Degeneracies and modelling choices in double-plane time-delay cosmography

TL;DR

This paper explores the complexities of double-plane gravitational lensing for cosmology, highlighting how line-of-sight effects influence modeling and proposing methods to mitigate degeneracies in estimating the Hubble constant.

Contribution

It generalizes the mass-sheet degeneracy to double-plane systems and offers a framework to incorporate line-of-sight uncertainties in $H_0$ measurements.

Findings

Line-of-sight contributions affect angular diameter distances in double-plane lensing.

The unfolding relation helps reduce uncertainties in the Hubble constant.

A prescription is provided to account for degeneracies while modeling double-plane lenses.

Abstract

Double-plane gravitational lensing is a rare but increasingly observed phenomenon in which the light from a distant source is lensed by two foreground objects at different redshifts. Such systems can be used to provide simultaneous constraints on the Hubble constant $H_0$ and the dark-energy equation of state, independent of and complementary to other probes. However, just as for single-plane gravitational lenses, the precision of these constraints is limited by the so-called mass-sheet degeneracy (MSD) -- a fundamental limit to the knowledge of the mass profiles of lens galaxies and the line of sight that can be obtained from imaging constraints alone. In this work, we show explicitly how contributions from the line of sight appear in double-plane systems. Because these contributions modify angular diameter distances, we argue that cosmological priors should not be used to simply fix the ``cosmological scaling factor'', a ratio of angular diameter distances which is key to the modelling of double-plane lenses. Motivated by this fact, we generalise the double-plane MSD to account for this uncertainty in the scaling factor. While this complicates the time-delay function, we show that, using the ``unfolding relation'', a geometric relation between distances which holds even in the presence of line-of-sight corrections, the uncertainty in the Hubble constant reduces to the familiar mass-sheet transformation of the first lens plane, and a line-of-sight contribution between the observer and the second lens plane. Our main message is therefore a prescription for reducing the degrees of freedom within double-plane models, while still safely accounting for the MSD in measurements of $H_0$.