Average luminosity distance in inhomogeneous universes
Valentin Kostov

TL;DR
This paper investigates how inhomogeneities modeled as voids affect the average luminosity distance in the universe, finding that such effects are largely canceled out by averaging over all directions, thus unlikely to mimic dark energy.
Contribution
It provides a non-perturbative analysis of inhomogeneity effects on luminosity distance averaging, demonstrating significant cancellations and setting bounds on their impact.
Findings
Average correction is about 20% of maximal velocity correction.
Cancellations between void fronts and backs reduce the net effect.
Voids cannot mimic dark energy unless much larger or faster.
Abstract
The paper studies the correction to the distance modulus induced by inhomogeneities and averaged over all directions from a given observer. The inhomogeneities are modeled as mass-compensated voids in random or regular lattices within Swiss-cheese universes. Void radii below 300 Mpc are considered, which are supported by current redshift surveys and limited by the recently observed imprint such voids leave on CMB. The averaging over all directions, performed by numerical ray tracing, is non-perturbative and includes the supernovas inside the voids. Voids aligning along a certain direction produce a cumulative gravitational lensing correction that increases with their number. Such corrections are destroyed by the averaging over all directions, even in non-randomized simple cubic void lattices. At low redshifts, the average correction is not zero but decays with the peculiar velocities…
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