Nonspherical similarity solutions for dark halo formation
Mark Vogelsberger (1), Roya Mohayaee (2), Simon D.M. White (3) ((1), Harvard/CfA, (2) IAP Paris, (3) MPA)

TL;DR
This paper uses 3D simulations to study dark matter halo formation from self-similar initial conditions, revealing non-spherical, non-universal structures that still exhibit some universal properties like the pseudo phase-space density profile.
Contribution
It demonstrates that dark matter haloes formed from self-similar initial conditions are triaxial with non-universal density profiles, yet share universal features in phase-space density.
Findings
Halos are triaxial with axis ratios around 3:1.
Density profiles follow a power-law and depend on initial conditions.
Pseudo phase-space density follows a nearly universal power law.
Abstract
We carry out fully 3-dimensional simulations of evolution from self-similar, spherically symmetric linear perturbations of a Cold Dark Matter dominated Einstein-de Sitter universe. As a result of the radial orbit instability, the haloes which grow from such initial conditions are triaxial with major-to-minor axis ratios of order 3:1. They nevertheless grow approximately self-similarly in time. In all cases they have power-law density profiles and near-constant velocity anisotropy in their inner regions. Both the power-law index and the value of the velocity anisotropy depend on the similarity index of the initial conditions, the former as expected from simple scaling arguments. Halo structure is thus not "universal" but remembers the initial conditions. On larger scales the density and anisotropy profiles show two characteristic scales, corresponding to particles at first pericentre and…
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