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2018

Prospects for resolving the Hubble constant tension with standard sirens

Feeney, Stephen M., Peiris, Hiranya V., Williamson, Andrew R. et al.

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The Hubble constant ($H_0$) estimated from the local Cepheid-supernova (SN) distance ladder is in 3-$\sigma$ tension with the value extrapolated from cosmic microwave background (CMB) data assuming the standard cosmological model.

Whether this tension represents new physics or systematic effects is the subject of intense debate.
Here, we investigate how new, independent $H_0$ estimates can arbitrate this tension, assessing whether the measurements are consistent with being derived from the same model using the posterior predictive distribution (PPD).
We show that, with existing data, the inverse distance ladder formed from BOSS baryon acoustic oscillation measurements and the Pantheon SN sample yields an $H_0$ posterior near-identical to the Planck CMB measurement.

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