Spectroscopic factors in dripline nuclei

33Cl Spectroscopic Factors via the 32S(3He, d)33Cl One-Proton Transfer Reaction

“…The investigation of nuclear reactions at low and intermediate energies has a paramount importance to understand the atomic nucleus. It allows to investigate the detailed properties of the structure of nuclear systems [1,2,3], the occurrence of continuum effects [4,5,6], the appearance of exotic configurations [7], clustering phenomena [8,9,10,11] [12,13,14]. Another important aspect observed in nucleus-nucleus collisions concerns their dynamical evolution [15,16,17,18], and the interplay between structure and dynamics [19,20].…”

Investigation of spectroscopic factors of deeply-bound nucleons in drip-line nuclei with the Gamow shell model

“…This is in contrast with medium and heavy nuclei at proton drip-line, which are confined by the Coulomb barrier and hence are very long-lived [11,12]. Many neutron halos, of one neutron or two-neutron character, have been identified in the nuclear chart: for example, 11 Be, 15 C, 19 C and 23 O for the former and 6 He, 11 Li, 14 Be, 17 B, 22 C, 29 F, and possibly 31 F, for the latter [13]. Proton halos also exist, even though they are in smaller number than neutron halos, e.g.…”

The nuclear shell model towards the drip lines

“…will be reduced from unity. This effect should be contained in ab-inito and continuum models [43], [44], but an understanding within these models requires an explicit separation of the one-nucleon removal overlaps in terms of the removed nucleon within the basis states for (A, Z) and the radial overlaps between the nuclei with (A) and (A − 1).…”