Weak lensing and the Dyer-Roeder approximation

TL;DR

This paper links the weak lensing approximation with the Dyer-Roeder relation, showing how density fluctuations affect cosmological distance measurements and proposing a modified relation for improved accuracy.

Contribution

It establishes a connection between weak lensing and Dyer-Roeder approximations and introduces a modified relation accounting for line-of-sight density fluctuations.

Findings

Distance correction is negligible if density fluctuations vanish after averaging.

A vanishing 3D average does not imply zero line-of-sight fluctuations.

Correction at z ~ 2 is of order a few percent.

Abstract

The distance-redshift relation plays an important role in cosmology. In the standard approach to cosmology it is assumed that this relation is the same as in the homogeneous universe. As the real universe is not homogeneous there are several methods to calculate the correction. The weak lensing approximation and the Dyer-Roeder relation are one of them. This paper establishes a link between these two approximations. It is shown that if the universe is homogeneous with only small, vanishing after averaging, density fluctuations along the line of sight, then the distance correction is negligible. It is also shown that a vanishing 3D average of density fluctuations does not imply that the mean of density fluctuations along the line of sight is zero. In this case, even within the linear approximation, the distance correction is not negligible. The modified version of the Dyer-Roeder relation is presented and it is shown that this modified relation is consistent with the correction obtained within the weak lensing approximation. The correction to the distance for a source at z ~ 2 is of order of a few percent. Thus, with an increasing precision of cosmological observations an accurate estimation of the distance is essential. Otherwise errors due to miscalculation the distance can become a major source of systematics.