Constraining uber gravity with recent observations and studying the H0 problem
Abstract
This paper studies both Î CDM and CDM models under the über gravity theory, named ü Î CDM and üCDM respectively. We report bounds over their parameter phase-space using several cosmological data, in particular, the recent Pantheon+ sample. Based on the joint analysis, the best fit value of the über characteristic parameter is zâ=0.046-0.032+0.047 and zâ=1.382-0.021+0.020 at 68% confidence level for ü Î CDM and üCDM respectively. Although über gravity can successfully mimics the cosmological constant, we find that the H0 (z) diagnostic suggests the H tension is not alleviated. Finally, both models are statistically compared with Î CDM through the Akaike and Bayesian information criteria. Both über gravity models and Î CDM are equally preferred for most of the single samples, in particular, ü Î CDM is not rejected by the CMB data. However, there is strong evidence against them for the joint analysis.
Más información
| Título según WOS: | Constraining uber gravity with recent observations and studying the H0 problem |
| Título según SCOPUS: | Constraining über gravity with recent observations and studying the H problem |
| Título de la Revista: | European Physical Journal C |
| Volumen: | 83 |
| Número: | 5 |
| Editorial: | Springer Nature |
| Fecha de publicación: | 2023 |
| Idioma: | English |
| DOI: |
10.1140/epjc/s10052-023-11596-7 |
| Notas: | ISI, SCOPUS |