The DOI matches its Crossref record; 52 of the 52 references it cites were found in a registry or an index.
The statistics of CDM halo concentrations
Open accessAbstract
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)
Overview
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Integrity signals
Registry
Cites
Statistics
Verification
Claims the paper makes
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Claims other papers make about this one
Each is checked against this paper’s own text: does it say what the citing paper says it does?
The source backs part of the claim, not all of it — or backs it for a different population, condition or comparison.
In the citing paper
“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
Experimental — accuracy not yet measuredThe source backs part of the claim, not all of it — or backs it for a different population, condition or comparison.
In the citing paper
“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)”
From The milky way total mass profile as inferred from Gaia DR2 (2020) · cites this paper as Neto et al. 2007
Experimental — accuracy not yet measuredThe cited source says what the claim attributes to it.
In the citing paper
“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
Self-check
Percentages, sums and reported differences re-computed from the paper’s own numbers.
The self-check needs the paper’s full text.
Citations
Cites
Spergel, D. N., Verde, L., Peiris, H. V., Komatsu, E., Nolta, M. R., Bennett, C. L., Halpern, M., Hinshaw, G., Jarosik, N., Kogut, A., et al. (2003) · The Astrophysical Journal Supplement Series · doi:10.1086/377226 · Cited by 10,976
A Universal Density Profile from Hierarchical Clustering
Navarro, J. F., Frenk, C. S., & White, S. D. M. (1997) · The Astrophysical Journal · doi:10.1086/304888 · Cited by 9,917
Self-citationThe Structure of Cold Dark Matter Halos
Navarro, J. F., Frenk, C. S., & White, S. D. M. (1996) · The Astrophysical Journal · doi:10.1086/177173 · Cited by 8,544
Self-citationThree‐Year Wilkinson Microwave Anisotropy Probe ( WMAP ) Observations: Implications for Cosmology
Spergel, D. N., Bean, R., Dore, O., Nolta, M. R., Bennett, C. L., Dunkley, J., Hinshaw, G., Jarosik, N., Komatsu, E., Page, L., et al. (2007) · The Astrophysical Journal Supplement Series · doi:10.1086/513700 · Cited by 6,778
The cosmological simulation code gadget-2
Springel, V. (2005) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2005.09655.x · Cited by 6,368
Self-citationA Universal Density Profile from Hierarchical ClusteringPreprint
Navarro, J. F., Frenk, C. S., & White, S. D. M. (1996) · Cited by 6,275
Self-citationSimulations of the formation, evolution and clustering of galaxies and quasars
Springel, V., White, S. D. M., Jenkins, A. R., Frenk, C. S., Yoshida, N., Gao, L., Navarro, J. F., Thacker, R. J., Croton, D., Helly, J. C., et al. (2005) · Nature · doi:10.1038/nature03597 · Cited by 5,060
Self-citationThe cosmological simulation code GADGET-2
Petkova, M., & Springel, V. (2005) · Cited by 3,918
Self-citationThe evolution of large-scale structure in a universe dominated by cold dark matter
Davis, M., Efstathiou, G., Frenk, C. S., & White, S. D. M. (1985) · The Astrophysical Journal · doi:10.1086/163168 · Cited by 3,397
Self-citationPopulating a cluster of galaxies - I. Results at \fontshape{it}{z}=0
Springel, V., White, S. D. M., Tormen, G., & Kauffmann, G. (2001) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.2001.04912.x · Cited by 2,852
Self-citation
Research works printed but not linked: 1
- 2005, AAS, 37, 1330
Cited by
Sorted by citations
The Aquarius Project: the subhaloes of galactic haloes
Springel, V., Wang, J., Vogelsberger, M., Ludlow, A. D., Jenkins, A. R., Helmi, A., Navarro, J. F., Frenk, C. S., & White, S. D. M. (2008) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2008.14066.x · Cited by 1,990
Self-citationDunkley, J., Komatsu, E., Nolta, M. R., Spergel, D. N., Larson, D., Hinshaw, G., Page, L., Bennett, C. L., Gold, B., Jarosik, N., et al. (2009) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/180/2/306 · Cited by 1,787
THE ROCKSTAR PHASE-SPACE TEMPORAL HALO FINDER AND THE VELOCITY OFFSETS OF CLUSTER CORES
Behroozi, P., Wechsler, R. H., & Wu, H. (2012) · The Astrophysical Journal · doi:10.1088/0004-637x/762/2/109 · Cited by 1,694
The Rockstar Phase-Space Temporal HALO Finder and the Velocity Offsets of Cluster Cores
Behroozi, P., Wechsler, R. H., & Wu, H. (2012) · University of North Texas Digital Library (University of North Texas) · Cited by 1,164
Cosmology and fundamental physics with the Euclid satellite
The Euclid Theory Working Group, Amendola, L., Appleby, S. A., Avgoustidis, A., Bacon, D., Baker, T., Baldi, M., Bartolo, N., Blanchard, A., Bonvin, C., et al. (2018) · Living Reviews in Relativity · doi:10.1007/s41114-017-0010-3 · Cited by 1,096
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
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
Are you an author, or do you see a problem with this page? Request a review
