The DOI matches its Crossref record.
A Microscopic Interpretation of Neutron Star Structure
Abstract
Neutron star models have been constructed using representative (15) equations of state. The behavior of some of those macroscopic properties which are of observational or evolutionary significance is examined systematically. A simple analysis is given which connects the microscopic parameters (strength and range) of a nonrelativistic interaction with the macroscopic properties of a neutron star; this provides a simple way of understanding the systematic trends in the numerical results. Subject headings: dense matter - equation of state - stars: interiors - stars: neutron
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
Theory and Experiment in Gravitational Physics
Will, C. M. (2018) · doi:10.1017/9781316338612 · Cited by 3,637
Nucleosynthesis, neutrino bursts and γ-rays from coalescing neutron stars
Eichler, D., Livio, M., Piran, T., & Schramm, D. N. (1989) · Nature · doi:10.1038/340126a0 · Cited by 2,107
Tensor-multi-scalar theories of gravitation
Damour, T., & Esposito-Farese, G. (1992) · Classical and Quantum Gravity · doi:10.1088/0264-9381/9/9/015 · Cited by 1,016
The tensor-vector-scalar theory and its cosmology
Skordis, C. (2009) · Classical and Quantum Gravity · doi:10.1088/0264-9381/26/14/143001 · Cited by 184
Ġ/G and a cosmological acceleration of gravitationally compact bodies
Nordtvedt, K. (1990) · Physical Review Letters · doi:10.1103/physrevlett.65.953 · Cited by 93
Metadata
- Authors
- Arnett, W. D., & Bowers, R. L.
- Venue
- The Astrophysical Journal Supplement Series
- Publisher
- American Astronomical Society
- Published
- 1977-04
- Volume
- 33
- Pages
- 415
- ISSN
- 0067-0049 (ISSN-L)
- 1538-4365
- OpenAlex
- W2074442735
- Cited by
- 315
- References
- 0
- Type
- conference abstract
- Language
- en
- Open access
- closed
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 Microscopic Interpretation of Neutron Star Structure. https://app.cochat.ai/papers/10.1086/190434
- The paper
- Arnett, W. D., & Bowers, R. L. (1977). A Microscopic Interpretation of Neutron Star Structure. The Astrophysical Journal Supplement Series. https://doi.org/10.1086/190434
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.
