Early dark energy resolution to the Hubble tension in light of weak lensing surveys and lensing anomalies

Understand

Early Dark Energy (EDE) contributing a fraction $f_{\rm EDE}(z_c)\sim 10 \%$ of the energy density of the universe around $z_c\simeq 3500$ and diluting as or faster than radiation afterwards, can provide a resolution to the Hubble tension, the $\sim 5\sigma$ discrepancy between the $H_0$ value derived from early- and late-universe observations within $\Lambda$CDM.

• However, it has been pointed out that Large-Scale Structure (LSS) data, which are in $\sim3\sigma$ tension with $\Lambda$CDM and EDE cosmologies, might alter these conclusions.
• We reassess the viability of the EDE against a host of high- and low-redshift measurements, by combining LSS observations from recent weak lensing (WL) surveys with CMB, Baryon Acoustic Oscillation (BAO), growth function (FS) and Supernova Ia (SNIa) data.
• Introducing a model whose only parameter is $f_{\rm EDE}(z_c)$, we report a $\sim 2\sigma$ preference for non-zero $f_{\rm EDE}(z_c)$ from Planck data alone and the tension with SH0ES is reduced below $2\sigma$.