The DOI matches its Crossref record.
A unified equation of state of dense matter and neutron star structure
Open accessAbstract
An equation of state (EOS) of neutron star matter, describing both the neutron star crust and the liquid core, is calculated. It is based on the effective nuclear interaction SLy of the Skyrme type, which is particularly suitable for the application to the calculation of the properties of very neutron rich matter (Chabanat et al. 1997, 1998). The structure of the crust, and its EOS, is calculated in the approximation, and under the assumption of the ground state composition. The crust-core transition is a very weakly first-order phase transition, with relative density jump of about one percent. The EOS of the liquid core is calculated assuming (minimal) npeμ composition. Parameters of static neutron stars are calculated and compared with existing observational data on neutron stars. The minimum and maximum masses of static neutron stars are and , respectively. Effects of rotation on the minimum and the maximum mass of neutron stars are briefly discussed.
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
Cited by
Physics of strongly magnetized neutron stars
Harding, A. K., & Lai, D. (2006) · Reports on Progress in Physics · doi:10.1088/0034-4885/69/9/r03 · Cited by 823
Spontaneous Scalarization of Black Holes and Compact Stars from a Gauss-Bonnet Coupling
Silva, H. O., Sakstein, J., Gualtieri, L., Sotiriou, T. P., & Berti, E. (2018) · Physical Review Letters · doi:10.1103/physrevlett.120.131104 · Cited by 624
Observation of Gravitational Waves from Two Neutron Star-Black Hole Coalescences
Abbott, R., Abbott, T. D., Abraham, S., Acernese, F., Ackley, K., Adams, A., Adams, C., Adhikari, R. X., Adya, V. B., Affeldt, C., et al. (2021) · Institutional Repository of Leibniz Universität Hannover (Leibniz Universität Hannover) · doi:10.15488/11385 · Cited by 609
Identifying a First-Order Phase Transition in Neutron-Star Mergers through Gravitational Waves
Bauswein, A., Bastian, N.-U. F., Blaschke, D. B., Chatziioannou, K., Clark, J. A., Fischer, T., & Oertel, M. (2019) · Physical Review Letters · doi:10.1103/physrevlett.122.061102 · Cited by 404
Metadata
- Authors
- Douchin, F., & Haensel, P.
- Venue
- Astronomy & Astrophysics
- Publisher
- EDP Sciences
- Published
- 2001-12
- Volume
- 380
- Issue
- 1
- Pages
- 151-167
- ISSN
- 0004-6361 (ISSN-L)
- 1432-0746
- OpenAlex
- W2103740830
- Cited by
- 1,294
- References
- 0
- FWCI
- 3.26
- 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: A unified equation of state of dense matter and neutron star structure. https://app.cochat.ai/papers/10.1051/0004-6361:20011402
- The paper
- Douchin, F., & Haensel, P. (2001). A unified equation of state of dense matter and neutron star structure. Astronomy & Astrophysics. https://doi.org/10.1051/0004-6361%3A20011402
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.