{ "id": "2308.08001", "version": "v1", "published": "2023-08-15T19:27:59.000Z", "updated": "2023-08-15T19:27:59.000Z", "title": "Constraints on the Nuclear Symmetry Energy from Experiments, Theory and Observations", "authors": [ "James M. Lattimer" ], "comment": "Compact Stars in the QCD Phase Diagram (CSQCD) IX, Banff, Canada, 2022. arXiv admin note: substantial text overlap with arXiv:2301.03666", "journal": "Journal of Physics: Conference Series, Volume 2536, Issue 1, id.012009, 10 pp. (2023)", "doi": "10.1088/1742-6596/2536/1/012009", "categories": [ "nucl-th", "astro-ph.HE", "nucl-ex" ], "abstract": "Nuclear mass measurements and neutron matter theory tightly constrain the nuclear symmetry energy parameters $J$, $L$, $K_{sym}$ and $Q_{sym}$. Corroboration of these constraints on $J$ and $L$ can be found from measurements of the neutron skin thicknesses and dipole polarizabilities of neutron-rich nuclei. The experimental constraints on these parameters are compared with those obtained from consideration of astrophysical measurements of the neutron star radius, which we show is highly correlated with $L$. Attention is aimed at the recent PREX and CREX neutron skin measurements from Jefferson Lab, NICER neutron star radius measurements, and a new interpretation of the GW170817 tidal deformability measurement. We find joint satisfaction of PREX and CREX gives $J=32.2\\pm1.7$ MeV and $L=52.9\\pm13.2$ MeV, in excellent agreement with neutron matter predictions of $J=32.0\\pm1.1$ MeV and $L=51.9\\pm7.9$ MeV.", "revisions": [ { "version": "v1", "updated": "2023-08-15T19:27:59.000Z" } ], "analyses": { "keywords": [ "constraints", "nicer neutron star radius measurements", "gw170817 tidal deformability measurement", "neutron matter theory tightly constrain", "nuclear symmetry energy parameters" ], "tags": [ "journal article" ], "publication": { "publisher": "IOP" }, "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable" } } }