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The Maximum Mass of a Neutron Star

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Kalogera, Vassiliki, Baym, Gordon·1996·The Astrophysical Journal

Abstract

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 .

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Metadata

Authors
Kalogera, V., & Baym, G.
Venue
The Astrophysical Journal
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

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CoChat. (2026). Citation check: The Maximum Mass of a Neutron Star. https://app.cochat.ai/papers/10.1086/310296
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Kalogera, V., & Baym, G. (1996). The Maximum Mass of a Neutron Star. The Astrophysical Journal. https://doi.org/10.1086/310296

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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.