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- W2840137645 abstract "Future large-scale spectroscopic astronomical surveys, e.g., Euclid, will enable the compilation of vast new catalogs of clusters and voids in the galaxy distribution. By combining the constraining power of both cluster and void number counts, such surveys could place stringent simultaneous limits on the sum of neutrino masses ${M}_{ensuremath{nu}}$ and the dark energy equation of state $w(z)={w}_{0}+{w}_{a}z/(1+z)$. For minimal normal-hierarchy neutrino masses, we forecast that Euclid clusters+voids ideally could reach uncertainties $ensuremath{sigma}({M}_{ensuremath{nu}})ensuremath{lesssim}15text{ }text{ }mathrm{meV}$, $ensuremath{sigma}({w}_{0})ensuremath{lesssim}0.02$, $ensuremath{sigma}({w}_{a})ensuremath{lesssim}0.07$, independent of other data. Such precision is competitive with expectations for, e.g., galaxy clustering and weak lensing in future cosmological surveys and could reject an inverted neutrino mass hierarchy at $ensuremath{gtrsim}99%$ confidence." @default.
- W2840137645 created "2018-07-19" @default.
- W2840137645 creator A5049029223 @default.
- W2840137645 date "2019-03-22" @default.
- W2840137645 modified "2023-10-06" @default.
- W2840137645 title "Cluster-void degeneracy breaking: Neutrino properties and dark energy" @default.
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- W2840137645 doi "https://doi.org/10.1103/physrevd.99.063525" @default.
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