Origin and Modelling of Cold Dark Matter Halo Properties: IV. Triaxial Ellipticity

TL;DR

This paper discusses the theoretical modeling of the triaxial shapes of cold dark matter haloes, focusing on their ellipticity properties, although the current version has been withdrawn and replaced by a different arXiv submission.

Contribution

The paper provides a theoretical framework for understanding the triaxial ellipticity of dark matter haloes, advancing the modeling of their shapes.

Findings

Theoretical model of halo ellipticity

Insights into halo shape distribution

Comparison with previous shape models

Abstract

This paper has been withdrawn owing a re-arrangement of two previously submitted papers. The new version of the theoretical work on the triaxial shape of dark matter haloes can be found at the ArXiv astro-ph list (CO) as article 1104.2905