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The combination of Baryonic Acoustic Oscillation (BAO) data together with light element abundance measurements from Big Bang Nucleosynthesis (BBN) has been shown to constrain the cosmological expansion history to an unprecedented degree.
1904
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1904
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1906
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1907
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L. Verde, T. Treu, and A. G. Riess, Tensions between the Early and the Late Universe
1907
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N. Schöneberg, J. Lesgourgues, and D. C. Hooper, The BAO+BBN take on the Hubble tension
1907
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L. Knox and M. Millea, Hubble constant hunter’s guide
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D. J. Eisenstein and W. Hu, Baryonic features in the matter transfer function
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K. Jedamzik and L. Pogosian, Relieving the Hubble tension with primordial magnetic fields
2004
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M. M. Ivanov, Y. Ali-Haïmoud, and J. Lesgourgues, H0 tension or T0 tension?
2005
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2007
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2007
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2007
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2007
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2018
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2018
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2018
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2019
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V. Mossa et al., The baryon density of the Universe from an improved rate of deuterium burning
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2008
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2009
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L. Verde, P. Protopapas, and R. Jimenez, Planck and the local Universe: Quantifying the tension
2013
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2013
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2014
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E. Aubourg et al., Cosmological implications of baryon acoustic oscillation measurements
2015
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2015
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A. G. Riess et al., A 2.4% Determination of the Local Value of the Hubble Constant
2016
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2020
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W. L. Freedman, Measurements of the Hubble Constant: Tensions in Perspective
2021
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2021
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PhD thesis, RWTH Aachen U., 2021
N. Schöneberg, Anomalies in cosmological data and probes of the dark sector · 2021
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2021
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2021
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2022
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2022
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2022
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2022
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S. Gariazzo, P. F. de Salas, O. Pisanti, and R. Consiglio, PArthENoPE revolutions
2022
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2022
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2022
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