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Phantom dark energy can produce amplified cosmic acceleration at late times, thus increasing the value of $H_0$ favored by CMB data and releasing the tension with local measurements of $H_0$.
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Michel Chevallier and David Polarski, “Accelerating universes with scaling dark matter,” Int. J. Mod. Phys. D10
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Eric V. Linder, “Exploring the expansion history of the universe,” Phys. Rev. Lett. 90
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https://github.com/GeorgeAlestas/H0_Tension_Data
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J. Zhang, “Most Frequent Value Statistics and the Hubble Constant,” Publ. Astron. Soc. Pac. 130
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Eric V. Linder, “No Slip Gravity,” JCAP 03
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