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.
Schunck, ed.,Energy Density Functional Methods for Atomic Nuclei, 2053-2563 (IOP Publishing, 2019)
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Neutron pairing gaps in calcium isotopes are insensitive to variations in third-order chiral interactions, indicating that nuclear superfluidity requires improved many-body modeling or higher-order terms.
Gaussian-folded finite-range pairing functionals stabilize nuclear DFT calculations in extended model spaces containing continuum states.
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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Chiral interactions and superfluidity in the calcium isotopic chain
Neutron pairing gaps in calcium isotopes are insensitive to variations in third-order chiral interactions, indicating that nuclear superfluidity requires improved many-body modeling or higher-order terms.
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Finite-range pairing in nuclear density functional theory
Gaussian-folded finite-range pairing functionals stabilize nuclear DFT calculations in extended model spaces containing continuum states.