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Maximum Mass of a Neutron Star
Abstract
On the basis of Einstein's theory of relativity, the principle of causality, and Le Chatelier's principle, it is here established that the maximum mass of the equilibrium configuration of a neutron star cannot be larger than $3.2{M}_{[m?]}$. The extremal principle given here applies as well when the equation of state of matter is unknown in a limited range of densities. The absolute maximum mass of a neutron star provides a decisive method of observationally distinguishing neutron stars from black holes.
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Citations
Cited by
GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence
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.116.241103 · Cited by 3,435
Harko, T., Lobo, F. S. N., Nojiri, S., & Odintsov, S. D. (2011) · Physical Review D · doi:10.1103/physrevd.84.024020 · Cited by 2,772
Quasinormal modes of black holes and black branes
Berti, E., Cardoso, V., & Starinets, A. O. (2009) · Classical and Quantum Gravity · doi:10.1088/0264-9381/26/16/163001 · Cited by 2,095
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
Binary 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
Metadata
- Authors
- Rhoades, C. E., & Ruffini, R.
- Venue
- Physical Review Letters
- Publisher
- American Physical Society (APS)
- Published
- 1974-02-11
- Volume
- 32
- Issue
- 6
- Pages
- 324-327
- ISSN
- 0031-9007 (ISSN-L)
- OpenAlex
- W2018944415
- Cited by
- 692
- References
- 0
- FWCI
- 7.34
- Type
- journal article
- Language
- en
- Open access
- closed
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- CoChat. (2026). Citation check: Maximum Mass of a Neutron Star. https://app.cochat.ai/papers/10.1103/physrevlett.32.324
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- Rhoades, C. E., & Ruffini, R. (1974). Maximum Mass of a Neutron Star. Physical Review Letters. https://doi.org/10.1103/physrevlett.32.324
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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.
