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...

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Detalles Bibliográficos
Autores principales: Geng, Chao-Qiang, Hsu, Yan-Ting, Lu, Jhih-Rong
Formato: Online Artículo Texto
Lenguaje:English
Publicado: MDPI 2021
Materias:
Article
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

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8534870/
https://www.ncbi.nlm.nih.gov/pubmed/34682044
http://dx.doi.org/10.3390/e23101320

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