论文标题
一个新的耦合三型深色能模型及其对$ H_0 $张力的影响
A new coupled three-form dark energy model and implications for the $H_0$ tension
论文作者
论文摘要
我们提出了一个新的耦合三型深色能模型，以减轻本文中哈勃张力。首先，通过使用耦合的三型深色能模型进行动态分析，我们获得了四个固定点，包括一个代表辐射主导的宇宙的鞍点，一个代表物质主导宇宙的鞍点，以及两个代表两个饱和的De de Sitter Universes的吸引者。其次，通过面对具有宇宙微波背景（CMB），Baryonic声学振荡（BAO）（BAO），IA Supernovae（IA SuperNovae（SN IA）型（SN IA）观察，我们获得$ H_0 = 67.8.8 __的$ 1-67.8 _____-级别）km/s/mpc，用于耦合的三型深色能模型和$ h_0 = 67.6 _ { - 0.5}^{+0.5} $（$1σ$级别）km/s/s/s/mpc的$λ$ $ cdm的$ cdm型号与最新级别的$ 4.3 $ 4.3 $ 4.3 $ cdmentive in_0 $ 4.3Scys in_0 $ 4.3Scys in_0 $ 4.3Scys in_0 $4.3σ $ H_0 $值$5.1σ$级别。
We propose a new coupled three-form dark energy model to relieve the Hubble tension in this paper. Firstly, by performing a dynamical analysis with the coupled three-form dark energy model, we obtain four fixed points, including a saddle point representing a radiation dominated Universe, a saddle point representing a matter dominated Universe, and two attractors representing two saturated de Sitter Universes. Secondly, by confronting the coupled three-form dark energy model and the $Λ$ cold dark matter model (the $Λ$CDM model) with cosmic microwave background (CMB), baryonic acoustic oscillations (BAO), Type Ia supernovae (SN Ia) observations, we obtain $H_0= 67.8_{-0.6}^{+0.7}$($1σ$ level) km/s/Mpc for the coupled three-form dark energy model and $H_0=67.6_{-0.5}^{+0.5}$($1σ$ level) km/s/Mpc for the $Λ$CDM model, the former is in strong tension with the latest local measured $H_0$ value at $4.3σ$ confidence level, while the latter is in strong tension with the latest local measured $H_0$ value at $5.1σ$ level.
