Emulator-assisted Bayesian inference of an extended Skyrme EDF, jointly constrained by nuclear observables, ab initio calculations, and NICER data, produces posteriors yielding consistent neutron star crust and core properties with a provided multivariate Gaussian for bulk nuclear matter parameters.
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Bayesian NS EoS study using full nuclear posterior distributions and consistent crust modeling finds increased surface thickness and crustal moment of inertia relative to prior work.
Dispersive optical model analyses of 40Ca to 208Pb nuclei show neutron skin thickness rising stronger than linearly with asymmetry, consistent with GFMC He results and drip-line expectations.
citing papers explorer
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Emulator-Assisted Nuclear DFT Inference and Its Consequences for the Structure of Neutron Stars
Emulator-assisted Bayesian inference of an extended Skyrme EDF, jointly constrained by nuclear observables, ab initio calculations, and NICER data, produces posteriors yielding consistent neutron star crust and core properties with a provided multivariate Gaussian for bulk nuclear matter parameters.
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Properties of the neutron star crust informed by nuclear structure data
Bayesian NS EoS study using full nuclear posterior distributions and consistent crust modeling finds increased surface thickness and crustal moment of inertia relative to prior work.
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Dispersive-optical-model analysis of the asymmetry dependence of neutron skins
Dispersive optical model analyses of 40Ca to 208Pb nuclei show neutron skin thickness rising stronger than linearly with asymmetry, consistent with GFMC He results and drip-line expectations.