{"title":"Reevaluating H 0 tension with non-Planck CMB and DESI BAO joint analysis","authors":"Ye-Huang Pang, Xue Zhang, Qing-Guo Huang","doi":"10.1088/1475-7516/2025/04/057","DOIUrl":null,"url":null,"abstract":"<italic toggle=\"yes\">H</italic>\n<sub>0</sub> tension in the spatially flat ΛCDM model is reevaluated by employing three sets of non-<italic toggle=\"yes\">Planck</italic> CMB data, namely WMAP, WMAP+ACT, and WMAP+SPT, in conjunction with DESI BAO data and non-DESI BAO datasets including 6dFGS, SDSS DR7, and SDSS DR16. Our analysis yields <italic toggle=\"yes\">H</italic>\n<sub>0</sub> = 68.86 ± 0.68 km s<sup>-1</sup> Mpc<sup>-1</sup> with WMAP+DESI BAO, <italic toggle=\"yes\">H</italic>\n<sub>0</sub> = 68.72 ± 0.51 km s<sup>-1</sup> Mpc<sup>-1</sup> with WMAP+ACT+DESI BAO, and <italic toggle=\"yes\">H</italic>\n<sub>0</sub> = 68.62 ± 0.52 km s<sup>-1</sup> Mpc<sup>-1</sup> with WMAP+SPT+DESI BAO.\nThe results of non-<italic toggle=\"yes\">Planck</italic> CMB+DESI BAO exhibit a 3.4<italic toggle=\"yes\">σ</italic>, 3.7<italic toggle=\"yes\">σ</italic>, and 3.8<italic toggle=\"yes\">σ</italic> tension with the SH0ES local measurement respectively which are around 1<italic toggle=\"yes\">σ</italic> lower in significance for the Hubble tension compared to <italic toggle=\"yes\">Planck</italic> CMB+DESI BAO.\nMoreover, by combining DESI BAO data+non-<italic toggle=\"yes\">Planck</italic> CMB measurements, we obtain a more stringent constraint on the Hubble constant compared to non-DESI BAO data+non-<italic toggle=\"yes\">Planck</italic> CMB data, as well as reducing the significance of the Hubble tension.","PeriodicalId":15445,"journal":{"name":"Journal of Cosmology and Astroparticle Physics","volume":"17 1","pages":""},"PeriodicalIF":5.3000,"publicationDate":"2025-04-22","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Cosmology and Astroparticle Physics","FirstCategoryId":"101","ListUrlMain":"https://doi.org/10.1088/1475-7516/2025/04/057","RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0
Abstract
H0 tension in the spatially flat ΛCDM model is reevaluated by employing three sets of non-Planck CMB data, namely WMAP, WMAP+ACT, and WMAP+SPT, in conjunction with DESI BAO data and non-DESI BAO datasets including 6dFGS, SDSS DR7, and SDSS DR16. Our analysis yields H0 = 68.86 ± 0.68 km s-1 Mpc-1 with WMAP+DESI BAO, H0 = 68.72 ± 0.51 km s-1 Mpc-1 with WMAP+ACT+DESI BAO, and H0 = 68.62 ± 0.52 km s-1 Mpc-1 with WMAP+SPT+DESI BAO.
The results of non-Planck CMB+DESI BAO exhibit a 3.4σ, 3.7σ, and 3.8σ tension with the SH0ES local measurement respectively which are around 1σ lower in significance for the Hubble tension compared to Planck CMB+DESI BAO.
Moreover, by combining DESI BAO data+non-Planck CMB measurements, we obtain a more stringent constraint on the Hubble constant compared to non-DESI BAO data+non-Planck CMB data, as well as reducing the significance of the Hubble tension.
期刊介绍:
Journal of Cosmology and Astroparticle Physics (JCAP) encompasses theoretical, observational and experimental areas as well as computation and simulation. The journal covers the latest developments in the theory of all fundamental interactions and their cosmological implications (e.g. M-theory and cosmology, brane cosmology). JCAP''s coverage also includes topics such as formation, dynamics and clustering of galaxies, pre-galactic star formation, x-ray astronomy, radio astronomy, gravitational lensing, active galactic nuclei, intergalactic and interstellar matter.