Large-Distance Lens Uncertainties and Time-Delay Measurements of $H_0$

TL;DR

This paper examines how uncertainties in the mass distribution far from lens centers affect time-delay measurements of $H_0$, highlighting potential errors and ways to improve accuracy.

Contribution

It identifies the impact of large-distance lens uncertainties on $H_0$ estimates and suggests methods like weak lensing and simulations to mitigate these errors.

Findings

Large-distance lens uncertainties can cause about 1% error in $H_0$.

Accounting for these uncertainties increases the tension between local and CMB $H_0$ measurements.

Weak lensing and simulations can help reduce these uncertainties.

Abstract

Given the tension between the values of the Hubble parameter $H_0$ inferred from the cosmic microwave background (CMB) and from supernovae, attention is turning to time delays of strongly lensed quasars. Current time-delay measurements indicate a value of $H_0$ closer to that from supernovae, with errors on the order of a few percent, and future measurements aim to bring the errors down to the subpercent level. Here we consider the uncertainties in the mass distribution in the outskirts of the lens. We show that these can lead to errors in the inferred $H_0$ on the order of a percent and, once accounted for, would correct $H_0$ upward (thus increasing slightly the tension with the CMB). Weak gravitational lensing and simulations may help to reduce these uncertainties.