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1907
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2005
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M. Braglia, W. T. Emond, F. Finelli, A. E. Gumrukcuoglu, and K. Koyama, Unified framework for early dark energy from α \alpha -attractors
Original
2005
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K. Ichikawa and T. Takahashi, Revisiting the constraint on the helium abundance from cmb
2006
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T. Sekiguchi and T. Takahashi, Early recombination as a solution to the H 0 H_{0} tension
Original
2007
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K. Ichikawa, T. Sekiguchi, and T. Takahashi, Probing the Effective Number of Neutrino Species with Cosmic Microwave Background
Original
2008
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K. Ichikawa, T. Sekiguchi, and T. Takahashi, Primordial Helium Abundance from CMB: a constraint from recent observations and a forecast
Original
2008
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T. Sekiguchi, K. Ichikawa, T. Takahashi, and L. Greenhill, Neutrino mass from cosmology: Impact of high-accuracy measurement of the Hubble constant
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2010
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T. Sekiguchi and T. Takahashi, Cosmological bound on neutrino masses in the light of H 0 H_{0} tension
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2011
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O. Pisanti, G. Mangano, G. Miele, and P. Mazzella, Primordial Deuterium after LUNA: concordances and error budget
Original
2011
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2023

Impact of big bang nucleosynthesis on the H0 tension

Takahashi, Tomo, Toda, Yo

Understand

We investigate the impact of big bang nucleosynthesis (BBN) on the Hubble tension, focusing on how the treatment of the reaction rate and observational data affect the evaluation of the tension.

We show that the significance of the tension can vary by $0.8 \sigma$ in some early dark energy model, depending on the treatment of the reaction rate and observational data.
This indicates that how we include the BBN data in the analysis can give a significant impact on the Hubble tension, and we need to carefully consider the assumptions of the analysis to evaluate the significance of the tension when the BBN data is used.