The redshift space power spectrum in the halo model
arXiv:astro-ph/0005085 · doi:10.1046/j.1365-8711.2001.03956.x
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