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Kuchta, R.

doi:10.1103/physrevc.38.1460

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Cited by 11 publications

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“…The elastic form factors of exotic 23 O and 24 F nuclei (red curves) calculated by PWBA using the WS and HO proton densities are compared in Fig. 4 with those for their stable 18 O and 19 F isotopes (dark-blue curves) together with the experimental data (dark-blue symbol) of stable isotopes [27,28]. It is noted that the form factors for each isotopes pairs are quite different although they have the same proton number.…”

Section: Resultsmentioning

confidence: 99%

Study of the nuclear structure of halo nuclei 23O and 24F using the two-body model

Sallh

Abdullah

2020

IJP

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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.

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