Volume 459, Number 2, November IV 2006
|Page(s)||375 - 389|
|Section||Cosmology (including clusters of galaxies)|
|Published online||12 September 2006|
Power spectrum of the SDSS luminous red galaxies: constraints on cosmological parameters
Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, 86740 Garching bei München, Germany e-mail: firstname.lastname@example.org
2 Tartu Observatory, Tõravere 61602, Estonia
Accepted: 21 August 2006
In this paper we determine the constraints on cosmological parameters using the CMB data from the Wmap experiment together with the recent power spectrum measurement of the SDSS Luminous Red Galaxies (LRGs). Specifically, we focus on spatially flat, low matter density models with adiabatic Gaussian initial conditions. The spatial flatness is achieved with an additional quintessence component whose equation of state parameter is taken to be independent of redshift. Throughout most of the paper we do not allow any massive neutrino contribution and also the influence of the gravitational waves on the CMB is taken to be negligible. The analysis is carried out separately for two cases: (i) using the acoustic scale measurements as presented in Hütsi (2006, A&A, 449, 891), (ii) using the full SDSS LRG power spectrum and its covariance matrix. We are able to obtain a very tight constraint on the Hubble constant: km s-1 Mpc-1, which helps in breaking several degeneracies between the parameters and allows us to determine the low redshift expansion law with much higher accuracy than available from the Wmap + HST data alone. The positive deceleration parameter q0 is found to be ruled out at confidence level. Finally, we extend our analysis by investigating the effects of relaxing the assumption of spatial flatness and also allow for a contribution from massive neutrinos.
Key words: cosmology: cosmological parameters / large-scale structure of Universe / cosmic microwave background
© ESO, 2006
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