ロード中...
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...
保存先:
| 出版年: | Eur Phys J C Part Fields |
|---|---|
| 主要な著者: | , , , |
| フォーマット: | Artigo |
| 言語: | Inglês |
| 出版事項: |
Springer Berlin Heidelberg
2018
|
| 主題: | |
| オンライン･アクセス: | https://ncbi.nlm.nih.gov/pmc/articles/PMC6413532/ https://ncbi.nlm.nih.gov/pubmed/30956562 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1140/epjc/s10052-018-6233-y |
| タグ: |
タグ追加
タグなし, このレコードへの初めてのタグを付けませんか!
|