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Light propagation in Swiss cheese models of random close-packed Szekeres structures: Effects of anisotropy and comparisons with perturbative results

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arxiv 1703.03572 v2 pith:7NCSSK4A submitted 2017-03-10 astro-ph.CO

classification astro-ph.CO
keywords modelslightresultssmallszekerescheesepropagationswiss
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abstract

Light propagation in two Swiss cheese models based on anisotropic Szekeres structures is studied and compared with light propagation in Swiss cheese models based on the Szekeres models' underlying LTB models. The study shows that the anisotropy of the Szekeres models has only a small effect on quantities such as redshift-distance relations, projected shear and expansion rate along individual light rays. \newline\indent The average angular diameter distance to the last scattering surface is computed for each model. Contrary to earlier studies, the results obtained here are (mostly) in agreement with perturbative results. In particular, a small negative shift, $\delta D_A:=\frac{D_A-D_{A,bg}}{D_{A,bg}}$, in the angular diameter distance is obtained upon line-of-sight averaging in three of the four models. The results are, however, not statistically significant. In the fourth model, there is a small positive shift which has an especially small statistical significance. The line-of-sight averaged inverse magnification at $z = 1100$ is consistent with $1$ to a high level of confidence for all models, indicating that the area of the surface corresponding to $z = 1100$ is close to that of the background.

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. OpenAlex reports about 33 citations worldwide. Full citation record

  1. Light path averages in spacetimes with non-vanishing average spatial curvature

    astro-ph.CO 2019-09 conditional novelty 6.0 of 10

    Light-path averaged observables in Swiss cheese cosmologies show nearly the same mean and scatter in curved and flat FLRW backgrounds, indicating curvature does not significantly alter the relationship between line-of...

  2. Physical geometry of the quasispherical Szekeres models

    gr-qc 2019-08 conditional novelty 6.0 of 10

    The dipole functions in quasispherical Szekeres models shift shells relative to each other and rotate their local frames by exact amounts, and the paper shows how these effects explain the models' geometry.

  3. Impact of inhomogeneous curvature on growth rate measurements from magnitude fluctuations

    astro-ph.CO 2026-06 unverdicted novelty 5.0 of 10

    Full-GR simulations find that inhomogeneous curvature produces only sub-dominant systematic offsets in growth-rate measurements from magnitude fluctuations at z ≲ 0.2 relative to current statistical errors.

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