标题： 二种关于分箱主样本解释的动力学情景 显示英文标题

标题： Two dynamical scenarios for the binned Master sample interpretation

摘要： 我们分析了晚期宇宙动力学的两种不同情景，这些情景导致哈勃参数偏离$\Lambda$CDM，主要是因为存在一个额外的自由参数，即暗能量参数。 第一个模型包含一个纯粹的演化暗能量范式，它是由膨胀宇宙的引力场产生的。 第二个模型也考虑了演化暗能量与物质成分的相互作用，该相互作用是通过它们的理想能量-动量张量之和守恒来假设的。 然后，使用有效运行哈勃常数的诊断工具，将这两个模型与Ia型超新星所谓的“主样本”的分箱数据进行比较。 基于标准 MCMC 分析的比较程序明显倾向于暗能量 - 物质相互作用模型的数据，该模型与幻影物质状态方程参数（非常接近 -1）相关，当数据自由时（它具有平坦的后验），它是固定的，以重现有效运行哈勃常数的递减幂律行为，这在文献中已经讨论过。 显示英文摘要

摘要： We analyze two different scenarios for the late Universe dynamics, resulting into Hubble parameters deviating from the $\Lambda$CDM, mainly for the presence of an additional free parameter, which is the dark energy parameter. The first model consists of a pure evolutionary dark energy paradigm, as result of its creation by the gravitational field of the expanding Universe. The second model also considers an interaction of the evolutionary dark energy with the matter component, postulated via the conservation of the sum of their ideal energy-momentum tensors. These two models are then compared \textit{via} the diagnostic tool of the effective running Hubble constant, with the binned data of the so-called ``Master sample'' for the Type Ia Supernovae. The comparison procedures, based on a standard MCMC analysis, led to a clear preference of data for the dark energy - matter interaction model, which is associated to a phantom matter equation of state parameter (very close to $-1$) when, being left free by data (it has a flat posterior), it is fixed in order to reproduce the decreasing power-law behavior of the effective running Hubble constant, already discussed in literature.