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Dwarf galaxies in CDM and SIDM with baryons: observational probes of the nature of dark matter

Vogelsberger, Mark; Zavala, Jesus; Simpson, Christine; Jenkins, Adrian

Dwarf galaxies in CDM and SIDM with baryons: observational probes of the nature of dark matter Thumbnail


Authors

Mark Vogelsberger

Jesus Zavala

Christine Simpson



Abstract

We present the first cosmological simulations of dwarf galaxies, which include dark matter self-interactions and baryons. We study two dwarf galaxies within cold dark matter, and four different elastic self-interacting scenarios with constant and velocity-dependent cross-sections, motivated by a new force in the hidden dark matter sector. Our highest resolution simulation has a baryonic mass resolution of 1.8 × 102 M⊙ and a gravitational softening length of 34 pc at z = 0. In this first study we focus on the regime of mostly isolated dwarf galaxies with halo masses ∼ 1010 M⊙ where dark matter dynamically dominates even at sub-kpc scales. We find that while the global properties of galaxies of this scale are minimally affected by allowed self-interactions, their internal structures change significantly if the cross-section is large enough within the inner sub-kpc region. In these dark-matter-dominated systems, self-scattering ties the shape of the stellar distribution to that of the dark matter distribution. In particular, we find that the stellar core radius is closely related to the dark matter core radius generated by self-interactions. Dark matter collisions lead to dwarf galaxies with larger stellar cores and smaller stellar central densities compared to the cold dark matter case. The central metallicity within 1 kpc is also larger by up to ∼15 per cent in the former case. We conclude that the mass distribution and characteristics of the central stars in dwarf galaxies can potentially be used to probe the self-interacting nature of dark matter.

Citation

Vogelsberger, M., Zavala, J., Simpson, C., & Jenkins, A. (2014). Dwarf galaxies in CDM and SIDM with baryons: observational probes of the nature of dark matter. Monthly Notices of the Royal Astronomical Society, 444(4), 3684-3698. https://doi.org/10.1093/mnras/stu1713

Journal Article Type Article
Acceptance Date Aug 17, 2014
Online Publication Date Sep 17, 2014
Publication Date Nov 11, 2014
Deposit Date Nov 26, 2014
Publicly Available Date Mar 29, 2024
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 444
Issue 4
Pages 3684-3698
DOI https://doi.org/10.1093/mnras/stu1713
Keywords Methods: numerical, Galaxies: haloes, Dark matter.
Related Public URLs http://mnras.oxfordjournals.org/content/444/4/3684.full.pdf+html

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Copyright Statement
This article has been accepted for publication in 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.





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