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Early dark energy (EDE) that behaves like a cosmological constant at early times (redshifts $z\gtrsim3000$) and then dilutes away like radiation or faster at later times can solve the Hubble tension.
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Gong-Bo Zhao et al. , “Dynamical dark energy in light of the latest observations,” Nat. Astron. 1
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Jose Luis Bernal, Licia Verde, and Adam G. Riess, “The trouble with H 0 H_{0} ,” JCAP 1610
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Jarah Evslin, Anjan A Sen, and Ruchika, “Price of shifting the Hubble constant,” Phys. Rev. D97
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Tanvi Karwal, Vivian Poulin, Tristan L. Smith, and Marc Kamionkowski, “The background and perturbation dynamics necessary to resolve the Hubble tension with early dark energy,” (2019)
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