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...

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Bibliografische gegevens

Hoofdauteurs:	García, Luz Ángela, Castañeda, Leonardo
Formaat:	Online
Taal:	spa
Gepubliceerd in:	Universidad Pedagógica y Tecnológica de Colombia 2022
Onderwerpen:	Energía Oscura, Cosmología, Tensión de Hubble, Inferencia Bayesiana. Dark Energy, Cosmology, Hubble tension, Bayesian Inference. 2
Online toegang:	https://revistas.uptc.edu.co/index.php/ciencia_en_desarrollo/article/view/15216