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A mass-dependent density profile for dark matter haloes including the influence of galaxy formation
Open accessAbstract
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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“In particular, these authors found that the α , β and γ parameters in Equation 13 depend only on the stellar-to-halo mass ratio, and thus leaving only two free parameters, ρ 0 and R s .”
From The milky way total mass profile as inferred from Gaia DR2 (2020) · cites this paper as Di Cintio et al. 2014
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Buckley, M. R., Charles, E., Gaskins, J., Brooks, A. M., Drlica-Wagner, A., Martin, P., & Zhao, G. (2015) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.91.102001 · Cited by 59
The frequency of dwarf galaxy multiples at low redshift in SDSS versus cosmological expectations
Besla, G., Patton, D. R., Stierwalt, S., Rodríguez-Gómez, V., Patel, E., Kallivayalil, N., Johnson, K. E., Pearson, S., Privon, G. C., & Putman, M. E. (2018) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sty2041 · Cited by 58
NIHAO XXI: the emergence of low surface brightness galaxies
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Self-citationMerluzzi, P., Busarello, G., Dopita, M. A., Haines, C. P., Steinhauser, D., Bourdin, H., & Mazzotta, P. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw1198 · Cited by 56
Dark-matter halo profiles of a general cusp/core with analytic velocity and potential
Dekel, A., Ishai, G., Dutton, A. A., & Macciò, A. V. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stx486 · Cited by 56
Self-citationBlazar-boosted dark matter at Super-Kamiokande
Granelli, A., Ullio, P., & Wang, J.-W. (2022) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2022/07/013 · Cited by 54
Dark matter contraction and stellar-mass-to-light ratio gradients in massive early-type galaxies
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Wasserman, A., van Dokkum, P., Romanowsky, A. J., Brodie, J. P., Danieli, S., Forbes, D. A., Abraham, R. G., Martin, C. D., Matuszewski, M., Villaume, A., et al. (2019) · The Astrophysical Journal · doi:10.3847/1538-4357/ab3eb9 · Cited by 53
Dark and luminous satellites of LMC-mass galaxies in the FIRE simulations
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Structure and kinematics of tidally limited satellite galaxies in LCDM
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Andromeda XXI – a dwarf galaxy in a low-density dark matter halo
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nIFTy galaxy cluster simulations – IV. Quantifying the influence of baryons on halo properties
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Self-citationProbing dark matter with star clusters: a dark matter core in the ultra-faint dwarf Eridanus II
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Bounds on long-lived dark matter mediators from neutron stars
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Forbes, D. A., Gannon, J. S., Romanowsky, A. J., Alabi, A., Brodie, J. P., Couch, W. J., & Ferré-Mateu, A. (2020) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staa3289 · Cited by 45
Gannon, J. S., Forbes, D. A., Romanowsky, A. J., Ferré-Mateu, A., Couch, W. J., Brodie, J. P., Huang, S., Janssens, S. R., & Okabe, N. (2021) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stab3297 · Cited by 45
The Faber–Jackson relation and Fundamental Plane from halo abundance matching
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Cintio, A. D., Tremmel, M., Governato, F., Pontzen, A., Zavala, J., Fry, A. B., Brooks, A. M., & Vogelsberger, M. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stx1043 · Cited by 45
Self-citationA constant characteristic volume density of dark matter haloes from SPARC rotation curve fits
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Monelli, M., & Trujillo, I. (2019) · The Astrophysical Journal Letters · doi:10.3847/2041-8213/ab2fd2 · Cited by 44
Review of Solutions to the Cusp-Core Problem of the ΛCDM Model
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Warm FIRE: simulating galaxy formation with resonant sterile neutrino dark matter
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On the stellar kinematics and mass of the Virgo ultradiffuse galaxy VCC 1287
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511 keV excess and primordial black holes
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Metadata
- 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
- 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
- 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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