Lilian Jiang
N-body dark matter haloes with simple hierarchical histories
Jiang, Lilian; Helly, John; Cole, Shaun; Frenk, Carlos
Authors
Dr John Helly j.c.helly@durham.ac.uk
Chief Experimental Officer
Professor Shaun Cole shaun.cole@durham.ac.uk
Director of the Institute for Computational Cosmology
Professor Carlos Frenk c.s.frenk@durham.ac.uk
Professor
Abstract
We present a new algorithm which groups the subhaloes found in cosmological N-body simulations by structure finders such as SUBFIND into dark matter haloes whose formation histories are strictly hierarchical. One advantage of these `Dhaloes' over the commonly used friends-of-friends (FoF) haloes is that they retain their individual identity in the cases when FoF haloes are artificially merged by tenuous bridges of particles or by an overlap of their outer diffuse haloes. Dhaloes are thus well suited for modelling galaxy formation and their merger trees form the basis of the Durham semi-analytic galaxy formation model, GALFORM. Applying the Dhalo construction to the Λ cold dark matter Millennium II Simulation, we find that approximately 90 per cent of Dhaloes have a one-to-one, bijective match with a corresponding FoF halo. The remaining 10 per cent are typically secondary components of large FoF haloes. Although the mass functions of both types of haloes are similar, the mass of Dhaloes correlates much more tightly with the virial mass, M200, than FoF haloes. Approximately 80 per cent of FoF and bijective and non-bijective Dhaloes are relaxed according to standard criteria. For these relaxed haloes, all three types have similar concentration-M200 relations and, at fixed mass, the concentration distributions are described accurately by log-normal distributions.
Citation
Jiang, L., Helly, J., Cole, S., & Frenk, C. (2014). N-body dark matter haloes with simple hierarchical histories. Monthly Notices of the Royal Astronomical Society, 440(3), 2115-2135. https://doi.org/10.1093/mnras/stu390
Journal Article Type | Article |
---|---|
Acceptance Date | Feb 24, 2014 |
Online Publication Date | Apr 4, 2014 |
Publication Date | May 21, 2014 |
Deposit Date | Apr 11, 2014 |
Publicly Available Date | Apr 14, 2014 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Royal Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 440 |
Issue | 3 |
Pages | 2115-2135 |
DOI | https://doi.org/10.1093/mnras/stu390 |
Keywords | Methods: numerical, Galaxies: haloes, Cosmology: theory, Dark matter. |
Public URL | https://durham-repository.worktribe.com/output/1435586 |
Files
Published Journal Article
(3.1 Mb)
PDF
Copyright Statement
This article has been published in the Monthly Notices of the Royal Astronomical Society. © 2014 The Authors
Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
You might also like
The FLAMINGO project: revisiting the S8 tension and the role of baryonic physics
(2023)
Journal Article
The Milky Way’s plane of satellites is consistent with ΛCDM
(2022)
Journal Article
Downloadable Citations
About Durham Research Online (DRO)
Administrator e-mail: dro.admin@durham.ac.uk
This application uses the following open-source libraries:
SheetJS Community Edition
Apache License Version 2.0 (http://www.apache.org/licenses/)
PDF.js
Apache License Version 2.0 (http://www.apache.org/licenses/)
Font Awesome
SIL OFL 1.1 (http://scripts.sil.org/OFL)
MIT License (http://opensource.org/licenses/mit-license.html)
CC BY 3.0 ( http://creativecommons.org/licenses/by/3.0/)
Powered by Worktribe © 2025
Advanced Search