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Large-scale homogeneity vs. small- scale inhomogeneity: testing ...

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In<strong>homogeneity</strong>: alternative to Dark<br />

• Is ‘perturbed FRW’ a valid description?<br />

• <strong>Large</strong> inhomogeneities → breakdown of FRW<br />

01/18/2013<br />

− Light paths distorted: distances inferred from redshifts are<br />

wrong (e.g. Wiltshire 2010)<br />

− “Averaging problem” and<br />

backreaction: different-density<br />

regions evolve differently, can have<br />

global accelerated expansion<br />

without Dark Energy<br />

(e.g. Buchert 2007, Li & Schwarz<br />

2009, Räsänen 2011)<br />

− Void models, e.g. Lemaître-<br />

Tolman-Bondi model<br />

Energy?<br />

Image: hubblesite.org<br />

Morag I. Scrimgeour 5

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