Investigating The Hubble Tension Through Hubble Parameter Data
نویسندگان
چکیده
The Hubble constant ($H_0$), which represents the expansion rate of Universe, is one most important cosmological parameters. recent measurements $H_0$ using distance ladder methods such as Type Ia Supernovae (SNe Ia) are significantly greater than CMB by Planck. difference points to a crisis in standard model cosmology termed tension. In this work we compare different models, determine and comment on tension data from differential ages galaxies. use free systematic effects absolute age estimation galaxies not needed. We have used Bayesian approach along with commonly maximum likelihood method estimate calculated AIC scores models.The non-flat provides higher value for matter density well compared flat $\Lambda$CDM model. score smaller indicating better choice. best-fit both these models $68.7\pm3.1$ km/s/Mpc $72.2\pm4$ km/s/Mpc, respectively. Our results consistent CCHP measurements. However, result does agree SH0ES result, while inconsistent Planck value.
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ژورنال
عنوان ژورنال: Research in Astronomy and Astrophysics
سال: 2023
ISSN: ['1674-4527', '2397-6209']
DOI: https://doi.org/10.1088/1674-4527/acd0e8