Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology
Scientific paper
2006-08-29
Astronomy and Astrophysics
Astrophysics
General Relativity and Quantum Cosmology
10 pages, 18 figures, Accepted for publication in A&A
Scientific paper
10.1051/0004-6361:20064965
In this paper, we confront the predictions of the power law cardassian model for the baryon power spectrum with the observations of the SDSS galaxy survey. We show that they fit only for very unusual values of the cold dark matter or baryon density parameters, the Hubble parameter or the spectral index of the initial power spectrum. Moreover, the best-fit Cardassian models turn out to be phantom models. If one wants to recover the usual values for these constants, as quoted by the WMAP team, the power law Cardassian model turns out to be indistinguishable from a LCDM model.
Amarzguioui Morad
Fay Stephane
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