Cited by 294Galaxies: Formation, Evolution, PhenomenaCosmology and Gravitation TheoriesDark Matter and Cosmic Phenomena

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A mass-dependent density profile for dark matter haloes including the influence of galaxy formation

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Cintio, Arianna Di, Brook, Chris B., Dutton, Aaron A., Macciò, Andrea V., Stinson, Greg S., Knebe, Alexander·2014·Monthly Notices of the Royal Astronomical Society

DOI 10.1093/mnras/stu729

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Abstract

We introduce a mass-dependent density profile to describe the distribution of dark matter within galaxies, which takes into account the stellar-to-halo mass dependence of the response of dark matter to baryonic processes. The study is based on the analysis of hydrodynamically simulated galaxies from dwarf to Milky Way mass, drawn from the Making Galaxies In a Cosmological Context project, which have been shown to match a wide range of disc scaling relationships. We find that the best-fitting parameters of a generic double power-law density profile vary in a systematic manner that depends on the stellar-to-halo mass ratio of each galaxy. Thus, the quantity M⋆/Mhalo constrains the inner (γ) and outer (β) slopes of dark matter density, and the sharpness of transition between the slopes (α), reducing the number of free parameters of the model to two. Due to the tight relation between stellar mass and halo mass, either of these quantities is sufficient to describe the dark matter halo profile including the effects of baryons. The concentration of the haloes in the hydrodynamical simulations is consistent with N-body expectations up to Milky Way-mass galaxies, at which mass the haloes become twice as concentrated as compared with pure dark matter runs. This mass-dependent density profile can be directly applied to rotation curve data of observed galaxies and to semi-analytic galaxy formation models as a significant improvement over the commonly used NFW profile.

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Authors: Cintio, A. D., Brook, C. B., Dutton, A. A., Macciò, A. V., Stinson, G. S., & Knebe, A.
Affiliations: Universidad Autónoma de Madrid (ES)
Max Planck Institute for Astronomy (DE)
Corresponding author: Cintio, Arianna Di
ORCID: Cintio, Arianna Di
Brook, Chris B.
Dutton, Aaron A.
Macciò, Andrea V.
Knebe, Alexander
Venue: Monthly Notices of the Royal Astronomical Society
Publisher: Oxford University Press (OUP)
Published: 2014-05-24
Volume: 441
Issue: 4
Pages: 2986-2995
ISSN: 0035-8711 (ISSN-L)
1365-2966
DOI: 10.1093/mnras/stu729
OpenAlex: W2125094672
Cited by: 294
References: 91
Citations by year: 2026: 20 · 2025: 23 · 2024: 21 · 2023: 17 · 2022: 29 · 2021: 26 · 2020: 26 · 2019: 27 · 2018: 31 · 2017: 21 · 2016: 27 · 2015: 21 · 2014: 5
FWCI: 13.30
Type: journal article
Language: en
Open access: bronze
doi.org
Locations: Monthly Notices of the Royal Astronomical Society (publishedVersion)
CLOK (University of Central Lancashire) (acceptedVersion)
arXiv (Cornell University) (submittedVersion)
Adelaide Research & Scholarship (AR&S) (University of Adelaide) (submittedVersion)
Max Planck Institute for Plasma Physics (submittedVersion)
arXiv (Cornell University)
Funders: University of Central Lancashire
European Commission (222919)
Deutsche Forschungsgemeinschaft (subproject A1), SFB881, CSD2009-00064)
Ministerio de Economía y Competitividad (AYA2012-31101, CSD-2009-00064, DP140100198)
Ministerio de Ciencia e Innovación (Multi-Dark CSD2009-00064, CSD2009, CSD2009-00064)
Max-Planck-Institut für Astronomie
Science and Technology Facilities Council (ST/K000373/1)
Australian Research Council (DP130100117, DP140100198)
Topics: Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Dark Matter and Cosmic Phenomena
Keywords: dark matter halos, halo density profiles, stellar-to-halo mass ratio, baryonic processes, galaxy formation, halo concentration, fluid simulation, rotation curves, Navarro-Frenk-White profile, semi-analytic galaxy formation models

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A mass-dependent density profile for dark matter haloes including the influence of galaxy formation

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