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 differen...
- Autores:
- Tipo de recurso:
- Fecha de publicación:
- 2022
- Institución:
- Universidad Pedagógica y Tecnológica de Colombia
- Repositorio:
- RiUPTC: Repositorio Institucional UPTC
- Idioma:
- spa
- OAI Identifier:
- oai:repositorio.uptc.edu.co:001/15374
- Acceso en línea:
- https://revistas.uptc.edu.co/index.php/ciencia_en_desarrollo/article/view/15216
https://repositorio.uptc.edu.co/handle/001/15374
- Palabra clave:
- Energía Oscura, Cosmología, Tensión de Hubble, Inferencia Bayesiana.
Dark Energy, Cosmology, Hubble tension, Bayesian Inference. 2
- Rights
- License
- http://purl.org/coar/access_right/c_abf2