Prepared for submission to JCAP Distribution function approach to redshift space distortions. Part IV: perturbation theory applied to dark matter Zvonimir Vlah,a UroˇsSeljak,a;b;c;d Patrick McDonald,c;e Teppei Okumura,d and Tobias Baldaufa aInstitute for Theoretical Physics, University of Z¨urich, Winterthurerstrasse 190, Z¨urich, Switzerland bPhysics, Astronomy Department, University of California, Berkeley, California, USA. cLawrence Berkeley National Laboratory, Berkeley, CA, USA dInstitute for Early Universe, Ewha University, Seoul, S. Korea ePhysics Dept., Brookhaven National Laboratory, Upton, NY, USA E-mail:
[email protected],
[email protected] Abstract. We develop a perturbative approach to redshift space distortions (RSD) using the phase space distribution function approach and apply it to the dark matter redshift space power spectrum and its moments. RSD can be written as a sum over density weighted velocity moments correlators, with the lowest order being density, momentum density and stress energy density. We use standard and extended perturbation theory (PT) to determine their auto and cross correlators, comparing them to N-body simulations. We show which of the terms can be modeled well with the standard PT and which need additional terms that include higher order corrections which cannot be modeled in PT. Most of these additional terms are related to the small scale velocity dispersion effects, the so called finger of god (FoG) effects, which affect some, but not all, of the terms in this expansion, and which can be approximately modeled using a simple physically motivated ansatz such as the halo model. We point out that there are several velocity dispersions that enter into the detailed RSD analysis with very different amplitudes, which can be approximately predicted by the halo model.