Cargando…
Constraining Early Dark Energy with Large-Scale Structure
An axion-like field comprising ∼10% of the energy density of the Universe near matter-radiation equality is a candidate to resolve the Hubble tension; this is the “early dark energy” (EDE) model. However, as shown in Hill et al., the model fails to simultaneously resolve the Hubble tension and maint...
| Autores principales: | , , , , , , |
|---|---|
| Lenguaje: | eng |
| Publicado: |
2020
|
| Materias: | |
| Acceso en línea: | https://dx.doi.org/10.1103/PhysRevD.102.103502 http://cds.cern.ch/record/2723281 |