{ "id": "astro-ph/0509799", "version": "v1", "published": "2005-09-27T10:27:08.000Z", "updated": "2005-09-27T10:27:08.000Z", "title": "A universal density slope - velocity anisotropy relation", "authors": [ "Steen H. Hansen", "Ben Moore", "Joachim Stadel" ], "comment": "4 pages, 1 figure, to appear in the XXIst IAP Colloquium \"Mass Profiles and Shapes of Cosmological Structures\", Paris 4-9 July 2005, France, (Eds.) G. Mamon, F. Combes, C. Deffayet, B. Fort, EAS Publications Series", "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 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. 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, central density slope of \\alpha_0 = -0.8, and outer anisotropy of approximately \\beta_\\infinity = 0.5.", "revisions": [ { "version": "v1", "updated": "2005-09-27T10:27:08.000Z" } ], "analyses": { "keywords": [ "velocity anisotropy relation", "universal density slope", "equilibrated dark matter structures", "phase-space density", "zero central velocity anisotropy" ], "tags": [ "journal article" ], "publication": { "doi": "10.1051/eas:2006042" }, "note": { "typesetting": "TeX", "pages": 4, "language": "en", "license": "arXiv", "status": "editable", "inspire": 693315, "adsabs": "2006EAS....20...33H" } } }