The data release six of the Atacama Cosmology Telescope (ACT DR6) and the second data release from the Dark Energy Spectroscopic Instrument (DESI DR2) recently became available. In light of these data, we update constraints on the early dark energy (EDE) resolution to the Hubble tension. While ACT DR6 does not favor EDE over the core cosmological model, $\mathrm{\Lambda }$ cold dark matter ($\mathrm{\Lambda }\mathrm{CDM}$), it allows for a significantly larger maximum contribution of EDE, $f_{\mathrm{EDE}}$, in the prerecombination era than the latest analysis of Planck NPIPE despite increased precision at small angular scales. Moreover, EDE rises the value of $H_0{r}_s$, improving consistency between cosmic microwave background and DESI DR2 data. We find a residual tension with SH0ES of $\sim 2\sigma$ for the combination of Planck at $\ell <1000+$ ACT DR6 + lensing + Pantheon-plus + DESI DR2, a significant decrease from $3.7\sigma$ for analyses that use NPIPE and SDSS baryonic acoustic oscillation data. A profile likelihood analysis reveals significant prior volume effects in Bayesian analyses which do not include SH0ES, with confidence intervals of $f_{\mathrm{EDE}}=0.09\pm 0.03$ and $H_0=71.0\pm 1.1\mathrm{km}/\mathrm{s}/\mathrm{Mpc}$. When including DESI data, the EDE model with $H_0=73\mathrm{km}/\mathrm{s}/\mathrm{Mpc}$ provides a better fit than the $\mathrm{\Lambda }\mathrm{CDM}$ model with $H_0=68.4\mathrm{km}/\mathrm{s}/\mathrm{Mpc}$. The inclusion of SH0ES data rises the preference well above $5\sigma$, with $\mathrm{\Delta }{\chi }^2=-35.4$. Our work demonstrates that after ACT DR6 and DESI DR2, EDE remains a potential resolution to the Hubble tension.

Close

PrevNext

View figure in article

• Baryon acoustic oscillations
• Cosmic microwave background
• Cosmological parameters
• Cosmology
• Dark energy