Theoretical study of the two-proton halo candidate Ne including contributions from resonant continuum and pairing correlations
arXiv:1105.0504 · doi:10.1140/epja/i2013-13077-8
Abstract
With the relativistic Coulomb wave function boundary condition, the energies, widths and wave functions of the single proton resonant orbitals for Ne are studied by the analytical continuation of the coupling constant (ACCC) approach within the framework of the relativistic mean field (RMF) theory. Pairing correlations and contributions from the single-particle resonant orbitals in the continuum are taken into consideration by the resonant Bardeen-Cooper-Schrieffer (BCS) approach, in which constant pairing strength is used. It can be seen that the fully self-consistent calculations with NL3 and NLSH effective interactions mostly agree with the latest experimental measurements, such as binding energies, matter radii, charge radii and densities. The energy of 2s orbital is slightly higher than that of orbital, and the occupation probability of the 2s orbital is about 20%, which are in accordance with the shell model calculation and three-body model estimation.
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- Neutron halo in deformed nuclei
- First Penning-trap mass measurement in the millisecond half-life range: the exotic halo nucleus 11Li
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Cited by in corpus (5)
- Halos in medium-heavy and heavy nuclei with covariant density functional theory in continuum
- Green's function method for the single-particle resonances in a deformed Dirac equation
- Green's function method for the spin and pseudospin symmetries in the single-particle resonant states
- Study of single-particle resonant states with Green's function method
- Particle number conserving BCS approach in the relativistic mean field model and its application to Ca