ar X iv : a st ro - p h / 97 06 03 4 v 1 4 J un 1 99 7 Cosmological redshift distortion : deceleration , bias and density parameters from future redshift surveys of galaxies

The observed two-point correlation functions of galaxies in redshift space become anisotropic due to the geometry of the universe as well as due to the presence of the peculiar velocity field. Expanding the induced anisotropies of the correlation functions with respect to the redshift z, we obtain explicit expressions for the deceleration parameter q0, the density parameter Ω0 and the derivative of the bias parameter db/dz at z = 0 in terms of the observable statistical quantities. The present method does not require any assumption of the shape and amplitude of the underlying fluctuation spectrum, and thus can be applied to future redshift surveys of galaxies including the Sloan Digital Sky Survey. We also evaluate quantitatively the systematic error in estimating the value of β0 ≡ Ω 0.6 0 /b from galaxy redshift survey on the basis of a conventional estimator for β0, which neglects both the geometrical distortion effect and the time evolution of the parameter β(z). If the magnitude limit of the survey is as faint as 18.5 (in B-band) as in the case of the Sloan Digital Sky Survey, the systematic error ranges between −20% and 10% depending on the cosmological parameters. Although such systematic errors are smaller than the statistical errors in the current surveys, they will definitely dominate the expected statistical error for future surveys. Subject headings: cosmology: theory — large-scale-structure of the universe — methods: statistical UTAP: University of Tokyo, Theoretical Astrophysics RESCEU: Research Center for the Early Universe UTAP-262/97 RESCEU-21/97