2021
DOI: 10.3847/1538-4357/abeb73
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Abstract: The Hubble constant (H 0) tension between Type Ia supernovae (SNe Ia) and Planck measurements ranges from 4 to 6σ. To investigate this tension, we estimate H 0 in the ΛCDM and w 0 … Show more

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Cited by 232 publications
(117 citation statements)
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“…In reference [1015] a running of H 0 as a function of redshift is proposed to alleviate the Hubble tension, although a full data analysis is missing. A similar idea has been explored in reference [1016] to analyse the Pantheon SNIa data.…”
Section: Running Hubble Tensionmentioning
confidence: 99%
“…In reference [1015] a running of H 0 as a function of redshift is proposed to alleviate the Hubble tension, although a full data analysis is missing. A similar idea has been explored in reference [1016] to analyse the Pantheon SNIa data.…”
Section: Running Hubble Tensionmentioning
confidence: 99%
“…As in Equation ( 20), we realize that the fine-structure constant α plays a role in determining orders of magnitude. By adjusting the exponent of the fine-structure constant α, we obtain a result identical to Equation (29).…”
Section: Precise Calculation Of Hmentioning
confidence: 97%
“…Indeed, Refs. [55][56][57][58][59][60] suggest that a transition in the dark energy equation of state or in the absolute magnitude as a possible solution to the Hubble tension. In addition to the SNIa observations, we also make use of BAO measurements [39-52, 61, 62] in order to take a fuller account of the possible evolution of M B (z).…”
Section: Distance Laddersmentioning
confidence: 99%