In this work we present a further investigation about Teleparallel Gravity Cosmology. We demonstrate that according the current astrophysical data (CC+Pantheon+BAO samplers with late universe measurements SH0ES+H0LiCOW), an $f(T,B)$ theory can provide another interpretation to the oscillatory behaviour of the dark energy equation of state when applied to late times. The four $f(T,B)$ cosmological viable models proposed here can undergo an epoch of late-time acceleration and reproduce quintessence and phantom regimes with a transition along the phantom-divided line, making this theory a good approach to modify the standard $\Lambda$CDM model.

中文翻译：

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f ( T , B ) 理论中的宇宙学可行模型作为H ₀张力的解决方案

在这项工作中，我们对遥平行引力宇宙学进行了进一步的研究。我们证明，根据当前的天体物理数据（CC+Pantheon+BAO 采样器与晚期宇宙测量 SH0ES+H0LiCOW），$f(T,B)$ 理论可以为暗能量状态方程的振荡行为提供另一种解释，当适用于后期。这里提出的四个 $f(T,B)$ 宇宙学可行模型可以经历一个后期加速时代，并通过沿着幻影分割线的过渡重现精髓和幻影状态，使该理论成为修改标准的好方法$\Lambda$CDM 模型。