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2022

A tale of two (or more) $h$'s

Brieden, Samuel, Gil-Marín, Héctor, Verde, Licia

Understand

We use the large-scale structure galaxy data (LSS) from the BOSS and eBOSS surveys, in combination with abundances information from Big Bang Nucleosynthesis (BBN) to measure two values of the Hubble expansion rate, $H_0=100h\,[{\rm km}\, {\rm s}^{-1}\,{\rm Mpc}^{-1}]$, each of them based on very different physical processes.

One is a (traditional) late-time-background measurement based on determining the BAO scale and using BBN abundances on baryons for calibrating its absolute size (BAO+BBN).
This method anchors $H_0$ to the (standard) physics of the sound horizon scale at pre-recombination times.
The other is a newer early-time based measurement associated with the broadband shape of the power spectrum.