The observational constraints on the flat [Formula: see text] CDM models

Most dark energy models have the [Formula: see text] CDM as their limit, and if future observations constrain our universe to be close to [Formula: see text] CDM Bayesian arguments about the evidence and the fine-tuning will have to be employed to discriminate between the models. Assuming a baseline...

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Detalles Bibliográficos
Autores principales: Avsajanishvili, Olga, Huang, Yiwen, Samushia, Lado, Kahniashvili, Tina
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Springer Berlin Heidelberg 2018
Materias:
Regular Article - Theoretical Physics
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6413532/
https://www.ncbi.nlm.nih.gov/pubmed/30956562
http://dx.doi.org/10.1140/epjc/s10052-018-6233-y

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6413532/
https://www.ncbi.nlm.nih.gov/pubmed/30956562
http://dx.doi.org/10.1140/epjc/s10052-018-6233-y

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