Test to early dark energy models using the Hubble expansion rate

In this work, we present two independent metrics to compute today’s value of the Hubble parameter Ho.Firstly, we implement the median statistics, a robust method unaffected by outliers and variations in thedata distribution. Under only a few assumptions and a large dataset of Ho, built from differe...

詳細記述

書誌詳細

主要な著者:	García, Luz Ángela, Castañeda, Leonardo
フォーマット:	Online
言語:	spa
出版事項:	Universidad Pedagógica y Tecnológica de Colombia 2022
主題:	Energía Oscura, Cosmología, Tensión de Hubble, Inferencia Bayesiana. Dark Energy, Cosmology, Hubble tension, Bayesian Inference. 2
オンライン･アクセス:	https://revistas.uptc.edu.co/index.php/ciencia_en_desarrollo/article/view/15216