are less effective.
Significant differences in symmetries between $ ext{Lambda}$CDM and $f(T)$ gravity.
Abstract
Noether's theory offers us a useful tool to research the conserved quantities and symmetries of the modified gravity theories, among which the theory, a generally modified teleparallel gravity, has been proposed to account for the dark energy phenomena. By the Noether symmetry approach, we investigate the power-law, exponential and polynomial forms of theories. All forms of concerned in this work possess the time translational symmetry, which is related with energy condition or Hamilton constraint. In addition, we find out that the performances of the power-law and exponential forms are not pleasing. It is rational adding a linear term to as the most efficient amendment to resemble the teleparallel gravity or General Relativity on small scales, ie., the scale of the solar system. The corresponding Noether symmetry indicates that only time translational…
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