Proton and neutron skins of light nuclei within the Relativistic Mean Field theory
arXiv:nucl-th/0309009 · doi:10.1016/j.nuclphysa.2003.10.014
Abstract
The Relativistic Mean Field (RMF) theory is applied to the analysis of ground-state properties of Ne, Na, Cl and Ar isotopes. In particular, we study the recently established proton skin in Ar isotopes and neutron skin in Na isotopes as a function of the difference between the proton and the neutron separation energy. We use the TMA effective interaction in the RMF Lagrangian, and describe pairing correlation by the density-independent delta-function interaction. We calculate single neutron and proton separation energies, quadrupole deformations, nuclear matter radii and differences between proton radii and neutron radii, and compare these results with the recent experimental data.
the version to be published in Nuclear Physics A
References in corpus (1)
Cited by in corpus (13)
- Two-Proton Radioactivity with 2p halo in light mass nuclei A1834
- Alpha-decay chains of and in the Relativistic Mean Field theory
- Proton and neutron skins and symmetry energy of mirror nuclei
- Odd-even staggering and shell effects of charge radii for nuclei with even from to and from to
- Study of Decay Modes in Transfermium Isotopes
- Structural Properties and -Decay Chains of Transfermium Nuclei (101Z110)
- Structural properties and decay modes of Z 122, 120 and 118 superheavy nuclei
- Microscopic study of the Shell Structure evolution in isotopes of light to middle mass range Nuclides
- Charge radii of potassium isotopes in the RMF(BCS)* approach
- Neutron drip line of isotopic chains
- Prediction of two-neutron halos in the isotones Mg and Na
- A systematic study of neutron magic nuclei with N = 8, 20, 28, 50, 82, and 126 in the relativistic mean field theory
- Novel feature of doubly bubble nuclei in 50Z(N)82 region along with magicity and weakly bound structure