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The Hubble tension between the $\Lambda$CDM-model-dependent prediction of the current expansion rate $H_0$ using Planck data and direct, model-independent measurements in the local universe from the SH0ES collaboration disagree at $>3.5\sigma$.
1902
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2016
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2016
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2016
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E. Di Valentino, A. Melchiorri, and J. Silk, “Reconciling Planck with the local value of H 0
2016
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J. L. Bernal, L. Verde, and A. G. Riess, “The trouble with H 0
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2018
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A. G. Riess, S. Casertano, W. Yuan, L. Macri, B. Bucciarelli, M. G. Lattanzi, J. W. MacKenty, J. B. Bowers, W. Zheng, A. V. Filippenko, C. Huang, and R. I. Anderson, “Milky Way Cepheid Standards for Measuring Cosmic Distances and Application to Gaia DR2: Implications for the Hubble Constant,” ApJ 861
2018
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E. Di Valentino and S. Bridle, “Exploring the Tension between Current Cosmic Microwave Background and Cosmic Shear Data,” Symmetry
2018
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R. C. Nunes, “Structure formation in f(T) gravity and a solution for H 0
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J. Evslin, A. A. Sen, and Ruchika, “Price of shifting the Hubble constant,” Phys. Rev
2018
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