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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

From dwarf galaxies to galaxy clusters: Self-Interacting Dark Matter over 7 orders of magnitude in halo mass Thumbnail


Authors

Kyrylo Bondarenko

Anastasia Sokolenko

Alexey Boyarsky

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

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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





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