The DOI matches its Crossref record.
The Maximum Mass of a Neutron Star
Open accessAbstract
Observational identification of black holes as members of binary systems requires the knowledge of the upper limit on the gravitational mass of a neutron star. We use modern equations of state for neutron star matter, fitted to experimental nucleon-nucleon scattering data and the properties of light nuclei, to calculate, within the framework of Rhoades & Ruffini (1974), the minimum upper limit on a neutron star mass. Regarding the equation of state as valid up to twice nuclear matter saturation density, ρ nm , we obtain a secure upper bound on the neutron star mass equal to 2.9 M ☉ . We also find that in order to reach the lowest possible upper bound of 2.2 M ☉ , we need to understand the physical properties of neutron matter up to a density of ~4ρ nm .
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
Abbott, R., Abbott, T. D., Acernese, F., Ackley, K., Adams, C., Adhikari, N., Adhikari, R. X., Adya, V. B., Affeldt, C., Agarwal, D., et al. (2023) · Physical Review X · doi:10.1103/physrevx.13.041039 · Cited by 1,754
Self-citationBinary Black Hole Mergers in the First Advanced LIGO Observing Run
Abbott, B. P., Abbott, R., Abbott, T. D., Abernathy, M. R., Acernese, F., Ackley, K., Adams, C., Adams, T., Addesso, P., Adhikari, R. X., et al. (2016) · Physical Review X · doi:10.1103/physrevx.6.041015 · Cited by 1,374
Self-citationProperties of the Binary Black Hole Merger GW150914
Abbott, B. P., Abbott, R., Abbott, T. D., Abernathy, M. R., Acernese, F., Ackley, K., Adams, C., Adams, T., Addesso, P., Adhikari, R. X., et al. (2016) · Physical Review Letters · doi:10.1103/physrevlett.116.241102 · Cited by 1,021
Self-citationPopulation of Merging Compact Binaries Inferred Using Gravitational Waves through GWTC-3
Abbott, R., Abbott, T. D., Acernese, F., Ackley, K., Adams, C., Adhikari, N., Adhikari, R. X., Adya, V. B., Affeldt, C., Agarwal, D., et al. (2023) · Physical Review X · doi:10.1103/physrevx.13.011048 · Cited by 889
Self-citationObservation 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
Self-citation
Metadata
- Authors
- Kalogera, V., & Baym, G.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 1996-10-10
- Volume
- 470
- Issue
- 1
- Pages
- L61-L64
- ISSN
- 0004-637X (ISSN-L)
- OpenAlex
- W1993030633
- Cited by
- 383
- References
- 0
- FWCI
- 6.16
- 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 Maximum Mass of a Neutron Star. https://app.cochat.ai/papers/10.1086/310296
- The paper
- Kalogera, V., & Baym, G. (1996). The Maximum Mass of a Neutron Star. The Astrophysical Journal. https://doi.org/10.1086/310296
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.