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Super-soft symmetry energy encountering non-Newtonian gravity in neutron stars

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.

preprint2009arXivOpen access
De-Hua WenBao-An LiLie-Wen Chen
astro-ph.COhep-phnucl-exgr-qcnucl-thastro-ph.SR
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Open access3 authors6 topics
Imported metadata coverageMissing code, dataset, citation and institution fields are tracked without dominating the paper.Details
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De-Hua WenBao-An LiLie-Wen Chen

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