Abstract
The nuclear structure included the matter, proton and neutron densities of the ground state, the nuclear root-mean-square (rms) radii and elastic form factors of one neutron 23O and 24F halo nuclei have been studied by the two body model of within the harmonic oscillator (HO) and Woods-Saxon (WS) radial wave functions. The calculated results show that the two body model within the HO and WS radial wave functions succeed in reproducing neutron halo in these exotic nuclei. Moreover, the Glauber model at high energy has been used to calculated the rms radii and reaction cross section of these nuclei.
Highlights
One of the most exciting discoveries in the recent experimental progress using radioactive nuclear beams is the neutron halo in some light neutron-rich nuclei [1, 2]
The theory based on the relativistic mean filed (RMF) approximation predicts the existence of proton halo or proton skin structure in some proton-rich nuclei [3, 4] and experiments have subsequently observed some of the theoretical predictions [5, 6]
The nuclear structure including the matter, proton and neutron densities of the ground state, the nuclear rms radii and elastic form factors of one neutron 23O and 24F halo nuclei were studied by the two body model of within the harmonic oscillator (HO) and WS radial wave functions
Summary
One of the most exciting discoveries in the recent experimental progress using radioactive nuclear beams is the neutron halo in some light neutron-rich nuclei [1, 2]. Abdullah [11] used the two body model of (Core+n) within the radial wave functions of the cosh potential to investigate the ground state features such as the proton, neutron and matter densities, the rms nuclear proton, neutron, charge and mass radii of unstable neutron-rich 14B, 15C, 19C and 22N nuclei. Abdullah [12] used the radial wave functions of the Bear–Hodgson potential to study the ground state features such as the proton, neutron and matter densities and the associated rms radii of two neutrons halo 6He, 11Li, 14Be and 17B nuclei. The WS and HO potentials wave functions will be used within the two-body model of (core + n) to study the nuclear structure including the matter, proton and neutron densities of the ground state, the nuclear root-mean-square (rms) radii and elastic form factors of one neutron 23O and 24F halo nuclei.
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