The equation of state for compact stars made of hidden-sector nucleons is written analytically in one variable, and varying the scalar coupling changes the dimensionless maximum mass from 0.535 to 0.567, about twice the free-fermion value.
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Influence of EOS on compact star made of hidden sector nucleons
The equation of state for compact stars made of hidden-sector nucleons is written analytically in one variable, and varying the scalar coupling changes the dimensionless maximum mass from 0.535 to 0.567, about twice the free-fermion value.