The redshift space power spectrum in the halo model

Abstract

Recently there has been a lot of attention focussed on a virialized halo-based approach to understanding the properties of the matter and galaxy power spectrum. We show that this model allows a natural treatment of the large and small scale redshift space distortions, which we develop here, which extends the pedagogical value of the approach.

4 pages, 2 figures, submitted to MNRAS

References in corpus (2)

• Weak Lensing by Large-Scale Structure: A Dark Matter Halo Approach
• Halo Profiles and the Nonlinear Two- and Three-Point Correlation Functions of Cosmological Mass Density

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