The DOI matches its Crossref record; 20 of the 20 references it cites were found in a registry or an index.
The Density Profiles of the Dark Matter Halo Are Not Universal
Open accessAbstract
We perform a series of high-resolution N-body simulations designed to examine the density profiles of dark matter halos. From 12 simulated halos ranging in mass from 2x1012 to 5x1014 h-1 M middle dot in circle (represented by approximately 1 million particles within the virial radius), we find a clear systematic correlation between the halo mass and the slope of the density profile at 1% of the virial radius, in addition to the variations of the slope among halos of similar mass. More specifically, the slope is approximately -1.5, -1.3, and -1.1 for galaxy-, group-, and cluster-mass halos, respectively. While we confirm the earlier simulation results that the inner slope is steeper than the universal profile originally proposed by Navarro, Frenk, & White, this mass dependence is inconsistent with several analytical arguments attempting to link the inner slope with the primordial index of the fluctuation spectrum. Thus, we conclude that the dark matter density profiles, especially in the inner region, are not universal.
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.
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
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
The 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
A Universal Density Profile from Hierarchical ClusteringPreprint
Navarro, J. F., Frenk, C. S., & White, S. D. M. (1996) · Cited by 6,275
The Large-Scale Structure of the Universe
(2007) · Astronomy and Astrophysics Library · doi:10.1007/978-3-540-73478-9_2 · Cited by 3,219
The Large-Scale Structure of the Universe
Peebles, P. J. E. (1981) · Princeton University Press eBooks · doi:10.1515/9780691206714 · Cited by 2,851
Resolving the Structure of Cold Dark Matter Halos
Moore, B., Governato, F., Quinn, T., Stadel, J., & Lake, G. (1998) · The Astrophysical Journal · doi:10.1086/311333 · Cited by 898
Non-linear evolution of cosmological power spectra
Peacock, J. A., & Dodds, S. J. (1996) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/280.3.l19 · Cited by 783
Hamilton, A. J. S., Matthews, A., Kumar, P., & Lu, E. (1991) · The Astrophysical Journal · doi:10.1086/186057 · Cited by 354
Hydra: an Adaptive-Mesh Implementation of P 3M-SPH
Couchman, H. M. P., Thomas, P. A., & Pearce, F. R. (1995) · The Astrophysical Journal · doi:10.1086/176348 · Cited by 280
On the Origin of Cusps in Dark Matter Halos
Fukushige, T., & Makino, J. (1997) · The Astrophysical Journal · doi:10.1086/310516 · Cited by 250
Cited by
The Aquarius Project: the subhaloes of galactic haloes
Springel, V., Wang, J., Vogelsberger, M., Ludlow, A., Jenkins, A., 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 1,889
Triaxial Modeling of Halo Density Profiles with High‐Resolution N‐Body Simulations
Jing, Y. P., & Suto, Y. (2002) · The Astrophysical Journal · doi:10.1086/341065 · Cited by 855
Self-citationThe Mass Distribution of SDSS J1004$+$4112 Revisited
Oguri, M. (2010) · Publications of the Astronomical Society of Japan · doi:10.1093/pasj/62.4.1017 · Cited by 347
The First Cosmic Structures and Their Effects
Ciardi, B., & Ferrara, A. (2005) · Space Science Reviews · doi:10.1007/s11214-005-3592-0 · Cited by 345
The Phase‐Space Density Profiles of Cold Dark Matter Halos
Taylor, J. E., & Navarro, J. F. (2001) · The Astrophysical Journal · doi:10.1086/324031 · Cited by 324
Metadata
- Authors
- Jing, Y. P., & Suto, Y.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 2000-02-01
- Volume
- 529
- Issue
- 2
- Pages
- L69-L72
- ISSN
- 0004-637X (ISSN-L)
- OpenAlex
- W2949078855
- Cited by
- 423
- References
- 20
- FWCI
- 33.59
- Type
- journal article
- Language
- en
- Open access
- bronze
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
How to cite
Cite CoChat for the checks on this page, and the paper for its own findings.
- This page
- CoChat. (2026). Citation check: The Density Profiles of the Dark Matter Halo Are Not Universal. https://app.cochat.ai/papers/10.1086/312463
- The paper
- Jing, Y. P., & Suto, Y. (2000). The Density Profiles of the Dark Matter Halo Are Not Universal. The Astrophysical Journal. https://doi.org/10.1086/312463
Data sources
Bibliographic data: Semantic Scholar, OpenAlex, Crossref.
Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.