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Maximal neutron star mass and the resolution of the hyperon puzzle in modified gravity

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Astashenok, Artyom V., Capozziello, Salvatore, Odintsov, Sergei D.·2014·Physical Review D

Abstract

The so-called ``hyperon puzzle'' in the theory of neutron stars is considered in the framework of modified $f(R)$ gravity. We show that for simple hyperon equations of state, it is possible to obtain the maximal neutron star mass which satisfies the recent observational data for PSR J1614-2230, in higher-derivative models with power-law terms as $f(R)=R+\ensuremath{\gamma}{R}^{2}+\ensuremath{\beta}{R}^{3}$. The soft hyperon equation of state under consideration is usually treated as unrealistic in the standard general relativity. The numerical analysis of the mass-radius relation for massive neutron stars with a hyperon equation of state in modified gravity turns out to be consistent with observations. Thus, we show that the same modified gravity can solve at once three problems: a consistent description of the maximal mass of a neutron star, a realistic mass-radius relation, and a method to account for hyperons in the equation of state.

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Metadata

Authors
Astashenok, A. V., Capozziello, S., & Odintsov, S. D.
Venue
Physical Review D
Published
2014-05-08
Volume
89
Issue
10
ISSN
  • 0556-2821 (ISSN-L)
  • 1550-7998
  • 1550-2368
OpenAlex
W2079584683
Cited by
255
References
7
FWCI
10.73
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: Maximal neutron star mass and the resolution of the hyperon puzzle in modified gravity. https://app.cochat.ai/papers/10.1103/physrevd.89.103509
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Astashenok, A. V., Capozziello, S., & Odintsov, S. D. (2014). Maximal neutron star mass and the resolution of the hyperon puzzle in modified gravity. Physical Review D. https://doi.org/10.1103/physrevd.89.103509

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

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