{"title":"A kinematics-dynamics double test of Hubble tension through the Gaussian processes","authors":"Ming-Jian Zhang , Maoyou Yang, Junmei Wang","doi":"10.1016/j.aop.2025.169934","DOIUrl":null,"url":null,"abstract":"<div><div>Hubble tension is a key problem in cosmology, which may signal a new physics. We perform a kinematics-dynamics double test of Hubble tension through the Gaussian processes. Reconstructions under the two types of <span><math><msub><mrow><mi>H</mi></mrow><mrow><mn>0</mn></mrow></msub></math></span> priors from the current supernovae, transversal baryon acoustic oscillation, Cosmic Chronometers and strong gravitational lensing data indicate that the kinematics jerk and dynamics equation of state of dark energy are consistent with the fiducial <span><math><mi>Λ</mi></math></span>CDM model within 68% confidence level, except at some redshift interval. Importantly, we find that the latter three observational data are sensitive to the Hubble constant, which have a potential to test the Hubble tension. Unfortunately, uncertainties of the current observational data are too large to distinguish the Hubble tension. We make a forecast using the simulated supernovae and strong gravitational lensing data. The supernovae from WFIRST can present a much tighter constraint on the reconstructions. It has a large potential to test the Hubble tension.</div></div>","PeriodicalId":8249,"journal":{"name":"Annals of Physics","volume":"475 ","pages":"Article 169934"},"PeriodicalIF":3.0000,"publicationDate":"2025-01-29","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Annals of Physics","FirstCategoryId":"101","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S0003491625000156","RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"PHYSICS, MULTIDISCIPLINARY","Score":null,"Total":0}
引用次数: 0
Abstract
Hubble tension is a key problem in cosmology, which may signal a new physics. We perform a kinematics-dynamics double test of Hubble tension through the Gaussian processes. Reconstructions under the two types of priors from the current supernovae, transversal baryon acoustic oscillation, Cosmic Chronometers and strong gravitational lensing data indicate that the kinematics jerk and dynamics equation of state of dark energy are consistent with the fiducial CDM model within 68% confidence level, except at some redshift interval. Importantly, we find that the latter three observational data are sensitive to the Hubble constant, which have a potential to test the Hubble tension. Unfortunately, uncertainties of the current observational data are too large to distinguish the Hubble tension. We make a forecast using the simulated supernovae and strong gravitational lensing data. The supernovae from WFIRST can present a much tighter constraint on the reconstructions. It has a large potential to test the Hubble tension.
期刊介绍:
Annals of Physics presents original work in all areas of basic theoretic physics research. Ideas are developed and fully explored, and thorough treatment is given to first principles and ultimate applications. Annals of Physics emphasizes clarity and intelligibility in the articles it publishes, thus making them as accessible as possible. Readers familiar with recent developments in the field are provided with sufficient detail and background to follow the arguments and understand their significance.
The Editors of the journal cover all fields of theoretical physics. Articles published in the journal are typically longer than 20 pages.