The ground state of 17Na decays by three-proton emission at 2.24 MeV via a sequential path through 16Ne, and mirror energy differences decrease systematically in 3p emitters, indicating enhanced isospin symmetry breaking.
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Two-proton emitters with diproton-correlated initial states can deliver spin-entangled proton pairs exceeding local-hidden-variable bounds in democratic three-body emission.
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.
citing papers explorer
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Ground State Decay of the Three-Proton Emitter $^{17}$Na Reveals Isospin Symmetry Breaking
The ground state of 17Na decays by three-proton emission at 2.24 MeV via a sequential path through 16Ne, and mirror energy differences decrease systematically in 3p emitters, indicating enhanced isospin symmetry breaking.
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Two-proton emission as source of spin-entangled proton pairs
Two-proton emitters with diproton-correlated initial states can deliver spin-entangled proton pairs exceeding local-hidden-variable bounds in democratic three-body emission.
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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.