论文标题
来自Horava-Lifshitz宇宙学的量子标志
Quantum signatures from Horava-Lifshitz cosmography
论文作者
论文摘要
在本文中，我们通过将Horava-Lifshitz重力作为量子重力模型来提出替代宇宙学，以在宇宙学层面寻找量子效应。对于我们的分析，我们考虑了当前的后期宇宙调查和爱因斯坦望远镜的重力波。我们自然地发现了一个非燃料方案，具有$ω_k= -0.021^{+0.023} _ { - 0.029} $，$ h_0 = 71.904^{+1.406} _ { - 1.347} $，没有显示标准$ 3.4 $ $ - $ - $ - $ - $ - $ - $ - 1.347} $。此外，我们获得了HO \ V RAVA参数$ω\左右的特定值-3.8 \ times 10^{ - 14} $，可以将其解释为量子效应的度量，可用于进一步测试该量子重力模型。我们得出的结论是，根据$λ$ CDM模型，我们的宇宙似乎在空间上是平坦的，但实际上，它是从量子的角度弯曲的。
In this paper we propose an alternative cosmography by considering Horava-Lifshitz gravity as a model of quantum gravity to search for quantum effects at the cosmological level. For our analyses we consider current late universe surveys and a Gravitational Waves forecast from Einstein Telescope. We found naturally a non-flat scenario with $Ω_k =-0.021^{+0.023}_{-0.029}$ with $H_0 = 71.904^{+1.406}_{-1.347}$, without showing the standard reported $3.4$-$σ$ inconsistency. Furthermore, we obtained a specific value for the Ho\v rava parameter $ω\approx -3.8\times 10^{-14}$, which can be interpreted as a measure of a quantum effect and could be used to further test this quantum gravity model. We conclude that classically, according to the $Λ$CDM model, our universe seems to be spatially flat, but in fact, it is curved from a quantum point of view.
