Baryons' coupling constants in the Sigma-Omega-Rho model and the mass-radius relation of neutron stars in the presence of hyperons

DOI10.1016/J.AOP.2021.168665zbMath1483.85005OpenAlexW3213148800MaRDI QIDQ2063622

H. R. Moshfegh, Reza Raymond Karimi

Publication date: 11 January 2022

Published in: Annals of Physics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1016/j.aop.2021.168665

zbMATH Keywords

chemical potentialnuclear matterneutron starhyperon puzzleSigma-Omega-Rho model

Mathematics Subject Classification ID

Nuclear physics (81V35) Classical and relativistic thermodynamics (80A10) Galactic and stellar structure (85A15)

Cites Work

• Appearance of hyperons in neutron stars within LOCV method
• On Massive Neutron Cores
• Unnamed Item

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