The surface properties of neutron-rich exotic nuclei within relativistic mean field formalisms
arXiv:1802.03476 · doi:10.1103/PhysRevC.97.024322
Abstract
In this theoretical study, we establish a correlation between the neutron skin thickness and the nuclear symmetry energy for the eveneven isotopes of Fe, Ni, Zn, Ge, Se and Kr within the framework of the axially deformed self-consistent relativistic mean field for the non-linear NL3 and density-dependent DD-ME1 interactions. The coherent density functional method is used to formulate the symmetry energy, the neutron pressure and the curvature of finite nuclei as a function of the nuclear radius. We have performed broad studies for the mass dependence on the symmetry energy in terms of the neutron-proton asymmetry for mass 70 A 96. From this analysis, we found a notable signature of a shell closure at = 50 in the isotopic chains of Fe, Ni, Zn, Ge, Se and Kr nuclei. The present study reveals an interrelationship between the characteristics of infinite nuclear matter and the neutron skin thickness of finite nuclei
13 Pages, 07 Figures, and 03 Tables
References in corpus (30)
- Relativistic Continuum Hartree Bogoliubov Theory for Ground State Properties of Exotic Nuclei
- Theory of Core-Collapse Supernovae
- Nuclear symmetry energy probed by neutron skin thickness of nuclei
- Exotic modes of excitation in atomic nuclei far from stability
- Relativistic Nuclear Energy Density Functionals: adjusting parameters to binding energies
- Relativistic Mean-Field Hadronic Models under Nuclear Matter Constraints
- Neutron skin of 208Pb, nuclear symmetry energy, and the parity radius experiment
- The Giant Dipole Resonance as a quantitative constraint on the symmetry energy
- Neutron and Proton Transverse Emission Ratio Measurements and the Density Dependence of the Asymmetry Term of the Nuclear Equation of State
- Density dependence of the nuclear symmetry energy: a microscopic perspective
- Neutron skin thickness in droplet model with surface width dependence: indications of softness of the nuclear symmetry energy
- Incompressibility of neutron-rich matter
- Surface Symmetry Energy of Nuclear Energy Density Functionals
- Neutron skin thickness of heavy nuclei with -particle correlations and the slope of the nuclear symmetry energy
- Analysis of bulk and surface contributions in the neutron skin of nuclei
- Nuclear skin emergence in Skyrme deformed Hartree-Fock calculations
- The structural evolution in transitional nuclei of mass 80 A 132
- Folding model study of the isobaric analog excitation: isovector density dependence, Lane potential and nuclear symmetry energy
- Low energy graphene edge termination via small diameter nanotube formation
- Relativistic mean field study of the properties of Z=117 nucleus and the decay chains of 117 isotopes
- Superdeformed and Hyperdeformed States in Z=122 Isotopes
- Symmetry and Surface Symmetry Energies in Finite Nuclei
- The neutron skin of Pb and the density dependence of the symmetry energy
- Influence of the single-particle structure on the nuclear surface and the neutron skin
- Nuclear symmetry energy effects on neutron stars properties
- Correlations between bulk parameters in relativistic and nonrelativistic hadronic mean-field models
- Proton-skins in momentum space and neutron-skins in coordinate space in heavy nuclei
- Thermal properties of the nuclear surface
- Neutron Skin and Giant Resonances in Nuclei
- Determining the density dependence of the nuclear symmetry energy using heavy-ion reactions
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