Kyrylo Bondarenko
From dwarf galaxies to galaxy clusters: Self-Interacting Dark Matter over 7 orders of magnitude in halo mass
Bondarenko, Kyrylo; Sokolenko, Anastasia; Boyarsky, Alexey; Robertson, Andrew; Harvey, David; Revaz, Yves
Authors
Anastasia Sokolenko
Alexey Boyarsky
Dr Andrew Robertson andrew.robertson@durham.ac.uk
Academic Visitor
David Harvey
Yves Revaz
Abstract
In this paper we study the density profiles of self-interacting dark matter (SIDM) haloes spanning the full observable mass range, from dwarf galaxies to galaxy clusters. Using realistic simulations that model the baryonic physics relevant for galaxy formation, we compare the density profiles of haloes simulated with either SIDM or cold and collisionless dark matter (CDM) to those inferred from observations of stellar velocity dispersion, gas rotation curves, weak and strong gravitational lensing, and/or X-ray maps. We make our comparison in terms of the maximal surface density of haloes, circumventing the need for semi-analytic or parametric models for dark matter density profiles. We find that the maximal surface density as a function of halo mass is well reproduced by CDM simulations that include baryons, while for SIDM with a velocity-independent cross-section of 1 cm2/g, the simulated galaxy clusters have mean maximal surface densities that are below those of observed systems by an amount greater than the standard deviation of the observed maximal surface density at fixed mass. For less massive systems both CDM and SIDM agree with the observation equally well.
Citation
Bondarenko, K., Sokolenko, A., Boyarsky, A., Robertson, A., Harvey, D., & Revaz, Y. (2021). From dwarf galaxies to galaxy clusters: Self-Interacting Dark Matter over 7 orders of magnitude in halo mass. Journal of Cosmology and Astroparticle Physics, 2021(01), Article 043. https://doi.org/10.1088/1475-7516/2021/01/043
Journal Article Type | Article |
---|---|
Acceptance Date | Dec 1, 2020 |
Online Publication Date | Jan 21, 2021 |
Publication Date | 2021-01 |
Deposit Date | Sep 9, 2021 |
Publicly Available Date | Jan 21, 2022 |
Journal | Journal of Cosmology and Astroparticle Physics |
Electronic ISSN | 1475-7516 |
Publisher | IOP Publishing |
Peer Reviewed | Peer Reviewed |
Volume | 2021 |
Issue | 01 |
Article Number | 043 |
DOI | https://doi.org/10.1088/1475-7516/2021/01/043 |
Public URL | https://durham-repository.worktribe.com/output/1251225 |
Files
Accepted Journal Article
(11.2 Mb)
PDF
Copyright Statement
This is the Accepted Manuscript version of an article accepted for publication in Journal of Cosmology and Astroparticle Physics. IOP Publishing Ltd is not responsible for any errors or omissions in this version of the manuscript or any version derived from it. The Version of Record is available online at https://doi.org/10.1088/1475-7516/2021/01/043
You might also like
Scanning for dark matter subhaloes in Hubble Space Telescope imaging of 54 strong lenses
(2023)
Journal Article
Data Downloaded via Parachute from a NASA Super-Pressure Balloon
(2023)
Journal Article
PyAutoGalaxy: Open-Source Multiwavelength Galaxy Structure & Morphology
(2023)
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 © 2024
Advanced Search