paper

Cluster-Void Degeneracy Breaking: Modified Gravity in the Balance

arXiv:1612.06595 · doi:10.1103/PhysRevD.97.103504

Abstract

Combining galaxy cluster and void abundances is a novel, powerful way to constrain deviations from General Relativity and the CDM model. For a flat CDM model with growth of large-scale structure parameterized by the redshift-dependent growth index of linear matter perturbations, combining void and cluster abundances in future surveys with Euclid and the 4-metre Multi-Object Spectroscopic Telescope (4MOST) could improve the Figure of Merit for () by a factor of 20 compared to individual abundances. In an ideal case, improvement on current cosmological data is a Figure of Merit factor or more.

9 pages, 3 figures, 4 tables. Matches published version. Added redshift-dependent growth index, significantly extended discussion on void sensitivity to cosmological parameters. Basic conclusions unchanged

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