Super-soft symmetry energy encountering non-Newtonian gravity in neutron stars
Wen, De-Hua · Li, Bao-An · Chen, Lie-Wen
Nuclear Theory
Cosmology and Nongalactic Astrophysics
Solar and Stellar Astrophysics
General Relativity and Quantum Cosmology
High Energy Physics - Phenomenology
Nuclear Experiment
الأصل · EN
Considering the non-Newtonian gravity proposed in the grand unification theories, we show that the stability and observed global properties of neutron stars can not rule out the super-soft nuclear symmetry energies at supra-saturation densities. The degree of possible violation of the Inverse-Square-Law of gravity in neutron stars is estimated using an Equation of State (EOS) of neutron-rich nuclear matter consistent with the available terrestrial laboratory data.
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