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Local measurements of the Hubble parameter are increasingly in tension with the value inferred from a $\Lambda$CDM fit to the cosmic microwave background (CMB) data.
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J. Lesgourgues, “The Cosmic Linear Anisotropy Solving System (CLASS) I: Overview,” arXiv e-prints
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S. X. Tian and Z.-H. Zhu, “Early dark energy in k k -essence,” Phys. Rev. D
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L. Perivolaropoulos and F. Skara, “Challenges for Λ \Lambda CDM: An update,” New Astron. Rev
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K. Kojima and Y. Okubo, “Early dark energy from a higher-dimensional gauge theory,” Phys. Rev. D
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F. Niedermann and M. S. Sloth, “Hot new early dark energy,” Phys. Rev. D
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V. I. Sabla and R. R. Caldwell, “Microphysics of early dark energy,” Phys. Rev. D
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L. Herold and E. G. M. Ferreira, “Resolving the Hubble tension with early dark energy,” Phys. Rev. D
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T. Rudelius, “Constraints on early dark energy from the axion weak gravity conjecture,” JCAP
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M. Maziashvili, “Inflaton-driven early dark energy,” Astropart. Phys
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