Cargando…
Constraints on Non-Flat Starobinsky f(R) Dark Energy Model
We study the viable Starobinsky [Formula: see text] dark energy model in spatially non-flat FLRW backgrounds, where [Formula: see text] with [Formula: see text] and [Formula: see text] representing the characteristic curvature scale and model parameter, respectively. We modify CAMB and CosmoMC packa...
| Autores principales: | , , |
|---|---|
| Formato: | Online Artículo Texto |
| Lenguaje: | English |
| Publicado: |
MDPI
2021
|
| Materias: | |
| Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8534870/ https://www.ncbi.nlm.nih.gov/pubmed/34682044 http://dx.doi.org/10.3390/e23101320 |