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
References in corpus (5)
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Cited by in corpus (15)
- Cosmic voids in modified gravity models with massive neutrinos
- The GIGANTES dataset: precision cosmology from voids in the machine learning era
- Euclid: Forecasts from redshift-space distortions and the Alcock-Paczynski test with cosmic voids
- Cosmological exploitation of the size function of cosmic voids identified in the distribution of biased tracers
- Euclid: Cosmological forecasts from the void size function
- Cosmological constraints from the BOSS DR12 void size function
- Cosmic voids: a novel probe to shed light on our Universe
- Redshift-space effects in voids and their impact on cosmological tests. Part I: the void size function
- Cluster-void degeneracy breaking: Neutrino properties and dark energy
- DEMNUni: disentangling dark energy from massive neutrinos with the void size function
- The halo bias inside cosmic voids
- A study on Cubic Galileon Gravity Using N-body Simulations
- Non-comoving baryons and cold dark matter in cosmic voids
- Unveiling the Universe with Emerging Cosmological Probes
- Cosmology with Cosmic Voids