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2014

A novel null test for the $\Lambda$CDM model with growth-rate data

Nesseris, Savvas, Sapone, Domenico

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Current and upcoming surveys will measure the cosmological parameters with an extremely high accuracy.

The primary goal of these observations is to eliminate some of the currently viable cosmological models created to explain the late time accelerated expansion (either real or only inferred).
However, most of the statistical tests used in cosmology have a strong requirement: the use of a model to fit the data.
Recently there has been an increased interest on finding tests that are model independent, i.e.

A novel null test for the $\Lambda$CDM model with growth-rate data · Around

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