TL;DRAbstract
The equations of state of the neutron star matter are calculated in the relativistic mean-field approximation with different hyperon coupling constants. The properties of neutron stars are studied by solving the Oppenheimer–Volkoff equation. It manifests the properties of neutron stars — change explicitly as different hyperon coupling constants are concerned.
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The equations of state of the neutron star matter are calculated in the relativistic mean-field approximation with different hyperon coupling constants. The properties of neutron stars are studied by solving the Oppenheimer–Volkoff equation. It manifests the properties of neutron stars — change explicitly as different hyperon coupling constants are concerned.
Keywords
HyperonPhysicsNeutron starEquation of stateCoupling constantNuclear physicsMean field theoryNeutron
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