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- W3124295108 abstract "The ΛCDM cosmological model assumes the existence of a small cosmological constant in order to explain the observed accelerating cosmic expansion. Despite the dramatic improvement of the quality of cosmological data during the last decade it remains the simplest model that fits remarkably well (almost) all cosmological observations. In this talk I review the increasingly successful fits provided by ΛCDM on recent geometric probe data of the cosmic expansion. I also briefly discuss some emerging shortcomings of the model in attempting to fit specific classes of data (eg cosmic velocity dipole flows and cluster halo profiles). Finally, I summarize recent results on the theoretically predicted matter overdensity evolution (a dynamical probe of the cosmic expansion), emphasizing its scale and gauge dependence on large cosmological scales in the context of general relativity. A new scale dependent parametrization which describes accurately the growth rate of perturbations even on scales larger than 100h−1 Mpc is shown to be a straightforward generalization of the well known scale independent parametrization f(a) = Ωm(a)γ valid on smaller cosmological scales." @default.
- W3124295108 created "2021-02-01" @default.
- W3124295108 creator A5076121373 @default.
- W3124295108 date "2010-04-01" @default.
- W3124295108 modified "2023-10-16" @default.
- W3124295108 title "Consistency of ΛCDM with geometric and dynamical probes" @default.
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- W3124295108 doi "https://doi.org/10.1088/1742-6596/222/1/012024" @default.
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