REVIEW 1 cited by
Relativistic models of the neutron-star matter equation of state
Not yet reviewed by Pith; the record is open.
This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.
SPECIMEN: schema-true, not a live event
T0 review · schema-true
One-sentence machine reading of the paper's core claim.
pith:XXXXXXXX · record.json · timestamp
Signed reviews
read the original abstract
Motivated by a recent astrophysical measurement of the pressure of cold matter above nuclear-matter saturation density, we compute the equation of state of neutron star matter using accurately calibrated relativistic models. The uniform stellar core is assumed to consist of nucleons and leptons in beta equilibrium; no exotic degrees of freedom are included. We found the predictions of these models to be in fairly good agreement with the measured equation of state. Yet the Mass-vs-Radius relations predicted by these same models display radii that are consistently larger than the observations.
Forward citations
Cited by 1 Pith paper
-
A relativistic mechanism for the enhanced isovector spin-orbit interaction suggested by parity-violating electron scattering experiments
An enhanced isovector tensor coupling in a covariant density functional fits both PREX-II and CREX weak-charge form-factor differences, acting through a strong isovector spin-orbit interaction.
Discussion (0). Continue with ORCID to comment.