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I explicitly show that the increase in $ω_c$ needed for EDE to preserve the fit to the CMB, which has been argued to worsen the fit to weak lensing and galaxy clustering measurements, is specifically required to lower the amplitude of the eISW effect, which would otherwise exceed $Λ$CDM's prediction by $\approx 20\%$: this is a generic problem beyond EDE and likely applying to most models enhancing the expansion rate around recombination.

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ClaimStatusCheckableCredenceUseStakesRests on
I explicitly show that the increase in $ω_c$ needed for EDE to preserve the fit to the CMB, which has been argued to wo…○ uncheckedyes0.5507.6—

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