In the chiral confining model, in-medium nucleon mass evolution driven by scalar-field response and separation of confinement versus chiral effects governs repulsive three-body forces for saturation, alongside changes to internal energy and pressure distributions.
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The IdylliQ model uses quark saturation to generate stiff equations of state and effective baryon repulsions that mitigate hyperon softening in neutron star matter.
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Mechanical properties of the nucleon in the chiral confining model. II -- in-medium evolution of the nucleon properties
In the chiral confining model, in-medium nucleon mass evolution driven by scalar-field response and separation of confinement versus chiral effects governs repulsive three-body forces for saturation, alongside changes to internal energy and pressure distributions.
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A quarkyonic matter model
The IdylliQ model uses quark saturation to generate stiff equations of state and effective baryon repulsions that mitigate hyperon softening in neutron star matter.