Cosmological constraints of Palatini f (R) gravity

被引:5
|
作者
Gomes, Debora Aguiar [1 ]
Briffa, Rebecca [2 ,3 ]
Kozak, Aleksander [4 ]
Said, Jackson Levi [2 ,3 ]
Saal, Margus [1 ]
Wojnar, Aneta [5 ,6 ]
机构
[1] Univ Tartu, Inst Phys, Lab Theoret Phys, W Ostwaldi 1, Tartu 50411, Estonia
[2] Univ Malta, Inst Space Sci & Astron, MSD 2080, Msida, Malta
[3] Univ Malta, Dept Phys, MSD 2080, Msida, Malta
[4] Univ Wroclaw, Inst Theoret Phys, Pl Maxa Borna 9, PL-50206 Wroclaw, Poland
[5] Univ Complutense Madrid, Dept Fis Teor, E-28040 Madrid, Spain
[6] Univ Complutense Madrid, IPARCOS, E-28040 Madrid, Spain
关键词
modified gravity; baryon acoustic oscillations; DARK-MATTER; INFLATION; CONSTANT; EXPANSION; DYNAMICS; SAMPLE;
D O I
10.1088/1475-7516/2024/01/011
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In this study, we investigate a Palatini f (R) gravity model featuring a quadratic term correction, aligning it with the most recent expansion rate data, with a particular focus on the latest SNIa and BAO data. Our analysis employs CC data as the fundamental dataset, complemented by contributions from the SN sample and a combination of non -overlapping transversal BAO datasets. We conduct a comprehensive MCMC analysis for each data set combination, yielding constraints on all cosmological parameters within the model. Additionally, we incorporate the latest Hubble constant value from the SH0ES Team. Finally, we present a statistical comparison between the Palatini quadratic model and Lambda CDM using the AIC and BIC metrics, ultimately obtaining the constraint |alpha| <= 1049 m2. We also stress the significance of studying stellar and substellar objects for obtaining more precise constraints on modified gravity compared to those derived from cosmological observations.
引用
收藏
页数:24
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