Skyrme-Hartree-Fock-Bogoliubov mass models on a 3D mesh. IIb. Fission properties of BSkG2
Wouter Ryssens, Guillaume Scamps, Stephane Goriely, Michael Bender

TL;DR
This paper extends the BSkG2 nuclear model to accurately predict fission barriers of actinide nuclei by incorporating symmetry breaking and complex deformations, achieving high precision in modeling nuclear properties.
Contribution
The paper introduces an advanced 3D Skyrme-Hartree-Fock-Bogoliubov model that includes symmetry breaking and deformation effects for improved fission property predictions.
Findings
Accurately reproduces fission barriers of 45 actinide nuclei.
Achieves rms deviations below 500 keV for barrier and isomer energies.
Demonstrates the importance of symmetry breaking and complex shapes in modeling.
Abstract
Large-scale models of nuclear structure are currently the only way to provide consistent datasets for the many properties of thousands of exotic nuclei that are required by nucleosynthesis simulations. In [W.Ryssens et al., Eur. Phys. J. A 58, 246 (2022)], we recently presented the new BSkG2 model based on an energy density functional of the Skyrme type. Relying on a flexible three-dimensional coordinate representation of the nucleus, the model takes into account both triaxial deformation and time-reversal symmetry breaking. BSkG2 achieves a state-of-the-art global description of nuclear ground state (g.s.) properties and reproduces in particular the known masses with a root-mean-square (rms) deviation of 678 keV. Moving beyond g.s. properties, the model also reproduces all empirical values for the primary and secondary barriers as well as isomer excitation energies of actinide nuclei…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsNuclear physics research studies · Astronomical and nuclear sciences · Quantum Chromodynamics and Particle Interactions
