Further explorations of Skyrme-Hartree-Fock-Bogoliubov mass formulas. II: Role of the effective mass
arXiv:nucl-th/0311086 · doi:10.1103/PhysRevC.68.054325
Abstract
We have constructed four new complete mass tables, referred to as HFB-4 to HFB-7, each one including all the 9200 nuclei lying between the two drip lines over the range of Z and N>8 and Z<120. HFB-4 and HFB-5 have the isoscalar effective mass M*_s$ constrained to the value 0.92 M, with the former having a density-independent pairing, and the latter a density-dependent pairing. HFB-6 and HFB-7 are similar, except that M*_s is constrained to 0.8 M. The rms errors of the mass-data fits are 0.680, 0.675, 0.686, and 0.676 MeV, respectively, almost as good as for the HFB-2 mass formula, for which M*_s was unconstrained. However, as usual, the single-particle spectra depend significantly on M*_s. This decoupling of the mass fits from the fits to the single-particle spectra has been achieved only by making the cutoff parameter of the delta-function pairing force a free parameter. An improved treatment of the center-of-mass correction was adopted, but although this makes a difference to individual nuclei it does not reduce the overall rms error of the fit. The extrapolations of all four new mass formulas out to the drip lines are essentially the same as for the original HFB-2 mass formula.
arXiv comment12 pages revtex, 9 eps figures, accepted for publication in Phys. Rev. C
References in corpus (7)
- Nuclear Ground-State Masses and Deformations
- The equation of state for nucleon matter and neutron star structure
- Asymmetric Nuclear Matter from Extended Brueckner-Hartree-Fock Approach
- Gamow-Teller strength and the spin-isospin coupling constants of the Skyrme energy functional
- Interplay of Three-Body Interactions in the EOS of Nuclear Matter
- Effective density dependent pairing forces in the T=1 and T=0 channels
- Consequences of the center-of-mass correction in nuclear mean-field models
Cited by in corpus (71)
- The r-process of stellar nucleosynthesis: Astrophysics and nuclear physics achievements and mysteries
- Skyrme Interaction and Nuclear Matter Constraints
- Further explorations of Skyrme-Hartree-Fock-Bogoliubov mass formulas. XII: Stiffness and stability of neutron-star matter
- Exotic modes of excitation in atomic nuclei far from stability
- Nuclear Energy Density Optimization
- Nuclear energy density optimization: Large deformations
- The tensor part of the Skyrme energy density functional. I. Spherical nuclei
- Microscopic HFB+QRPA predictions of dipole strength for astrophysics applications
- Symmetry Energy II: Isobaric Analog States
- Symmetry Energy I: Semi-Infinite Matter
- Nuclear constraints on properties of neutron star crusts
- Axially Deformed Solution of the Skyrme-Hartree-Fock-Bogolyubov Equations using The Transformed Harmonic Oscillator Basis. The program HFBTHO (v1.66p)
- The outer crust of non-accreting cold neutron stars
- Higher-order effects on the incompressibility of isospin asymmetric nuclear matter
- Relativistic mean field interaction with density dependent meson-nucleon vertices based on microscopical calculations
- Global study of quadrupole correlation effects
- Isovector splitting of nucleon effective masses, ab-initio benchmarks and extended stability criteria for Skyrme energy functionals
- Further explorations of Skyrme-Hartree-Fock-Bogoliubov mass formulas. IX: Constraint of pairing force to neutron-matter gap
- From Brueckner Approach to Skyrme-type Energy Density Functional
- Self-Consistent Description of Multipole Strength in Exotic Nuclei I: Method
- High-precision mass measurements of nickel, copper, and gallium isotopes and the purported shell closure at N=40
- Further explorations of Skyrme-Hartree-Fock-Bogoliubov mass formulas. III: Role of particle-number projection
- Databases and tools for nuclear astrophysics applications BRUSsels Nuclear LIBrary (BRUSLIB), Nuclear Astrophysics Compilation of REactions II (NACRE II) and Nuclear NETwork GENerator (NETGEN)
- r-Process Calculations and Galactic Chemical Evolution
- From finite nuclei to the nuclear liquid drop: leptodermous expansion based on the self-consistent mean-field theory
- Dipole polarizability of 120Sn and nuclear energy density functionals
- Photodisintegration of Ultra-High-Energy Cosmic Rays revisited
- Surface Symmetry Energy of Nuclear Energy Density Functionals
- Properties of heaviest nuclei with and
- BCS-BEC crossover of neutron pairs in symmetric and asymmetric nuclear matter
- Fitting theories of nuclear binding energies
- Application of the RMF mass model to the r-process and the influence of mass uncertainties
- The many facets of the (non relativistic) Nuclear Equation of State
- Adiabatic fission barriers in superheavy nuclei
- A Minimal Nuclear Energy Density Functional
- Single-nucleon potential decomposition of the nuclear symmetry energy
- Microscopic study of 240Pu, mean-field and beyond
- Systematics of quadrupolar correlation energies
- First observation of low-energy γ-ray enhancement in the rare-earth region
- Crustal heating in accreting neutron stars from the nuclear energy-density functional theory. I. Proton shell effects and neutron-matter constraint
- Isospin Dependence in the Odd-Even Staggering of Nuclear Binding Energies
- Skyrme-Hartree-Fock-Bogoliubov mass models on a 3D mesh: II. Time-reversal symmetry breaking
- New analysis method of the halo phenomenon in finite many-fermion systems. First applications to medium-mass atomic nuclei
- Q-alpha values in superheavy nuclei from the deformed Woods-Saxon model
- Experimentally constrained ()Y and ()Y reaction rates relevant to the -process nucleosynthesis
- Constraining the surface properties of effective Skyrme interactions
- Nuclear Masses and Neutron Stars
- Compiled Properties of Nucleonic Matter and Nuclear and Neutron Star Models from Non-Relativistic and Relativistic Interactions
- Adjustment studies in self-consistent relativistic mean-field models
- Large-Scale Self-Consistent Nuclear Mass Calculations
- Exploration of a modified density dependence in the Skyrme functional
- Correlation energies by the generator coordinate method: computational aspects for quadrupolar deformations
- Extended Skyrme pseudo-potential deduced from infinite matter properties
- Nuclear energy density functional from chiral pion-nucleon dynamics revisited
- Candidates for Long Lived High-K Ground States in Superheavy Nuclei
- Skyrme-Hartree-Fock-Bogoliubov mass models on a 3D mesh. IIb. Fission properties of BSkG2
- Energy systematics of heavy nuclei -- mean field models in comparison
- Nuclear matter properties, phenomenological theory of clustering at the nuclear surface, and symmetry energy
- Accreting neutron stars from the nuclear energy-density functional theory. II. Equation of state and global properties
- Nuclear density-functional theory and fission of super-heavy elements
- Nuclear energy density functional from chiral pion-nucleon dynamics: Isovector terms
- Nuclear structure far from stability
- Role of the Symmetry Energy on the Structure of Neutron Stars with Unified Equations of State
- The nuclear symmetry energy and other isovector observables from the point of view of nuclear structure
- Properties of N=90 Isotones within the Mean Field Perspective
- Impact of choices for center-of-mass correction energy on the surface energy of Skyrme energy density functionals
- Proton pygmy resonances: predictions for N=20 isotones
- Three-body Force Effects on the Properties of Neutron-rich Nuclear Matter
- Decomposition of EOS of Asymmetric Nuclear Matter into Different Spin-isospin Channels
- -delayed -proton decay in Zn: analysis of the charged-particle spectrum
- Single particle potentials of asymmetric nuclear matter in different spin-isospin channels