2009

Hubble Diagram Dispersion From Large-Scale Structure

Clifton, Timothy, Zuntz, Joe

Understand

We consider the effects of large structures in the Universe on the Hubble diagram.

This problem is treated non-linearly by considering a Swiss Cheese model of the Universe in which under-dense voids are represented as negatively curved regions of space-time.
Exact expressions for luminosity distances and redshifts are used to investigate the non-linear effects of structure on the magnitudes of astrophysical sources.
It is found that the intervening voids we consider, between the observer and source, produce changes in apparent magnitude of less than 0.012.

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