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The statistics of CDM halo concentrations
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We use the Millennium Simulation (MS) to study the statistics of LCDM halo concentrations at z = 0. Our results confirm that the average halo concentration declines monotonically with mass; a power-law fits well the concentration-mass relation for over 3 decades in mass, up to the most massive objects to form in a LCDM universe (~ 10^15 h^-1 Msol). This is in clear disagreement with the predictions of the model proposed by Bullock et al. for these rare objects, and agrees better with the original predictions of Navarro, Frenk, & White. The large volume surveyed, together with the unprecedented numerical resolution of the MS, allow us to estimate with confidence the distribution of concentrations and, consequently, the abundance of systems with unusual properties. About one in a hundred cluster haloes (M200 >~ 3x10^14 h^-1 Msol) have concentrations exceeding c200 = 7.5, a result that may be used to interpret the likelihood of unusually strong massive gravitational lenses, such as Abell 1689, in the LCDM cosmogony. A similar fraction (1 in 100) of galaxy-sized haloes (M200 ~ 10^12 h^-1 Msol) have c200 < 4.5, an important constraint on models that attempt to reconcile the rotation curves of low surface-brightness galaxies by appealing to haloes of unexpectedly low concentration. We find that halo concentrations are independent of spin once haloes manifestly out of equilibrium are removed from the sample. Compared to their relaxed brethren, the concentrations of out-of-equilibrium haloes tend to be lower and to have more scatter, while their spins tend to be higher... (continue)
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“As argued in previous studies (e.g. Neto et al. 2007; Schaller et al. 2015), we limit the fits to the radial range [0 . 05 , 1] R 200 .”
From The milky way total mass profile as inferred from Gaia DR2 (2020) · cites this paper as Neto et al. 2007
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“The ML value for the concentration is, in fact, equal to the median concentration of ∼ 1 × 10 12 M ⊙ haloes (e.g. Neto et al. 2007; Hellwing et al. 2016)”
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“Some haloes are not in equilibrium, typically because of transient events such as mergers (e.g. see Neto et al. 2007); including such haloes would misrepresent the longterm relation between the DM distributions in the DMO and hydrodynamics simulations so we do not consider them further.”
From The milky way total mass profile as inferred from Gaia DR2 (2020) · cites this paper as Neto et al. 2007
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Metadata
- Authors
- Neto, A. F., Gao, L., Bett, P., Cole, S., Navarro, J. F., Frenk, C. S., White, S. D. M., Springel, V., & Jenkins, A.
- Affiliations
- Universidade Federal do Rio Grande do Sul (BR)
- Durham University (GB)
- Max Planck Society (DE)
- Venue
- Monthly Notices of the Royal Astronomical Society
- Publisher
- Oxford University Press (OUP)
- Published
- 2007-11-11
- Volume
- 381
- Issue
- 4
- Pages
- 1450-1462
- ISSN
- 0035-8711 (ISSN-L)
- 1365-2966
- OpenAlex
- W1968752888
- Cited by
- 764
- References
- 52
- Citations by year
- 2026: 5 · 2025: 17 · 2024: 20 · 2023: 23 · 2022: 34 · 2021: 38 · 2020: 41 · 2019: 32 · 2018: 37 · 2017: 38 · 2016: 55 · 2015: 58 · 2014: 43 · 2013: 57 · 2012: 68
- FWCI
- 30.70
- Type
- journal article
- Language
- en
- Open access
- green
- arxiv.org
- Locations
- Monthly Notices of the Royal Astronomical Society (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- Durham Research Online (Durham University) (submittedVersion)
- Max Planck Institute for Plasma Physics (submittedVersion)
- Max Planck Digital Library (submittedVersion)
- Durham Research Online (Durham University) (submittedVersion, cc-by)
- MPG.PuRe (Max Planck Society) (submittedVersion)
- arXiv (Cornell University)
- 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 › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Keywords
- dark matter halo concentration, concentration-mass relation, Millennium Simulation, LCDM cosmology, galaxy halos, gravitational lensing, Abell 1689, low surface brightness galaxies, halo spin
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