Can late dark energy transitions raise the Hubble constant?
Giampaolo Benevento, Wayne Hu, Marco Raveri
Abstract
Late times dark energy transitions at redshifts $z\ensuremath{\ll}0.1$ can raise the predicted value of the Hubble constant to the SH0ES value, $74.03\ifmmode\pm\else\textpm\fi{}1.42\text{ }(\mathrm{km}\text{ }{\mathrm{s}}^{\ensuremath{-}1}\text{ }{\mathrm{Mpc}}^{\ensuremath{-}1})$ or more, while providing an equally good fit as $\mathrm{\ensuremath{\Lambda}}\mathrm{CDM}$ at $67.73\ifmmode\pm\else\textpm\fi{}0.41$ to higher redshift data, in particular from the cosmic microwave background and baryon acoustic oscillations. These models however do not fully resolve the true source of tension between the distance ladder and high redshift observations: the local calibration of supernovae luminosities well out into the Hubble flow. When tested in this manner by transferring the SH0ES calibration to the Pantheon supernovae dataset, the ability of such transitions to raise the Hubble constant is reduced to $69.17\ifmmode\pm\else\textpm\fi{}1.09$. Such an analysis should also be used when testing any dynamical dark energy model which can produce similarly fine features in redshift or local void models.