Light-cone averages in a swiss-cheese universe
Valerio Marra, Edward W. Kolb, Sabino Matarrese

TL;DR
This paper investigates how inhomogeneities in a swiss-cheese universe affect light-cone averages and the apparent dark energy behavior, finding that voids influence the effective equation of state.
Contribution
It introduces a toy swiss-cheese cosmological model analyzing light-cone averages and shows how inhomogeneities can mimic dark energy effects.
Findings
The expansion scalar is unaffected by inhomogeneities due to spherical symmetry.
The density average along light-cones is influenced by voids and high-density structures.
The effective equation of state depends linearly on the size of inhomogeneities.
Abstract
We analyze a toy swiss-cheese cosmological model to study the averaging problem. In our model, the cheese is the EdS model and the holes are constructed from a LTB solution. We study the propagation of photons in the swiss-cheese model, and find a phenomenological homogeneous model to describe observables. Following a fitting procedure based on light-cone averages, we find that the the expansion scalar is unaffected by the inhomogeneities. This is because of spherical symmetry. However, the light-cone average of the density as a function of redshift is affected by inhomogeneities. The effect arises because, as the universe evolves, a photon spends more and more time in the (large) voids than in the (thin) high-density structures. The phenomenological homogeneous model describing the light-cone average of the density is similar to the concordance model. Although the sole source in the…
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