Covariant density functional theory input for r-process simulations in actinides and superheavy nuclei: the ground state and fission properties
arXiv:2011.13368 · doi:10.1103/PhysRevC.102.054330
Abstract
The systematic investigation of the ground state and fission properties of even-even actinides and superheavy nuclei with from the two-proton up to two-neutron drip lines with proper assessment of systematic theoretical uncertainties has been performed for the first time in the framework of covariant density functional theory (CDFT). These results provide a necessary theoretical input for the r-process modeling in heavy nuclei and, in particular, for the study of fission recycling. Four state-of-the-art globally tested covariant energy density functionals (CEDFs), namely, DD-PC1, DD-ME2, NL3* and PC-PK1, representing the major classes of the CDFT models are employed in the present study. Ground state deformations, binding energies, two neutron separation energies, -decay values and half-lives and the heights of fission barriers have been calculated for all these nuclei. Theoretical uncertainties in these physical observables and their evolution as a function of proton and neutron numbers have been quantified and their major sources have been identified. Spherical shell closures at , and and the structure of the single-particle (especially, high-) states in their vicinities as well as nuclear matter properties of employed CEDFs are two major factors contributing into theoretical uncertainties. However, different physical observables are affected in a different way by these two factors. For example, theoretical uncertainties in calculated ground state deformations are affected mostly by former factor, while theoretical uncertainties in fission barriers depend on both of these factors.
28 pages, 18 figures, Physical Review C, in press
References in corpus (16)
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- Multi-messenger Observations of a Binary Neutron Star Merger
- Origin of the heavy elements in binary neutron-star mergers from a gravitational wave event
- New parametrization for the nuclear covariant energy density functional with point-coupling interaction
- Comprehensive nucleosynthesis analysis for ejecta of compact binary mergers
- Relativistic Nuclear Energy Density Functionals: adjusting parameters to binding energies
- Relativistic Mean-Field Hadronic Models under Nuclear Matter Constraints
- Neutron Star Mergers and Nucleosynthesis of Heavy Elements
- The dynamical mass ejection from binary neutron star mergers: Radiation-hydrodynamics study in general relativity
- Global performance of covariant energy density functionals: ground state observables of even-even nuclei and the estimate of theoretical uncertainties
- Microscopic description of complex nuclear decay: multimodal fission
- Pairing-induced speedup of nuclear spontaneous fission
- Global study of beyond-mean-field correlation energies in covariant energy density functional theory using a collective Hamiltonian method
- Optimizing the relativistic energy density functional with nuclear ground state and collective excitation properties
- Octupole deformation in the ground states of even-even actinides and superheavy nuclei
- Microscopic description of fission in superheavy nuclei with the parametrization D1M of the Gogny energy density functional