MR-SCDFT augments standard multireference DFT by using stochastic fields to create reference configurations and a projection-selection step, yielding lower ground-state energies, smaller proton radii, and softer bands than conventional MR-CDFT for 20Ne, 24Mg, and 28Si.
Evolution of shell structure in exotic nuclei.Rev
5 Pith papers cite this work. Polarity classification is still indexing.
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Three qubit mappings for VQE on nuclear shell model are compared for 10B and 12C, with SD mapping achieving 0.21% error on hardware for 10B ground state.
Analysis of transfer to continuum states in 16C(d,p)17C requires a large N=16 shell gap (>5 MeV) in 17C.
Review of experimental evidence and theoretical models for dineutron correlations in two-neutron halo nuclei and candidates beyond the drip line, including discussion of tetraneutron states.
Review highlighting ab initio calculations for heavy nuclei and dark matter-nucleus scattering to reduce nuclear uncertainties.
citing papers explorer
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Multireference Covariant Density Functional Theory with Stochastic Basis
MR-SCDFT augments standard multireference DFT by using stochastic fields to create reference configurations and a projection-selection step, yielding lower ground-state energies, smaller proton radii, and softer bands than conventional MR-CDFT for 20Ne, 24Mg, and 28Si.
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Qubit-efficient variational algorithm for nuclear structure
Three qubit mappings for VQE on nuclear shell model are compared for 10B and 12C, with SD mapping achieving 0.21% error on hardware for 10B ground state.
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Constraining the $N=16$ Shell Gap in $^{17}$C via Transfer to the Continuum in the $^{16}$C$(d,p)^{17}$C Reaction
Analysis of transfer to continuum states in 16C(d,p)17C requires a large N=16 shell gap (>5 MeV) in 17C.
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Dineutron clusters
Review of experimental evidence and theoretical models for dineutron correlations in two-neutron halo nuclei and candidates beyond the drip line, including discussion of tetraneutron states.
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Ab Initio Nuclear Theory for Heavy Nuclei and Its Application to Dark Matter-Nucleus Scattering
Review highlighting ab initio calculations for heavy nuclei and dark matter-nucleus scattering to reduce nuclear uncertainties.