Abstract
In this work, the nuclear density distributions, size radii and elastic electron scattering form factors are calculated for proton-rich 8B, 17F, 17Ne, 23Al and 27P nuclei using the radial wave functions of Woods-Saxon potential. The parameters of such potential for nuclei under study are generated so as to reproduce the experimentally available size radii and binding energies of the last nucleons on the Fermi surface.
Highlights
The chosen radial wave functions are played a crucial role in understanding the nuclear structure in the aspect of nuclear sizes and radial distributions of nucleons in any nuclear system [1]
Due to very short lifetime of halo nuclei there is no ability to make tthe arget of them; such nuclei are studied in inverse kinematics [4]
Experimental matter rms radii are available through nucleus-nucleus scattering in Glauber model [6, 7], besides the proton rms radii can be obtained from charge-changing cross section [8]
Summary
The chosen radial wave functions are played a crucial role in understanding the nuclear structure in the aspect of nuclear sizes and radial distributions of nucleons in any nuclear system [1]. We undertook the calculation of rms radii, density distributions and elastic electron scattering form factors for proton-rich 8B, 17F, 17Ne, 23Al and 27P nuclei utilizing the realistic radial wave functions of WS potential.
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