Abstract
We use the Om statistic and the genetic algorithms (GAs) in order to derive a null test on the spatially flat cosmological constant model Lambda cold dark matter (ΛCDM). This is done in two steps: first, we apply the GAs to the Constitution SNIa data in order to acquire a model-independent reconstruction of the expansion history of the Universe H(z) and secondly, we use the reconstructed H(z) in conjunction with the Om statistic, which is constant only for the ΛCDM model, to derive our constraints. We find that while ΛCDM is consistent with the data at the 2σ level, some deviations from ΛCDM model at low redshifts can be accommodated.
Original language | English |
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Journal | Monthly Notices of the Royal Astronomical Society |
Volume | 408 |
Issue number | 3 |
Pages (from-to) | 1879-1885 |
Number of pages | 6 |
ISSN | 0035-8711 |
DOIs | |
Publication status | Published - 1 Nov 2010 |