2010
DOI: 10.1016/j.nuclphysa.2010.01.052
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Measurements of nuclear radii for neutron-rich Ne isotopes 28−32Ne

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Cited by 33 publications
(42 citation statements)
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“…Indeed, such a structure has been suggested for this isotope by Coulomb breakup studies [22]. This has been further supported by measurements [39] of the interaction cross sections for Ne isotopes incident on a 12 C target at the beam energy of 240 MeV/nucleon, where it was found that for 31 Ne the interaction cross section was much larger than that of any other Ne isotope. Recently, measurements of σ R for 24−38 Mg isotopes on 12 C target at the beam energy of 240 MeV/nucleon have been reported in Ref.…”
Section: Introductionmentioning
confidence: 54%
“…Indeed, such a structure has been suggested for this isotope by Coulomb breakup studies [22]. This has been further supported by measurements [39] of the interaction cross sections for Ne isotopes incident on a 12 C target at the beam energy of 240 MeV/nucleon, where it was found that for 31 Ne the interaction cross section was much larger than that of any other Ne isotope. Recently, measurements of σ R for 24−38 Mg isotopes on 12 C target at the beam energy of 240 MeV/nucleon have been reported in Ref.…”
Section: Introductionmentioning
confidence: 54%
“…They interpreted the large value of Coulomb breakup cross section by considering the valence neutron in 2p 3/2 (for S n ≈ 0.4 MeV) or 2s 1/2 (for S n ≤ 0.8 MeV) and not in 1f 7/2 , as one would have expected from a standard shell model configuration. Recently, Takechi et al, [12,13] measured the interaction cross section, σ I , of 28−32 Ne on 12 C target at 240 MeV/u. They also explained the large value of σ I of 31 Ne by considering sor p-wave valence neutron [13], which is consistent with Ref.…”
Section: Introductionmentioning
confidence: 99%
“…The ground state spin-parity suggested was 3/2 − corresponding to core deformation parameter β 2 ≈ 0.2, even though there was a possibility of J π = 1/2 + with β 2 ≈ 1 or β 2 ≈ −0.4. Takechi et al [21], also analyzed the data [12] by considering the single particle levels in a deformed potential. Using the β 2 value (0.6 ± 0.2) of the core, deduced from the experimental B(E2) data [6], it was suggested that 31 Ne has s-or p-orbital halo structure corresponding to Nilsson level [200 1/2] or [321 3/2], respectively.…”
Section: Introductionmentioning
confidence: 99%
“…[9] while we evaluate The experimental data for the reaction cross sections are taken from Ref. [9], while the empirical separation energies are taken from Refs. [41] and [42].…”
Section: Odd-even Staggering Of Reaction Cross Sectionsmentioning
confidence: 99%
“…Experimentally large odd-even staggering (OES) phenomena have been revealed in reaction cross sections of unstable nuclei close to the neutron drip line, for example, in the isotopes 14,15,16 C [8], 18,19,20 C [3], 28,29,30 Ne [9], 30,31,32 Ne [9], and 36,37,38 Mg [10]. In Ref.…”
Section: Introductionmentioning
confidence: 99%