Detailed illustration of accuracy of presently used nuclear-mass models
arXiv:1903.00886 · doi:10.1016/j.adt.2017.05.001
Abstract
The accuracy of description of measured nuclear masses by presently used nuclear-mass models is studied. Twelve models of various kinds are considered, eleven of the global character and one local model specially adapted to description of heavy nuclei. To decrease the number of nuclei over which the accuracy is averaged, the global region (Z,N >= 8) is divided into four subregions, in which the accuracy is studied separately. Still, to reach the best precision, the accuracy is finally investigated without any averaging, for each nucleus separately. The results are presented in a form of colored maps, large enough to be easily and accurately read. Besides the accuracy of the studied models, also their predictive power is considered. It is found that the accuracy of description of mass strongly depends on a nuclear-mass model and on the region of nuclei to which the model is applied. The best accuracy is obtained by the recent two Chinese models WS3+ and WS4+. Generally, no clear, strong correlation between the accuracy of description of already known masses by a given model and its predictive power for new masses is observed. Still, such correlation is found for separate models and in separate regions of nuclei. More often for the macroscopic-microscopic models than for the other approaches.
arXiv comment70 pages
References in corpus (16)
- Nuclear Ground-State Masses and Deformations
- Nuclear ground-state masses and deformations: FRDM(2012)
- Microscopic mass formulae
- Surface diffuseness correction in global mass formula
- Further explorations of Skyrme-Hartree-Fock-Bogoliubov mass formulas. XII: Stiffness and stability of neutron-star matter
- Further improvements on a global nuclear mass model
- Direct mapping of nuclear shell effects in the heaviest elements
- Nuclear mass predictions with radial basis function approach
- Precision Mass Measurements of 129-131Cd and Their Impact on Stellar Nucleosynthesis via the Rapid Neutron Capture Process
- The anatomy of the simplest Duflo-Zuker mass formula
- Living on the edge of stability, the limits of the nuclear landscape
- Storage ring mass spectrometry for nuclear structure and astrophysics research
- Identification of the Lowest , Isobaric Analog State in Co and Its Impact on the Understanding of -Decay Properties of Ni
- Schottky mass measurements of heavy neutron-rich nuclides in the element range $70\leZ \le79$ at the ESR
- Mass Predictions of Atomic Nuclei in the Infinite Nuclear Matter Model
- Nuclear Masses and Neutron Stars
Cited by in corpus (10)
- Current Status of r-Process Nucleosynthesis
- Isochronous mass measurements of -shell nuclei from projectile fragmentation of Ni
- Mass Measurements of Neutron-Deficient Y, Zr, and Nb Isotopes and Their Impact on and Nucleosynthesis Processes
- Mass measurements for -shell nuclei Ti, Cr, Mn, Fe, Co and Ni
- Distinguishing fission-like events from deep-inelastic collisions
- High Precision Binding Energies from Physics Informed Machine Learning
- Explosive Nucleosynthesis: What we learned and what we still do not understand
- Limitations of the Geiger-Nuttall Law in heavy cluster decay
- Further exploration of binding energy residuals using machine learning and the development of a composite ensemble model
- Bayesian model mixing with multi-reference energy density functional