Talk detail

MG13 - Talk detail

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 Participant

Hahn, Oliver

Institution

Stanford University / SLAC  - 2575 Sand Hill Rd - Menlo Park - CA - USA

Session

OC4

Accepted

Yes

Order

9

Time

17:55 - 18:15

Talk

Oral abstract

Title

Tracing, Analyzing and Visualizing Dark Matter in Phase Space
Co-authors Tom Abel, Ralf Kaehler

Abstract

In a Universe dominated by cold dark matter, structure forms from foldings of a three-dimensional sheet permeating six-dimensional phase space. The dynamics of the sheet is governed by gravity alone, and it never tears or intersects itself in phase space. In position space, these foldings lead to the formation pancakes, filaments and finally dark matter halos: the cosmic web. N-body simulations already follow the motion of this sheet in phase space. This fact can be used to extract full fine-grained phase-space-structure information from existing cosmological N-body simulations. Particles are considered as the vertices of an unstructured three dimensional mesh, moving in six dimensional phase-space. On this mesh, mass density and momentum are uniquely defined. We show how to obtain the space density of the fluid, local velocity dispersion and detect caustics. We also discuss how information about the sheet can be used to create highly accurate volume visualizations of the dark matter distribution in simulations.

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