{ "id": "astro-ph/0510656", "version": "v1", "published": "2005-10-21T20:44:02.000Z", "updated": "2005-10-21T20:44:02.000Z", "title": "The velocity anisotropy - density slope relation", "authors": [ "Steen H. Hansen", "Joachim Stadel" ], "comment": "15 pages, 7 figures", "journal": "JCAP 0605:014,2006", "doi": "10.1088/1475-7516/2006/05/014", "categories": [ "astro-ph" ], "abstract": "One can solve the Jeans equation analytically for equilibrated dark matter structures, once given two pieces of input from numerical simulations. These inputs are 1) a connection between phase-space density and radius, and 2) a connection between velocity anisotropy and density slope, the \\alpha-\\beta relation. The first (phase-space density v.s. radius) has already been analysed through several different simulations, however the second (\\alpha-\\beta relation) has not been quantified yet. We perform a large set of numerical experiments in order to quantify the slope and zero-point of the \\alpha-\\beta relation. We find strong indication that the relation is indeed an attractor. When combined with the assumption of phase-space being a power-law in radius, this allows us to conclude that equilibrated dark matter structures indeed have zero central velocity anisotropy \\beta_0 = 0, central density slope of \\alpha_0 = -0.8, and outer anisotropy of \\beta_\\infty = 0.5.", "revisions": [ { "version": "v1", "updated": "2005-10-21T20:44:02.000Z" } ], "analyses": { "keywords": [ "density slope relation", "equilibrated dark matter structures", "phase-space density", "zero central velocity anisotropy", "central density slope" ], "tags": [ "journal article" ], "publication": { "publisher": "IOP", "journal": "J. Cosmol. Astropart. Phys." }, "note": { "typesetting": "TeX", "pages": 15, "language": "en", "license": "arXiv", "status": "editable", "inspire": 695906 } } }